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19,300
1501.00661
Shi-Ju Ran
Shi-Ju Ran, Cheng Peng, Wei Li, and Gang Su
Identification of Degeneracy and Criticality of Two-Dimensional Statistical and Quantum Systems by the Boundary States of Tensor Networks
4+3 pages, 3+3 figures
null
null
null
cond-mat.str-el cond-mat.stat-mech physics.comp-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We propose a systematic scheme to reach the properties of two-dimensional (2D) statistical and quantum systems by studying the effective (1+1)-dimensional theory that is constructed from the tensor network representation. On on hand, we discover that the degeneracy of the 2D system can be determined by the purity of the boundary thermal state, which is the density operator of the effective theory at zero (effective) temperature. On the other hand, we find that the gapped (or critical) 2D system leads to a gapped (or critical) effective (1+1)-dimensional theory whose criticality can be accessed by the entanglement entropy $S$ of its ground state dubbed as boundary pure state. We also uncover that for the critical systems, $S$ obeys the same logarithmic law as that found in the critical 1D quantum chains, which reads $S = (\kappa c/6)\log_2 D + const.$, with $c$ the central charge and $\kappa$ a constant related to the scaling property of the correlation length $\xi$ as $\xi \sim D^{\kappa}$. Such a scaling law presents an efficient way to characterize the critical universality class of the original 2D systems. An important implication of our work is that many well-established theories for 1D quantum chains become available for studying 2D systems with the help of the proposed lower dimensional correspondence.
[{'version': 'v1', 'created': 'Sun, 4 Jan 2015 10:41:06 GMT'} {'version': 'v2', 'created': 'Tue, 20 Jan 2015 08:37:13 GMT'}]
2015-01-21
[array(['Ran', 'Shi-Ju', ''], dtype=object) array(['Peng', 'Cheng', ''], dtype=object) array(['Li', 'Wei', ''], dtype=object) array(['Su', 'Gang', ''], dtype=object)]
19,301
1802.08245
Satrya Fajri Pratama
Satrya Fajri Pratama, Azah Kamilah Muda, and Yun-Huoy Choo
Arbitrarily Substantial Number Representation for Complex Number
This is a published version of an article published in Journal of Telecommunication, Electronic and Computer Engineering, available online at: http://journal.utem.edu.my/index.php/jtec/article/view/3590
Journal of Telecommunication, Electronic and Computer Engineering (2018), 23-26
null
null
cs.NA
http://creativecommons.org/licenses/by/4.0/
Researchers are often perplexed when their machine learning algorithms are required to deal with complex number. Various strategies are commonly employed to project complex number into real number, although it is frequently sacrificing the information contained in the complex number. This paper proposes a new method and four techniques to represent complex number as real number, without having to sacrifice the information contained. The proposed techniques are also capable of retrieving the original complex number from the representing real number, with little to none of information loss. The promising applicability of the proposed techniques has been demonstrated and worth to receive further exploration in representing the complex number.
[{'version': 'v1', 'created': 'Thu, 22 Feb 2018 18:58:09 GMT'} {'version': 'v2', 'created': 'Fri, 23 Feb 2018 02:12:53 GMT'} {'version': 'v3', 'created': 'Mon, 2 Apr 2018 07:09:04 GMT'}]
2018-04-03
[array(['Pratama', 'Satrya Fajri', ''], dtype=object) array(['Muda', 'Azah Kamilah', ''], dtype=object) array(['Choo', 'Yun-Huoy', ''], dtype=object)]
19,302
1304.3042
Jean-Luc Marichal
Miguel Couceiro, Jean-Luc Marichal
Discrete integrals based on comonotonic modularity
null
Axioms 2 (3) (2013) 390-403
10.3390/axioms2030390
null
math.FA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
It is known that several discrete integrals, including the Choquet and Sugeno integrals as well as some of their generalizations, are comonotonically modular functions. Based on a recent description of the class of comonotonically modular functions, we axiomatically identify more general families of discrete integrals that are comonotonically modular, including signed Choquet integrals and symmetric signed Choquet integrals as well as natural extensions of Sugeno integrals.
[{'version': 'v1', 'created': 'Wed, 10 Apr 2013 18:16:25 GMT'} {'version': 'v2', 'created': 'Tue, 27 Aug 2013 11:13:31 GMT'}]
2013-08-28
[array(['Couceiro', 'Miguel', ''], dtype=object) array(['Marichal', 'Jean-Luc', ''], dtype=object)]
19,303
2001.06475
Mattia Halter
Mattia Halter, Laura B\'egon-Lours, Valeria Bragaglia, Marilyne Sousa, Bert Jan Offrein, Stefan Abel, Mathieu Luisier, Jean Fompeyriney
A back-end, CMOS compatible ferroelectric Field Effect Transistor for synaptic weights
14 pages, 5 figures, supplementary information available, submitted to ACS Applied Materials & Interfaces
null
10.1021/acsami.0c00877
null
cs.ET physics.app-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Neuromorphic computing architectures enable the dense co-location of memory and processing elements within a single circuit. This co-location removes the communication bottleneck of transferring data between separate memory and computing units as in standard von Neuman architectures for data-critical applications including machine learning. The essential building blocks of neuromorphic systems are non-volatile synaptic elements such as memristors. Key memristor properties include a suitable non-volatile resistance range, continuous linear resistance modulation and symmetric switching. In this work, we demonstrate voltage-controlled, symmetric and analog potentiation and depression of a ferroelectric Hf$_{57}$Zr$_{43}$O$_{2}$ (HZO) field effect transistor (FeFET) with good linearity. Our FeFET operates with a low writing energy (fJ) and fast programming time (40 ns). Retention measurements have been done over 4-bits depth with low noise (1%) in the tungsten oxide (WO$_{x}$) read out channel. By adjusting the channel thickness from 15nm to 8nm, the on/off ratio of the FeFET can be engineered from 1% to 200% with an on-resistance ideally >100 kOhm, depending on the channel geometry. The device concept is using earth-abundant materials, and is compatible with a back end of line (BEOL) integration into complementary metal-oxidesemiconductor (CMOS) processes. It has therefore a great potential for the fabrication of high density, large-scale integrated arrays of artificial analog synapses.
[{'version': 'v1', 'created': 'Fri, 17 Jan 2020 18:54:13 GMT'}]
2020-03-31
[array(['Halter', 'Mattia', ''], dtype=object) array(['Bégon-Lours', 'Laura', ''], dtype=object) array(['Bragaglia', 'Valeria', ''], dtype=object) array(['Sousa', 'Marilyne', ''], dtype=object) array(['Offrein', 'Bert Jan', ''], dtype=object) array(['Abel', 'Stefan', ''], dtype=object) array(['Luisier', 'Mathieu', ''], dtype=object) array(['Fompeyriney', 'Jean', ''], dtype=object)]
19,304
math/0502159
Satyan L. Devadoss
Suzanne M. Armstrong, Michael Carr, Satyan L. Devadoss, Eric Engler, Ananda Leininger, Michael Manapat
Particle Configurations and Coxeter Operads
25 pages, 18 figures; revision of Coxeter operads
Homotopy and Related Structures, Volume 4 (2009) 83-109.
null
null
math.GT math-ph math.MP math.QA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
There exist natural generalizations of the real moduli space of Riemann spheres based on manipulations of Coxeter complexes. These novel spaces inherit a tiling by the graph-associahedra convex polytopes. We obtain explicit configuration space models for the classical infinite families of finite and affine Weyl groups using particles on lines and circles. A Fulton-MacPherson compactification of these spaces is described and this is used to define the Coxeter operad. A complete classification of the building sets of these complexes is also given, along with a computation of their Euler characteristics.
[{'version': 'v1', 'created': 'Tue, 8 Feb 2005 15:21:49 GMT'} {'version': 'v2', 'created': 'Fri, 9 Dec 2005 20:54:51 GMT'} {'version': 'v3', 'created': 'Mon, 9 Mar 2009 18:19:10 GMT'}]
2009-08-27
[array(['Armstrong', 'Suzanne M.', ''], dtype=object) array(['Carr', 'Michael', ''], dtype=object) array(['Devadoss', 'Satyan L.', ''], dtype=object) array(['Engler', 'Eric', ''], dtype=object) array(['Leininger', 'Ananda', ''], dtype=object) array(['Manapat', 'Michael', ''], dtype=object)]
19,305
1910.12302
Nihal Yilmaz \"Ozg\"ur
Nihal \"Ozg\"ur and Nihal Ta\c{s}
Pata Zamfirescu Type Fixed-Disc Results with a Proximal Application
11 pages
null
null
null
math.MG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper is concerning to the geometric study of fixed points of a self-mapping on a metric space. We establish new generalized contractive conditions which ensure that a self-mapping has a fixed disc or a fixed circle. We introduce the notion of a best proximity circle and explore some proximal contractions for a non-self-mapping as an application. Necessary illustrative examples are presented to highlight the importance of the obtained results.
[{'version': 'v1', 'created': 'Sun, 27 Oct 2019 17:07:22 GMT'}]
2019-10-29
[array(['Özgür', 'Nihal', ''], dtype=object) array(['Taş', 'Nihal', ''], dtype=object)]
19,306
2004.12675
Toshihiko Hiraiwa
Toshihiko Hiraiwa, Kouichi Soutome and Hitoshi Tanaka
A Forced Harmonic Oscillator, Interpreted as Diffraction of Light
4 pages, 3 figures
Phys. Rev. E 102, 032211 (2020)
10.1103/PhysRevE.102.032211
null
physics.class-ph physics.optics
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate a simple forced harmonic oscillator with a natural frequency varying with time. It is shown that the time evolution of such a system can be written in a simplified form with Fresnel integrals, as long as the variation of the natural frequency is sufficiently slow compared to the time period of oscillation. Thanks to such a simple formulation, we found, for the first time, that a forced harmonic oscillator with a slowly-varying natural frequency is essentially equivalent to diffraction of light.
[{'version': 'v1', 'created': 'Mon, 27 Apr 2020 09:43:16 GMT'} {'version': 'v2', 'created': 'Tue, 14 Jul 2020 09:56:06 GMT'}]
2020-09-16
[array(['Hiraiwa', 'Toshihiko', ''], dtype=object) array(['Soutome', 'Kouichi', ''], dtype=object) array(['Tanaka', 'Hitoshi', ''], dtype=object)]
19,307
1908.08570
Ayush Maheshwari
Ayush Maheshwari, Kamal Kumar Murari, T. Jayaraman
Peak Electricity Demand and Global Warming in the Industrial and Residential areas of Pune : An Extreme Value Approach
20 pages, 6 figures, 2 tables
null
null
null
stat.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Industrial and residential activities respond distinctly to electricity demand on temperature. Due to increasing temperature trend on account of global warming, its impact on peak electricity demand is a proxy for effective management of electricity infrastructure. Few studies explore the relationship between electricity demand and temperature changes in industrial areas in India mainly due to the limitation of data. The precise role of industrial and residential activities response to the temperature is not explored in sub-tropical humid climate of India. Here, we show the temperature sensitivity of industrial and residential areas in the city of Pune, Maharashtra by keeping other influencing variables on electricity demand as constant. The study seeks to estimate the behaviour of peak electricity demand with the apparent temperature (AT) using the Extreme Value Theory. Our analysis shows that industrial activities are not much influenced by the temperature whereas residential activities show around 1.5-2% change in average electricity demand with 1 degree rise in AT. Further, we show that peak electricity demand in residential areas, performed using stationary and non-stationary GEV models, are significantly influenced by the rise in temperature. The study shows that with the improvement in data collection, better planning for the future development, accounting for the climate change effects, will enhance the effectiveness of electricity distribution system. The study is limited to the geographical area of Pune. However, the methods are useful in estimating the peak power load attributed to climate change to other geographical regions located in subtropical and humid climate.
[{'version': 'v1', 'created': 'Thu, 22 Aug 2019 19:17:34 GMT'}]
2019-08-26
[array(['Maheshwari', 'Ayush', ''], dtype=object) array(['Murari', 'Kamal Kumar', ''], dtype=object) array(['Jayaraman', 'T.', ''], dtype=object)]
19,308
1607.03363
Izabela Spaleniak
Izabela Spaleniak, David G. MacLachlan, Itandehui Gris-S\'anchez, Debaditya Choudhury, Robert J. Harris, Alexander Arriola, Jeremy R. Allington-Smith, Timothy A. Birks, Robert R. Thomson
Modal noise characterisation of a hybrid reformatter
9 pages, 9 figures, submitted to SPIE Astronomical Telescopes & Instrumentation 2016 (9912-78)
null
10.1117/12.2232708
null
physics.optics astro-ph.IM
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper reports on the modal noise characterisation of a hybrid reformatter. The device consists of a multicore-fibre photonic lantern and an ultrafast laser-inscribed slit reformatter. It operates around 1550 nm and supports 92 modes. Photonic lanterns transform a multimode signal into an array of single-mode signals, and thus combine the high coupling efficiency of multimode fibres with the diffraction-limited performance of single-mode fibres. This paper presents experimental measurements of the device point spread function properties under different coupling conditions, and its throughput behaviour at high spectral resolution. The device demonstrates excellent scrambling but its point spread function is not completely stable. Mode field diameter and mode barycentre position at the device output vary as the multicore-fibre is agitated due to the fabrication imperfections.
[{'version': 'v1', 'created': 'Mon, 11 Jul 2016 12:46:55 GMT'}]
2016-12-07
[array(['Spaleniak', 'Izabela', ''], dtype=object) array(['MacLachlan', 'David G.', ''], dtype=object) array(['Gris-Sánchez', 'Itandehui', ''], dtype=object) array(['Choudhury', 'Debaditya', ''], dtype=object) array(['Harris', 'Robert J.', ''], dtype=object) array(['Arriola', 'Alexander', ''], dtype=object) array(['Allington-Smith', 'Jeremy R.', ''], dtype=object) array(['Birks', 'Timothy A.', ''], dtype=object) array(['Thomson', 'Robert R.', ''], dtype=object)]
19,309
1711.05694
Stephen Green
J\'er\'emie Gagnon-Bischoff, Stephen R. Green, Philippe Landry, N\'estor Ortiz
Extended I-Love relations for slowly rotating neutron stars
31 pages, 6 figures, 9 tables; v2: updated to match published version
Phys. Rev. D 97, 064042 (2018)
10.1103/PhysRevD.97.064042
null
gr-qc astro-ph.HE
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Observations of gravitational waves from inspiralling neutron star binaries---such as GW170817---can be used to constrain the nuclear equation of state by placing bounds on stellar tidal deformability. For slowly rotating neutron stars, the response to a weak quadrupolar tidal field is characterized by four internal-structure-dependent constants called "Love numbers." The tidal Love numbers $k_2^\text{el}$ and $k_2^\text{mag}$ measure the tides raised by the gravitoelectric and gravitomagnetic components of the applied field, and the rotational-tidal Love numbers $\mathfrak{f}^\text{o}$ and $\mathfrak{k}^\text{o}$ measure those raised by couplings between the applied field and the neutron star spin. In this work we compute these four Love numbers for perfect fluid neutron stars with realistic equations of state. We discover (nearly) equation-of-state independent relations between the rotational-tidal Love numbers and the moment of inertia, thereby extending the scope of I-Love-Q universality. We find that similar relations hold among the tidal and rotational-tidal Love numbers. These relations extend the applications of I-Love universality in gravitational-wave astronomy. As our findings differ from those reported in the literature, we derive general formulas for the rotational-tidal Love numbers in post-Newtonian theory and confirm numerically that they agree with our general-relativistic computations in the weak-field limit.
[{'version': 'v1', 'created': 'Wed, 15 Nov 2017 17:41:20 GMT'} {'version': 'v2', 'created': 'Mon, 2 Apr 2018 17:27:38 GMT'}]
2018-04-03
[array(['Gagnon-Bischoff', 'Jérémie', ''], dtype=object) array(['Green', 'Stephen R.', ''], dtype=object) array(['Landry', 'Philippe', ''], dtype=object) array(['Ortiz', 'Néstor', ''], dtype=object)]
19,310
1606.07723
John M. Myers
John M. Myers, F. Hadi Madjid
Logical synchronization: how evidence and hypotheses steer atomic clocks
16 pages, 4 figures. arXiv admin note: substantial text overlap with arXiv:1407.8020
Proc. SPIE 9123, Quantum Information and Computation XII, 91230T (May 22, 2014)
10.1117/12.2054945
null
quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A clock steps a computer through a cycle of phases. For the propagation of logical symbols from one computer to another, each computer must mesh its phases with arrivals of symbols from other computers. Even the best atomic clocks drift unforeseeably in frequency and phase; feedback steers them toward aiming points that depend on a chosen wave function and on hypotheses about signal propagation. A wave function, always under-determined by evidence, requires a guess. Guessed wave functions are coded into computers that steer atomic clocks in frequency and position---clocks that step computers through their phases of computations, as well as clocks, some on space vehicles, that supply evidence of the propagation of signals. Recognizing the dependence of the phasing of symbol arrivals on guesses about signal propagation elevates `logical synchronization.' from its practice in computer engineering to a discipline essential to physics. Within this discipline we begin to explore questions invisible under any concept of time that fails to acknowledge the unforeseeable. In particular, variation of spacetime curvature is shown to limit the bit rate of logical communication.
[{'version': 'v1', 'created': 'Fri, 24 Jun 2016 15:29:27 GMT'}]
2016-06-27
[array(['Myers', 'John M.', ''], dtype=object) array(['Madjid', 'F. Hadi', ''], dtype=object)]
19,311
1103.0746
Ovidiu Munteanu
Ovidiu Munteanu and Jiaping Wang
Smooth metric measure spaces with non-negative curvature
24 pages, Theorem 4.1 has been improved
null
null
null
math.DG math.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study both function theoretic and spectral properties on complete noncompact smooth metric measure space $(M,g,e^{-f}dv)$ with nonnegative Bakry-\'{E}mery Ricci curvature. Among other things, we derive a gradient estimate for positive $f$-harmonic functions and obtain as a consequence the strong Liouville property under the optimal sublinear growth assumption on $f.$ We also establish a sharp upper bound of the bottom spectrum of the $f$-Laplacian in terms of the linear growth rate of $f.$ Moreover, we show that if equality holds and $M$ is not connected at infinity, then $M$ must be a cylinder. As an application, we conclude steady Ricci solitons must be connected at infinity.
[{'version': 'v1', 'created': 'Thu, 3 Mar 2011 18:02:46 GMT'} {'version': 'v2', 'created': 'Mon, 7 Mar 2011 20:38:23 GMT'}]
2011-03-08
[array(['Munteanu', 'Ovidiu', ''], dtype=object) array(['Wang', 'Jiaping', ''], dtype=object)]
19,312
quant-ph/0202162
Tobias J. Osborne
Tobias J. Osborne, Michael A. Nielsen
Entanglement in a simple quantum phase transition
14 pages, 7 eps figures
Phys. Rev. A 66, 032110 (2002)
10.1103/PhysRevA.66.032110
null
quant-ph cond-mat
null
What entanglement is present in naturally occurring physical systems at thermal equilibrium? Most such systems are intractable and it is desirable to study simple but realistic systems which can be solved. An example of such a system is the 1D infinite-lattice anisotropic XY model. This model is exactly solvable using the Jordan-Wigner transform, and it is possible to calculate the two-site reduced density matrix for all pairs of sites. Using the two-site density matrix, the entanglement of formation between any two sites is calculated for all parameter values and temperatures. We also study the entanglement in the transverse Ising model, a special case of the XY model, which exhibits a quantum phase transition. It is found that the next-nearest neighbour entanglement (though not the nearest-neighbour entanglement) is a maximum at the critical point. Furthermore, we show that the critical point in the transverse Ising model corresponds to a transition in the behaviour of the entanglement between a single site and the remainder of the lattice.
[{'version': 'v1', 'created': 'Wed, 27 Feb 2002 04:29:23 GMT'}]
2007-05-23
[array(['Osborne', 'Tobias J.', ''], dtype=object) array(['Nielsen', 'Michael A.', ''], dtype=object)]
19,313
2102.10906
Jordan Richards
Jordan Richards and Jonathan A. Tawn and Simon Brown
Modelling Extremes of Spatial Aggregates of Precipitation using Conditional Methods
null
null
null
null
stat.ME stat.AP
http://creativecommons.org/licenses/by/4.0/
Inference on the extremal behaviour of spatial aggregates of precipitation is important for quantifying river flood risk. There are two classes of previous approach, with one failing to ensure self-consistency in inference across different regions of aggregation and the other imposing highly restrictive assumptions. To overcome these issues, we propose a model for high-resolution precipitation data, from which we can simulate realistic fields and explore the behaviour of spatial aggregates. Recent developments have seen spatial extensions of the Heffernan and Tawn (2004) model for conditional multivariate extremes, which can handle a wide range of dependence structures. Our contribution is twofold: extensions and improvements of this approach and its model inference for high-dimensional data; and a novel framework for deriving aggregates addressing edge effects and sub-regions without rain. We apply our modelling approach to gridded East-Anglia, UK precipitation data. Return-level curves for spatial aggregates over different regions of various sizes are estimated and shown to fit very well to the data.
[{'version': 'v1', 'created': 'Mon, 22 Feb 2021 11:14:12 GMT'} {'version': 'v2', 'created': 'Tue, 9 Nov 2021 14:54:54 GMT'} {'version': 'v3', 'created': 'Fri, 28 Jan 2022 16:55:40 GMT'} {'version': 'v4', 'created': 'Tue, 21 Jun 2022 10:59:46 GMT'}]
2022-06-22
[array(['Richards', 'Jordan', ''], dtype=object) array(['Tawn', 'Jonathan A.', ''], dtype=object) array(['Brown', 'Simon', ''], dtype=object)]
19,314
1508.03945
Tatsuo Nishitani
F. Colombini, T. Nishitani, J. Rauch
Weakly Hyperbolic Systems by Symmetrization
null
null
null
null
math.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study hyperbolic first order systems and propose a new method proving Gevrey well posedness, constructing a symmetrizer, motivated by a special Lyapunov function for linear ODE. The proof not only gives a priori estimates straightforward so simply but also clarifies some effects coming from the spectral structures other than the multiplicities of the eigenvalues.
[{'version': 'v1', 'created': 'Mon, 17 Aug 2015 08:16:43 GMT'} {'version': 'v2', 'created': 'Mon, 18 Apr 2016 08:34:17 GMT'}]
2016-04-19
[array(['Colombini', 'F.', ''], dtype=object) array(['Nishitani', 'T.', ''], dtype=object) array(['Rauch', 'J.', ''], dtype=object)]
19,315
2009.09714
Antonios Nathanail
Antonios Nathanail, Ramandeep Gill, Oliver Porth, Christian M. Fromm, Luciano Rezzolla
3D magnetised jet break-out from neutron-star binary merger ejecta: afterglow emission from the jet and the ejecta
MNRAS accepted, updated version
null
10.1093/mnras/stab115
null
astro-ph.HE gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We perform three-dimensional (3D) general-relativistic magnetohydrodynamic simulations to model the jet break-out from the ejecta expected to be produced in a binary neutron-star merger. The structure of the relativistic outflow from the 3D simulation confirms our previous results from 2D simulations, namely, that a relativistic magnetized outflow breaking out from the merger ejecta exhibits a hollow core of $\theta_{\rm core}\approx4^{\circ}$, an opening angle of $\theta_{\rm jet}\gtrsim10^{\circ}$, and is accompanied by a wind of ejected matter that will contribute to the kilonova emission. We also compute the non-thermal afterglow emission of the relativistic outflow and fit it to the panchromatic afterglow from GRB170817A, together with the superluminal motion reported from VLBI observations. In this way, we deduce an observer angle of $\theta_{\rm obs}= 35.7^{\circ \,\,+1.8}_{\phantom{\circ \,\,}-2.2}$. We further compute the afterglow emission from the ejected matter and constrain the parameter space for a scenario in which the matter responsible for the thermal kilonova emission will also lead to a non-thermal emission yet to be observed.
[{'version': 'v1', 'created': 'Mon, 21 Sep 2020 09:31:29 GMT'} {'version': 'v2', 'created': 'Fri, 29 Jan 2021 08:35:03 GMT'}]
2021-02-01
[array(['Nathanail', 'Antonios', ''], dtype=object) array(['Gill', 'Ramandeep', ''], dtype=object) array(['Porth', 'Oliver', ''], dtype=object) array(['Fromm', 'Christian M.', ''], dtype=object) array(['Rezzolla', 'Luciano', ''], dtype=object)]
19,316
astro-ph/0607247
Mathieu de Naurois
Mathieu de Naurois
Analysis methods for Atmospheric Cerenkov Telescopes
12 pages, 10 figures, proceedings of the conference "Towards a Network of Atmospheric Cherenkov Detectors VII", April 2005, Palaiseau, France
null
null
null
astro-ph
null
Three different analysis techniques for Atmospheric Imaging System are presented. The classical Hillas parameters based technique is shown to be robust and efficient, but more elaborate techniques can improve the sensitivity of the analysis. A comparison of the different analysis techniques shows that they use different information for gamma-hadron separation, and that it is possible to combine their qualities.
[{'version': 'v1', 'created': 'Wed, 12 Jul 2006 04:22:43 GMT'}]
2007-05-23
[array(['de Naurois', 'Mathieu', ''], dtype=object)]
19,317
2001.06615
Mitchell Burger
Mitchell Burger
The Risk to Population Health Equity Posed by Automated Decision Systems: A Narrative Review
11 pages excluding references
null
null
null
cs.CY cs.AI
http://creativecommons.org/licenses/by-nc-nd/4.0/
Artificial intelligence is already ubiquitous, and is increasingly being used to autonomously make ever more consequential decisions. However, there has been relatively little research into the existing and possible consequences for population health equity. A narrative review was undertaken using a hermeneutic approach to explore current and future uses of narrow AI and automated decision systems (ADS) in medicine and public health, issues that have emerged, and implications for equity. Accounts reveal a tremendous expectation on AI to transform medical and public health practices. Prominent demonstrations of AI capability - particularly in diagnostic decision making, risk prediction, and surveillance - are stimulating rapid adoption, spurred by COVID-19. Automated decisions being made have significant consequences for individual and population health and wellbeing. Meanwhile, it is evident that hazards including bias, incontestability, and privacy erosion have emerged in sensitive domains such as criminal justice where narrow AI and ADS are in common use. Reports of issues arising from their use in health are already appearing. As the use of ADS in health expands, it is probable that these hazards will manifest more widely. Bias, incontestability, and privacy erosion give rise to mechanisms by which existing social, economic and health disparities are perpetuated and amplified. Consequently, there is a significant risk that use of ADS in health will exacerbate existing population health inequities. The industrial scale and rapidity with which ADS can be applied heightens the risk to population health equity. It is incumbent on health practitioners and policy makers therefore to explore the potential implications of using ADS, to ensure the use of artificial intelligence promotes population health and equity.
[{'version': 'v1', 'created': 'Sat, 18 Jan 2020 06:52:47 GMT'} {'version': 'v2', 'created': 'Thu, 20 Jan 2022 05:25:43 GMT'}]
2022-01-21
[array(['Burger', 'Mitchell', ''], dtype=object)]
19,318
1401.6094
Leonardo Giuliano Trombetta
Diana L. L\'opez Nacir, Francisco D. Mazzitelli and Leonardo G. Trombetta
Hartree approximation in curved spacetimes revisited II: The semiclassical Einstein equations and de Sitter self-consistent solutions
32 pages, 4 figures
Phys. Rev. D 89, 084013 (2014)
10.1103/PhysRevD.89.084013
null
hep-th gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We consider the semiclassical Einstein equations (SEE) in the presence of a quantum scalar field with self-interaction $\lambda\phi^4$. Working in the Hartree truncation of the two-particle irreducible (2PI) effective action, we compute the vacuum expectation value of the energy-momentum tensor of the scalar field, which act as a source of the SEE. We obtain the renormalized SEE by implementing a consistent renormalization procedure. We apply our results to find self-consistent de Sitter solutions to the SEE in situations with or without spontaneous breaking of the $Z_2$-symmetry.
[{'version': 'v1', 'created': 'Thu, 23 Jan 2014 18:38:17 GMT'}]
2016-09-22
[array(['Nacir', 'Diana L. López', ''], dtype=object) array(['Mazzitelli', 'Francisco D.', ''], dtype=object) array(['Trombetta', 'Leonardo G.', ''], dtype=object)]
19,319
0711.3244
Sangtaek Kim
Sangtaek Kim, Robert R. Mcleod, Mark Saffman, and Kelvin H. Wagner
Doppler-free, Multi-wavelength Acousto-optic deflector for two-photon addressing arrays of Rb atoms in a Quantum Information Processor
28 pages, 16 figures, submitted to Applied Optics
Appl. Opt. 47, 1816 (2008)
10.1364/AO.47.001816
null
quant-ph
null
We demonstrate a dual wavelength acousto-optic deflector (AOD) designed to deflect two wavelengths to the same angles by driving with two RF frequencies. The AOD is designed as a beam scanner to address two-photon transitions in a two-dimensional array of trapped neutral Rb atoms in a quantum computer. Momentum space is used to design AODs that have the same diffraction angles for two wavelengths (780 nm and 480 nm) and have non-overlapping Bragg-matched frequency response at these wavelengths, so that there will be no crosstalk when proportional RF frequencies are applied to diffract the two wavelengths. The appropriate crystal orientation, crystal shape, transducer size, and transducer height are determined for an AOD made with a Tellurium dioxide crystal (TeO2). The designed and fabricated AOD has more than 100 resolvable spots, widely separated bandshapes for the two wavelengths within an overall octave bandwidth, spatially overlapping diffraction angles for both wavelengths (780 nm and 480 nm), and a 4 usec or less access time. Cascaded AODs in which the first device upshifts and the second downshifts allow Doppler-free scanning as required for addressing the narrow atomic resonance without detuning. We experimentally show the diffraction-limited Doppler-free scanning performance and spatial resolution of the designed AOD.
[{'version': 'v1', 'created': 'Wed, 21 Nov 2007 01:34:55 GMT'}]
2012-06-05
[array(['Kim', 'Sangtaek', ''], dtype=object) array(['Mcleod', 'Robert R.', ''], dtype=object) array(['Saffman', 'Mark', ''], dtype=object) array(['Wagner', 'Kelvin H.', ''], dtype=object)]
19,320
1807.06564
Daniel Ueltschi
Costanza Benassi, Daniel Ueltschi
Loop correlations in random wire models
20 pages, 5 figures. An error in Prop. 4.1 has been corrected
Commun. Math. Phys. 374, 525-547 (2020)
10.1007/s00220-019-03474-9
null
math-ph math.MP math.PR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We introduce a family of loop soup models on the hypercubic lattice. The models involve links on the edges, and random pairings of the link endpoints on the sites. We conjecture that loop correlations of distant points are given by Poisson-Dirichlet correlations in dimensions three and higher. We prove that, in a specific random wire model that is related to the classical XY spin system, the probability that distant sites form an even partition is given by the Poisson-Dirichlet counterpart.
[{'version': 'v1', 'created': 'Tue, 17 Jul 2018 17:13:22 GMT'} {'version': 'v2', 'created': 'Tue, 31 Jul 2018 11:17:15 GMT'} {'version': 'v3', 'created': 'Sat, 6 Apr 2019 15:29:41 GMT'} {'version': 'v4', 'created': 'Wed, 27 Apr 2022 15:09:16 GMT'}]
2022-04-28
[array(['Benassi', 'Costanza', ''], dtype=object) array(['Ueltschi', 'Daniel', ''], dtype=object)]
19,321
1402.2875
Anton Daitche
Anton Daitche and Tam\'as T\'el
Memory effects in chaotic advection of inertial particles
null
New Journal of Physics 16 073008 (2014)
10.1088/1367-2630/16/7/073008
null
physics.flu-dyn nlin.CD
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A systematic investigation of the effect of the history force on particle advection is carried out for both heavy and light particles. General relations are given to identify parameter regions where the history force is expected to be comparable with the Stokes drag. As an illustrative example, a paradigmatic two-dimensional flow, the von K\'arm\'an flow is taken. For small (but not extremely small) particles all investigated dynamical properties turn out to heavily depend on the presence of memory when compared to the memoryless case: the history force generates a rather non-trivial dynamics that appears to weaken (but not to suppress) inertial effects, it enhances the overall contribution of viscosity. We explore the parameter space spanned by the particle size and the density ratio, and find a weaker tendency for accumulation in attractors and for caustics formation. The Lyapunov exponent of transients becomes larger with memory. Periodic attractors are found to have a very slow, $t^{-1/2}$ type convergence towards the asymptotic form. We find that the concept of snapshot attractors is useful to understand this slow convergence: an ensemble of particles converges exponentially fast towards a snapshot attractor, which undergoes a slow shift for long times.
[{'version': 'v1', 'created': 'Wed, 12 Feb 2014 16:19:54 GMT'} {'version': 'v2', 'created': 'Thu, 24 Jul 2014 11:50:37 GMT'}]
2014-07-25
[array(['Daitche', 'Anton', ''], dtype=object) array(['Tél', 'Tamás', ''], dtype=object)]
19,322
1810.12947
Tsung-Han Hsieh
Tsung-Han Hsieh, Li Su and Yi-Hsuan Yang
A Streamlined Encoder/Decoder Architecture for Melody Extraction
This is a pre-print version of an ICASSP 2019 paper
null
null
null
eess.AS cs.SD
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Melody extraction in polyphonic musical audio is important for music signal processing. In this paper, we propose a novel streamlined encoder/decoder network that is designed for the task. We make two technical contributions. First, drawing inspiration from a state-of-the-art model for semantic pixel-wise segmentation, we pass through the pooling indices between pooling and un-pooling layers to localize the melody in frequency. We can achieve result close to the state-of-the-art with much fewer convolutional layers and simpler convolution modules. Second, we propose a way to use the bottleneck layer of the network to estimate the existence of a melody line for each time frame, and make it possible to use a simple argmax function instead of ad-hoc thresholding to get the final estimation of the melody line. Our experiments on both vocal melody extraction and general melody extraction validate the effectiveness of the proposed model.
[{'version': 'v1', 'created': 'Tue, 30 Oct 2018 18:15:03 GMT'} {'version': 'v2', 'created': 'Mon, 18 Feb 2019 07:54:41 GMT'}]
2019-02-19
[array(['Hsieh', 'Tsung-Han', ''], dtype=object) array(['Su', 'Li', ''], dtype=object) array(['Yang', 'Yi-Hsuan', ''], dtype=object)]
19,323
2108.02640
Dipramit Majumdar
Dipramit Majumdar and B. Sury
Fruit Diophantine Equation
3 pages, couple of typos fixed
null
null
null
math.HO math.NT
http://creativecommons.org/licenses/by/4.0/
We show that the Diophantine equation given by X^3+ XYZ = Y^2+Z^2+5 has no integral solution. As a consequence, we show that the family of elliptic curve given by the Weierstrass equations Y^2-kXY = X^3 - (k^2+5) has no integral point.
[{'version': 'v1', 'created': 'Thu, 5 Aug 2021 14:26:57 GMT'} {'version': 'v2', 'created': 'Sat, 7 Aug 2021 09:25:30 GMT'}]
2021-11-15
[array(['Majumdar', 'Dipramit', ''], dtype=object) array(['Sury', 'B.', ''], dtype=object)]
19,324
cond-mat/0308441
Joerg Rottler
Joerg Rottler and A.C. Maggs
A Continuum,O(N) Monte-Carlo algorithm for charged particles
null
null
10.1063/1.1642590
null
cond-mat.soft cond-mat.mtrl-sci physics.chem-ph physics.comp-ph
null
We introduce a Monte-Carlo algorithm for the simulation of charged particles moving in the continuum. Electrostatic interactions are not instantaneous as in conventional approaches, but are mediated by a constrained, diffusing electric field on an interpolating lattice. We discuss the theoretical justifications of the algorithm and show that it efficiently equilibrates model polyelectrolytes and polar fluids. In order to reduce lattice artifacts that arise from the interpolation of charges to the grid we implement a local, dynamic subtraction algorithm. This dynamic scheme is completely general and can also be used with other Coulomb codes, such as multigrid based methods.
[{'version': 'v1', 'created': 'Thu, 21 Aug 2003 20:32:04 GMT'}]
2009-11-10
[array(['Rottler', 'Joerg', ''], dtype=object) array(['Maggs', 'A. C.', ''], dtype=object)]
19,325
1907.13431
Sujoy Chakraborty
Sujoy Chakraborty
Chow Group of 1-cycles of the Moduli of Parabolic Bundles Over a Curve
Made changes in the overall presentation; comments and suggestions are welcome
null
null
null
math.AG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the Chow group of 1-cycles of the moduli space of semistable parabolic vector bundles of fixed rank, determinant and a generic weight over a nonsingular projective curve over $\mathbb{C}$ of genus at least 3. We show that, the Chow group of 1-cycles remains isomorphic as we vary the generic weight. As a consequence, we can give an explicit description of the Chow group in the case of rank 2 and determinant $\mathcal{O}(x)$, where $x\in X$ is a fixed point.
[{'version': 'v1', 'created': 'Wed, 31 Jul 2019 11:53:44 GMT'} {'version': 'v2', 'created': 'Thu, 1 Aug 2019 16:26:10 GMT'} {'version': 'v3', 'created': 'Sun, 19 Apr 2020 06:00:16 GMT'}]
2020-04-21
[array(['Chakraborty', 'Sujoy', ''], dtype=object)]
19,326
1405.4466
Amir H. Abbassi
Ali A. Asgari, Amir H. Abbassi, Jafar Khodagholizadeh
On the perturbation theory in spatially closed background
25 pages,no figures,accepted for publiction in EPJC
Eur.Phys.J.C(2014)74:2917
10.1140/epjc/s10052-014-2917-0
null
astro-ph.CO gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this article,we investigate some features of the perturbation theory in spatially closed universe. We will show that the perturbative field equations in a spatially closed universe always have two independent adiabatic solutions provided that the wavelengths of perturbation modes are very longer than the Hubble horizon. It will be revealed that these adiabatic solutions do not depend on the curvature directly. We also propound a new interpretation for the curvature perturbation in terms of the unperturbed geometry.
[{'version': 'v1', 'created': 'Sun, 18 May 2014 07:26:43 GMT'}]
2014-06-06
[array(['Asgari', 'Ali A.', ''], dtype=object) array(['Abbassi', 'Amir H.', ''], dtype=object) array(['Khodagholizadeh', 'Jafar', ''], dtype=object)]
19,327
2010.14778
Yonggan Fu
Yongan Zhang, Yonggan Fu, Weiwen Jiang, Chaojian Li, Haoran You, Meng Li, Vikas Chandra, Yingyan Lin
DNA: Differentiable Network-Accelerator Co-Search
null
null
null
null
cs.LG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Powerful yet complex deep neural networks (DNNs) have fueled a booming demand for efficient DNN solutions to bring DNN-powered intelligence into numerous applications. Jointly optimizing the networks and their accelerators are promising in providing optimal performance. However, the great potential of such solutions have yet to be unleashed due to the challenge of simultaneously exploring the vast and entangled, yet different design spaces of the networks and their accelerators. To this end, we propose DNA, a Differentiable Network-Accelerator co-search framework for automatically searching for matched networks and accelerators to maximize both the task accuracy and acceleration efficiency. Specifically, DNA integrates two enablers: (1) a generic design space for DNN accelerators that is applicable to both FPGA- and ASIC-based DNN accelerators and compatible with DNN frameworks such as PyTorch to enable algorithmic exploration for more efficient DNNs and their accelerators; and (2) a joint DNN network and accelerator co-search algorithm that enables simultaneously searching for optimal DNN structures and their accelerators' micro-architectures and mapping methods to maximize both the task accuracy and acceleration efficiency. Experiments and ablation studies based on FPGA measurements and ASIC synthesis show that the matched networks and accelerators generated by DNA consistently outperform state-of-the-art (SOTA) DNNs and DNN accelerators (e.g., 3.04x better FPS with a 5.46% higher accuracy on ImageNet), while requiring notably reduced search time (up to 1234.3x) over SOTA co-exploration methods, when evaluated over ten SOTA baselines on three datasets. All codes will be released upon acceptance.
[{'version': 'v1', 'created': 'Wed, 28 Oct 2020 05:57:16 GMT'}]
2020-10-29
[array(['Zhang', 'Yongan', ''], dtype=object) array(['Fu', 'Yonggan', ''], dtype=object) array(['Jiang', 'Weiwen', ''], dtype=object) array(['Li', 'Chaojian', ''], dtype=object) array(['You', 'Haoran', ''], dtype=object) array(['Li', 'Meng', ''], dtype=object) array(['Chandra', 'Vikas', ''], dtype=object) array(['Lin', 'Yingyan', ''], dtype=object)]
19,328
nucl-th/0407098
Hartmuth Arenh\"ovel
Agus Salam and Hartmuth Arenhoevel
Interaction effects in ${\bm K^+}$ photoproduction on the deuteron
20 pages, 18 figures, revtex4
Phys.Rev. C70 (2004) 044008
10.1103/PhysRevC.70.044008
MKPH-T-04_06
nucl-th
null
Kaon photoproduction on the deuteron is studied with respect to a specific two-body contribution, namely a pion mediated production process, besides other final state interaction contributions from kaon-nucleon and hyperon-nucleon scattering. In this process, a pion is first photoproduced on one nucleon and then interacts with the spectator nucleon in a strangeness exchange reaction leading to a kaon and a hyperon. A sizeable effect from this pion mediated contribution is found, considerably larger than the previously studied hyperon-nucleon rescattering, whereas kaon-nucleon rescattering is much less important. Besides total and semi-inclusive differential cross sections, tensor target asymmetries are studied with respect to the influence of such interaction effects.
[{'version': 'v1', 'created': 'Wed, 28 Jul 2004 11:54:27 GMT'}]
2009-11-10
[array(['Salam', 'Agus', ''], dtype=object) array(['Arenhoevel', 'Hartmuth', ''], dtype=object)]
19,329
1904.02286
Fabio Botelho Ph.D.
Fabio Botelho
A primal dual variational formulation and a multi-duality principle for a non-linear model of plates
21 pages, some more corrections implemented
null
null
null
math.OC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This article develops a new primal dual formulation for the Kirchhoff-Love non-linear plate model. At first we establish a duality principle which includes sufficient conditions of global optimality through the dual formulation. At this point we highlight this first duality principle is specially suitable for the case in which the membrane stress tensor is negative definite. In a second step, from such a general principle, we develop a primal dual variational formulation which also includes the corresponding sufficient conditions for global optimality. The results are based on standard tools of convex analysis and on a well known Toland result for D.C. optimization. Finally, in the last section, we present a multi-duality principle and qualitative relations between the critical points of the primal and dual formulations. We formally prove there is no duality gap between such primal and dual formulations in a local extremal context.
[{'version': 'v1', 'created': 'Wed, 3 Apr 2019 16:00:42 GMT'} {'version': 'v2', 'created': 'Thu, 18 Apr 2019 13:25:29 GMT'} {'version': 'v3', 'created': 'Mon, 11 May 2020 21:28:24 GMT'} {'version': 'v4', 'created': 'Wed, 13 May 2020 12:26:10 GMT'}]
2020-05-14
[array(['Botelho', 'Fabio', ''], dtype=object)]
19,330
math/0002035
Robert Lazarsfeld
Jean-Pierre Demailly, Lawrence Ein and Robert Lazarsfeld
A Subadditivity Property of Multiplier Ideals
Dedication reinserted, typos fixed
null
null
null
math.AG math.CV
null
Given an effective Q-divisor D on a smooth complex variety, one can associate to D its multiplier ideal sheaf J(D), which measures in a somewhat subtle way the singularities of D. Because of their strong vanishing properties, these ideals have come to play an increasingly important role in higher dimensional geometry. We prove that for two effective Q-divisors D and E, one has the "subadditivity" relation: J(D + E) \subseteq J(D) . J(E) . (We also establish several natural variants, including the analogous statement for the analytic multiplier ideals associated to plurisubharmonic functions.) As an application, we give a new proof of a theorem of Fujita concerning the volume of a big linear series on a projective variety. The first section of the paper contains an overview of the construction and basic properties of multiplier ideals from an algebro-geometric perspective, as well as a discussion of the relation between some asymptotic algebraic constructions and their analytic counterparts.
[{'version': 'v1', 'created': 'Fri, 4 Feb 2000 18:10:50 GMT'} {'version': 'v2', 'created': 'Mon, 17 Apr 2000 17:09:29 GMT'}]
2007-05-23
[array(['Demailly', 'Jean-Pierre', ''], dtype=object) array(['Ein', 'Lawrence', ''], dtype=object) array(['Lazarsfeld', 'Robert', ''], dtype=object)]
19,331
1703.10639
Amir Sani
Francesco Lamperti, Andrea Roventini and Amir Sani
Agent-Based Model Calibration using Machine Learning Surrogates
32 pages, 19 figures
null
null
null
q-fin.EC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Taking agent-based models (ABM) closer to the data is an open challenge. This paper explicitly tackles parameter space exploration and calibration of ABMs combining supervised machine-learning and intelligent sampling to build a surrogate meta-model. The proposed approach provides a fast and accurate approximation of model behaviour, dramatically reducing computation time. In that, our machine-learning surrogate facilitates large scale explorations of the parameter-space, while providing a powerful filter to gain insights into the complex functioning of agent-based models. The algorithm introduced in this paper merges model simulation and output analysis into a surrogate meta-model, which substantially ease ABM calibration. We successfully apply our approach to the Brock and Hommes (1998) asset pricing model and to the "Island" endogenous growth model (Fagiolo and Dosi, 2003). Performance is evaluated against a relatively large out-of-sample set of parameter combinations, while employing different user-defined statistical tests for output analysis. The results demonstrate the capacity of machine learning surrogates to facilitate fast and precise exploration of agent-based models' behaviour over their often rugged parameter spaces.
[{'version': 'v1', 'created': 'Thu, 30 Mar 2017 18:57:56 GMT'} {'version': 'v2', 'created': 'Thu, 6 Apr 2017 07:30:13 GMT'}]
2017-04-07
[array(['Lamperti', 'Francesco', ''], dtype=object) array(['Roventini', 'Andrea', ''], dtype=object) array(['Sani', 'Amir', ''], dtype=object)]
19,332
1012.0244
Roie Volkovich
Roie Volkovich and Uri Peskin
Transient Dynamics in Molecular Junctions: Coherent Bichromophoric Molecular Electron Pumps
null
Physical Review B 83, 033403. 2011
10.1103/PhysRevB.83.033403
null
quant-ph cond-mat.mes-hall
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The possibility of using single molecule junctions as electron pumps for energy conversion and storage is considered. It is argued that the small dimensions of these systems enable to make use of unique intra-molecular quantum coherences in order to pump electrons between two leads and to overcome relaxation processes which tend to suppress the pumping efficiency. In particular, we demonstrate that a selective transient excitation of one chromophore in a bi-chromophoric donor-bridge-acceptor molecular junction model yields currents which transfer charge (electron and holes) unevenly to the two leads in the absence of a bias potential. The utility of this mechanism for charge pumping in steady state conditions is proposed.
[{'version': 'v1', 'created': 'Wed, 1 Dec 2010 16:54:20 GMT'}]
2015-05-20
[array(['Volkovich', 'Roie', ''], dtype=object) array(['Peskin', 'Uri', ''], dtype=object)]
19,333
cond-mat/0612245
Molly De Raychaudhury
Molly De Raychaudhury, T. Saha-Dasgupta and D. D. Sarma
Theoretical study of doped-Tl$_{2}$Mn$_{2}$O$_{7}$ and Tl$_{2}$Mn$_{2}$O$_{7}$ under pressure
Accepted for publication in PRB
null
10.1103/PhysRevB.75.014443
null
cond-mat.mtrl-sci cond-mat.str-el
null
Using first-principles density functional based calculations, we study the effect of doping and pressure in manganese based pyrochlore compound,Tl$_{2}$Mn$_{2}$O$_{7}$ that exhibits colossal magneto-resistive behavior. The theoretical study is motivated by the counter-intuitive experimental observation of suppression of ferromagnetic transition temperature upon application of pressure and its enhancement upon substitution of Mn by moderate amount of nonmagnetic Sb ion. We also attempt to resolve the issue related to crystal structure changes that may occur upon application of pressure.
[{'version': 'v1', 'created': 'Mon, 11 Dec 2006 06:02:48 GMT'} {'version': 'v2', 'created': 'Tue, 2 Jan 2007 06:38:36 GMT'}]
2009-11-11
[array(['De Raychaudhury', 'Molly', ''], dtype=object) array(['Saha-Dasgupta', 'T.', ''], dtype=object) array(['Sarma', 'D. D.', ''], dtype=object)]
19,334
1009.2493
Christian Gogolin
Christian Gogolin, Markus P. Mueller, and Jens Eisert
Absence of Thermalization in Nonintegrable Systems
5 pages, 2 figures, to appear in PRL, improved presentation of the numerical findings, editorial changes
Phys. Rev. Lett. 106, 040401 (2011)
10.1103/PhysRevLett.106.040401
null
quant-ph cond-mat.stat-mech
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We establish a link between unitary relaxation dynamics after a quench in closed many-body systems and the entanglement in the energy eigenbasis. We find that even if reduced states equilibrate, they can have memory on the initial conditions even in certain models that are far from integrable. We show that in such situations the equilibrium states are still described by a maximum entropy or generalized Gibbs ensemble, regardless of whether a model is integrable or not, thereby contributing to a recent debate. In addition, we discuss individual aspects of the thermalization process, comment on the role of Anderson localization, and collect and compare different notions of integrability.
[{'version': 'v1', 'created': 'Mon, 13 Sep 2010 19:55:21 GMT'} {'version': 'v2', 'created': 'Thu, 6 Jan 2011 11:10:39 GMT'}]
2011-01-25
[array(['Gogolin', 'Christian', ''], dtype=object) array(['Mueller', 'Markus P.', ''], dtype=object) array(['Eisert', 'Jens', ''], dtype=object)]
19,335
2012.14435
Fumio Uchida
Kohei Kamada, Fumio Uchida, Jun'ichi Yokoyama
Baryon isocurvature constraints on the primordial hypermagnetic fields
40 pages, 4 figures, 1 table
null
10.1088/1475-7516/2021/04/034
RESCEU-24/20
astro-ph.CO hep-ph hep-th
http://creativecommons.org/licenses/by/4.0/
It has been pointed out that hypermagnetic helicity decay at the electroweak symmetry breaking may have produced the observed baryon asymmetry of the Universe through the chiral anomaly in the standard model of particle physics. Although fully helical magnetic field that can adequately produce the observed baryon asymmetry is not strong enough to explain the origin of the intergalactic magnetic field inferred by the Fermi satellite, the mixture of helical and nonhelical primordial magnetic fields may explain both baryogenesis and the intergalactic magnetic fields simultaneously. We first show that such a scenario is ruled out by the constraint on the amplitude of baryon isocurvature perturbations produced by the primordial magnetic fields to avoid overproduction of deuterium at the big bang nucleosynthesis. Then we show that any attempt to explain the origin of intergalactic magnetic field by primordial magnetogenesis before the electroweak symmetry breaking does not work due to the above constraint irrespective of the helicity and baryogenesis mechanism.
[{'version': 'v1', 'created': 'Mon, 28 Dec 2020 19:00:00 GMT'}]
2021-04-21
[array(['Kamada', 'Kohei', ''], dtype=object) array(['Uchida', 'Fumio', ''], dtype=object) array(['Yokoyama', "Jun'ichi", ''], dtype=object)]
19,336
1002.3921
Elke-Caroline Aschenauer
The HERMES Collaboration: A. Airapetian, et al
Leading-Order Determination of the Gluon Polarization from high-$p_T$ Hadron Electroproduction
null
JHEP 1008:130,2010
10.1007/JHEP08(2010)130
DESY-10-021
hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Longitudinal double-spin asymmetries of charged hadrons with high transverse momentum $p_T$ have been measured in electroproduction using the \hermes\ detector at \hera. Processes involving gluons in the nucleon have been enhanced relative to others by selecting hadrons with $p_T$ typically above 1 GeV. In this kinematic domain the gluon polarization has been extracted in leading order making use of the model embedded in the Monte Carlo Generator \Pythia\ 6.2. The gluon polarization obtained from single inclusive hadrons in the $p_T$ range 1 GeV $< p_T <$ 2.5 GeV using a deuterium target is $\frac{\Delta g}{g}(\langle x\rangle, \langle \mu^2\rangle)=0.049\pm 0.034 (stat)\pm 0.010 (sys\textrm{-}exp)^{+0.126}_{-0.099}(sys\textrm{-}models)$ at a scale $\la\mu^2\ra=1.35~{\rm GeV}^2$ and $\langle x\rangle = 0.22$. For different final states and kinematic domains, consistent values of \DGG\ have been found within statistical uncertainties using hydrogen and deuterium targets.
[{'version': 'v1', 'created': 'Sat, 20 Feb 2010 17:31:24 GMT'} {'version': 'v2', 'created': 'Mon, 23 Aug 2010 12:26:48 GMT'}]
2012-08-03
[array(['The HERMES Collaboration', '', ''], dtype=object) array(['Airapetian', 'A.', ''], dtype=object)]
19,337
2302.06657
Istv\'an Fazekas
Istv\'an Fazekas and Borb\'ala Fazekas and Michael Ochieng Suja
Convergence rate for the longest T-contaminated runs of heads. Paper with detailed proofs
20 pages, 4 figures
null
null
null
math.PR
http://creativecommons.org/licenses/by/4.0/
We study the length of $T$-contaminated runs of heads in the well-known coin tossing experiment. A $T$-contaminated run of heads is a sequence of consecutive heads interrupted by $T$ tails. For $T=1$ and $T=2$ we find the asymptotic distribution for the first hitting time of the $T$ contaminated run of heads having length $m$; furthermore, we obtain a limit theorem for the length of the longest $T$-contaminated head run. We prove that the rate of the approximation of our accompanying distribution for the length of the longest $T$-contaminated head run is considerably better than the previous ones. For the proof we use a powerful lemma by Cs\'aki, F\"oldes and Koml\'os.
[{'version': 'v1', 'created': 'Mon, 13 Feb 2023 19:41:04 GMT'}]
2023-02-15
[array(['Fazekas', 'István', ''], dtype=object) array(['Fazekas', 'Borbála', ''], dtype=object) array(['Suja', 'Michael Ochieng', ''], dtype=object)]
19,338
1111.6751
Pedro Sacramento
P. D. Sacramento, L. C. Fernandes Silva, G. S. Nunes, M. A. N. Araujo and V. R. Vieira
Supercurrent induced domain wall motion
10 pages, 8 figures
Physical Review B 83, 054403 (2011)
10.1103/PhysRevB.83.054403
null
cond-mat.supr-con
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the dynamics of a magnetic domain wall, inserted in, or juxtaposed to, a conventional superconductor, via the passage of a spin polarized current through a FSF junction. Solving the Landau-Lifshitz-Gilbert equation of motion for the magnetic moments we calculate the velocity of the domain wall and compare it with the case of a FNF junction. We find that in several regimes the domain wall velocity is larger when it is driven by a supercurrent.
[{'version': 'v1', 'created': 'Tue, 29 Nov 2011 10:20:52 GMT'}]
2015-06-03
[array(['Sacramento', 'P. D.', ''], dtype=object) array(['Silva', 'L. C. Fernandes', ''], dtype=object) array(['Nunes', 'G. S.', ''], dtype=object) array(['Araujo', 'M. A. N.', ''], dtype=object) array(['Vieira', 'V. R.', ''], dtype=object)]
19,339
1912.12013
Shaofei Du
Jiyong Chen, Shaofei Du, Cai Heng Li
Skew-morphisms of nonabelian characteristically simple groups
18 Pages
null
null
null
math.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A skew-morphism of a finite group $G$ is a permutation $\s$ on $G$ fixing the identity element, and for which there exists an integer function $\pi$ on $G$ such that $\s(xy)=\s(x)\s^{\pi(x)}(y)$ for all $x,y\in G$. It has been known that given a skew-morphism $\s $ of $G$, the product of $\lg \s \rg$ with the left regular representation of $G$ forms a permutation group on $G$, called the skew-product group of $\s$. The skew-morphism was introduced as an algebraic tool to investigate regular Cayley maps. In this paper, the skew-product groups are characterized, for all skew-morphisms of finite nonabelian characteristically simple groups (see Theorem 1.1) and correspondingly the Cayley maps on these groups are characterized (see Theorem 1.5).
[{'version': 'v1', 'created': 'Fri, 27 Dec 2019 07:38:44 GMT'}]
2019-12-30
[array(['Chen', 'Jiyong', ''], dtype=object) array(['Du', 'Shaofei', ''], dtype=object) array(['Li', 'Cai Heng', ''], dtype=object)]
19,340
1303.6584
Christophe Ley
Christophe Ley and Thomas Verdebout
Simple, asymptotically distribution-free, optimal tests for circular reflective symmetry about a known median direction
23 pages, 2 figures
null
null
null
stat.ME
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we propose optimal tests for circular reflective symmetry about a fixed median direction. The distributions against which optimality is achieved are the so-called k-sine-skewed distributions of Umbach and Jammalamadaka (2009). We first show that sequences of k-sine-skewed models are locally and asymptotically normal in the vicinity of reflective symmetry. Following the Le Cam methodology, we then construct optimal (in the maximin sense) parametric tests for reflective symmetry, which we render semi-parametric by a studentization argument. These asymptotically distribution-free tests happen to be uniformly optimal (under any reference density) and are moreover of a very simple and intuitive form. They furthermore exhibit nice small sample properties, as we show through a Monte Carlo simulation study. Our new tests also allow us to re-visit the famous red wood ants data set of Jander (1957). We further show that one of the proposed parametric tests can as well serve as a test for uniformity against cardioid alternatives; this test coincides with the famous circular Rayleigh (1919) test for uniformity which is thus proved to be (also) optimal against cardioid alternatives. Moreover, our choice of k-sine-skewed alternatives, which are the circular analogues of the classical linear skew-symmetric distributions, permits us a Fisher singularity analysis \`a la Hallin and Ley (2012) with the result that only the prominent sine-skewed von Mises distribution suffers from these inferential drawbacks. Finally, we conclude the paper by discussing the unspecified location case.
[{'version': 'v1', 'created': 'Tue, 26 Mar 2013 18:13:08 GMT'}]
2013-03-27
[array(['Ley', 'Christophe', ''], dtype=object) array(['Verdebout', 'Thomas', ''], dtype=object)]
19,341
2103.02967
Antonio Bazco Nogueras
Hui Zhao, Antonio Bazco-Nogueras, Petros Elia
Wireless Coded Caching Can Overcome the Worst-User Bottleneck by Exploiting Finite File Sizes
null
null
null
null
cs.IT math.IT
http://creativecommons.org/licenses/by-nc-nd/4.0/
We address the worst-user bottleneck of wireless coded caching, which is known to severely diminish cache-aided multicasting gains due to the fundamental worst-channel limitation of multicasting transmission. We consider the quasi-static Rayleigh fading Broadcast Channel, for which we first show that the effective coded caching gain of the XOR-based standard coded-caching scheme completely vanishes in the low-SNR regime. Then, we reveal that this collapse is not intrinsic to coded caching. We do so by presenting a novel scheme that can fully recover the coded caching gains by capitalizing on one aspect that has to date remained unexploited: the shared side information brought about by the effectively unavoidable file-size constraint. As a consequence, the worst-user effect is dramatically ameliorated, as it is substituted by a much more subtle worst-group-of-users effect, where the suggested grouping is fixed, and it is decided before the channel or the demands are known. In some cases, the theoretical gains are completely recovered, and this is done without any user selection technique. We analyze the achievable rate performance of the proposed scheme and derive insightful performance approximations which prove to be very precise.
[{'version': 'v1', 'created': 'Thu, 4 Mar 2021 11:41:32 GMT'}]
2021-03-05
[array(['Zhao', 'Hui', ''], dtype=object) array(['Bazco-Nogueras', 'Antonio', ''], dtype=object) array(['Elia', 'Petros', ''], dtype=object)]
19,342
2304.05450
Bastien Grosso
Bastien F. Grosso, Daniel W. Davies, Bonan Zhu, Aron Walsh, David O. Scanlon
Accessible Chemical Space for Metal Nitride Perovskites
null
null
null
null
cond-mat.mtrl-sci
http://creativecommons.org/licenses/by-nc-nd/4.0/
Building on the extensive exploration of metal oxide and metal halide perovskites, metal nitride perovskites represent a largely unexplored class of materials. We report a multi-tier computational screening of this chemical space. From a pool of 3660 ABN$_3$ compositions covering I-VIII, II-VII, III-VI and IV-V oxidation state combinations, 279 are predicted to be chemically feasible. The ground-state structures of the 25 most promising candidate compositions were explored through enumeration over octahedral tilt systems and global optimisation. We predict 12 dynamically and thermodynamically stable nitride perovskite materials, including YMoN$_3$, YWN$_3$, ZrTaN$_3$, and LaMoN$_3$. These feature significant electric polarisation and low predicted switching electric field, showing similarities with metal oxide perovskites and making them attractive for ferroelectric memory devices
[{'version': 'v1', 'created': 'Tue, 11 Apr 2023 18:47:15 GMT'}]
2023-04-13
[array(['Grosso', 'Bastien F.', ''], dtype=object) array(['Davies', 'Daniel W.', ''], dtype=object) array(['Zhu', 'Bonan', ''], dtype=object) array(['Walsh', 'Aron', ''], dtype=object) array(['Scanlon', 'David O.', ''], dtype=object)]
19,343
1505.06716
Jakob Bj\"ornberg
J. E. Bj\"ornberg
Large cycles in random permutations related to the Heisenberg model
11 pages
Electron. Commun. Probab., Volume 20, 2015
10.1214/ECP.v20-4328
null
math.PR math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the weighted version of the interchange process where a permutation receives weight $\theta^{\#\mathrm{cycles}}$. For $\theta=2$ this is T\'oth's representation of the quantum Heisenberg ferromagnet on the complete graph. We prove, for $\theta>1$, that large cycles appear at `low temperature'.
[{'version': 'v1', 'created': 'Mon, 25 May 2015 18:57:06 GMT'} {'version': 'v2', 'created': 'Sat, 6 Jun 2015 10:23:25 GMT'} {'version': 'v3', 'created': 'Sun, 5 Jul 2015 19:23:19 GMT'}]
2019-12-16
[array(['Björnberg', 'J. E.', ''], dtype=object)]
19,344
1503.02584
Keith Bechtol
The DES Collaboration, K. Bechtol, A. Drlica-Wagner, E. Balbinot, A. Pieres, J. D. Simon, B. Yanny, B. Santiago, R. H. Wechsler, J. Frieman, A. R. Walker, P. Williams, E. Rozo, E. S. Rykoff, A. Queiroz, E. Luque, A. Benoit-Levy, D. Tucker, I. Sevilla, R. A. Gruendl, L. N. da Costa, A. Fausti Neto, M. A. G. Maia, T. Abbott, S. Allam, R. Armstrong, A. H. Bauer, G. M. Bernstein, R. A. Bernstein, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. Burke, A. Carnero Rosell, F. J. Castander, R. Covarrubias, C. B. D'Andrea, D. L. DePoy, S. Desai, H. T. Diehl, T. F. Eifler, J. Estrada, A. E. Evrard, E. Fernandez, D. A. Finley, B. Flaugher, E. Gaztanaga, D. Gerdes, L. Girardi, M. Gladders, D. Gruen, G. Gutierrez, J. Hao, K. Honscheid, B. Jain, D. James, S. Kent, R. Kron, K. Kuehn, N. Kuropatkin, O. Lahav, T. S. Li, H. Lin, M. Makler, M. March, J. Marshall, P. Martini, K. W. Merritt, C. Miller, R. Miquel, J. Mohr, E. Neilsen, R. Nichol, B. Nord, R. Ogando, J. Peoples, D. Petravick, A. A. Plazas, A. K. Romer, A. Roodman, M. Sako, E. Sanchez, V. Scarpine, M. Schubnell, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarle, J. Thaler, D. Thomas, W. Wester, J. Zuntz
Eight New Milky Way Companions Discovered in First-Year Dark Energy Survey Data
33 pages, 12 figures, 3 tables. Accepted for publication in ApJ. Readers may be interested in the concurrent work by Koposov, Belokurov, Torrealba, & Evans (http://arxiv.org/abs/1503.02079). Indirect dark matter search results are presented in Drlica-Wagner, Albert, Bechtol, Wood, Strigari, et al. (The LAT and DES Collaborations, http://arxiv.org/abs/1503.02632)
null
10.1088/0004-637X/807/1/50
null
astro-ph.GA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We report the discovery of eight new Milky Way companions in ~1,800 deg^2 of optical imaging data collected during the first year of the Dark Energy Survey (DES). Each system is identified as a statistically significant over-density of individual stars consistent with the expected isochrone and luminosity function of an old and metal-poor stellar population. The objects span a wide range of absolute magnitudes (M_V from -2.2 mag to -7.4 mag), physical sizes (10 pc to 170 pc), and heliocentric distances (30 kpc to 330 kpc). Based on the low surface brightnesses, large physical sizes, and/or large Galactocentric distances of these objects, several are likely to be new ultra-faint satellite galaxies of the Milky Way and/or Magellanic Clouds. We introduce a likelihood-based algorithm to search for and characterize stellar over-densities, as well as identify stars with high satellite membership probabilities. We also present completeness estimates for detecting ultra-faint galaxies of varying luminosities, sizes, and heliocentric distances in the first-year DES data.
[{'version': 'v1', 'created': 'Mon, 9 Mar 2015 17:54:00 GMT'} {'version': 'v2', 'created': 'Thu, 28 May 2015 22:44:22 GMT'}]
2015-09-02
[array(['The DES Collaboration', '', ''], dtype=object) array(['Bechtol', 'K.', ''], dtype=object) array(['Drlica-Wagner', 'A.', ''], dtype=object) array(['Balbinot', 'E.', ''], dtype=object) array(['Pieres', 'A.', ''], dtype=object) array(['Simon', 'J. D.', ''], dtype=object) array(['Yanny', 'B.', ''], dtype=object) array(['Santiago', 'B.', ''], dtype=object) array(['Wechsler', 'R. H.', ''], dtype=object) array(['Frieman', 'J.', ''], dtype=object) array(['Walker', 'A. R.', ''], dtype=object) array(['Williams', 'P.', ''], dtype=object) array(['Rozo', 'E.', ''], dtype=object) array(['Rykoff', 'E. S.', ''], dtype=object) array(['Queiroz', 'A.', ''], dtype=object) array(['Luque', 'E.', ''], dtype=object) array(['Benoit-Levy', 'A.', ''], dtype=object) array(['Tucker', 'D.', ''], dtype=object) array(['Sevilla', 'I.', ''], dtype=object) array(['Gruendl', 'R. A.', ''], dtype=object) array(['da Costa', 'L. N.', ''], dtype=object) array(['Neto', 'A. Fausti', ''], dtype=object) array(['Maia', 'M. A. G.', ''], dtype=object) array(['Abbott', 'T.', ''], dtype=object) array(['Allam', 'S.', ''], dtype=object) array(['Armstrong', 'R.', ''], dtype=object) array(['Bauer', 'A. H.', ''], dtype=object) array(['Bernstein', 'G. M.', ''], dtype=object) array(['Bernstein', 'R. A.', ''], dtype=object) array(['Bertin', 'E.', ''], dtype=object) array(['Brooks', 'D.', ''], dtype=object) array(['Buckley-Geer', 'E.', ''], dtype=object) array(['Burke', 'D. L.', ''], dtype=object) array(['Rosell', 'A. Carnero', ''], dtype=object) array(['Castander', 'F. J.', ''], dtype=object) array(['Covarrubias', 'R.', ''], dtype=object) array(["D'Andrea", 'C. B.', ''], dtype=object) array(['DePoy', 'D. L.', ''], dtype=object) array(['Desai', 'S.', ''], dtype=object) array(['Diehl', 'H. T.', ''], dtype=object) array(['Eifler', 'T. F.', ''], dtype=object) array(['Estrada', 'J.', ''], dtype=object) array(['Evrard', 'A. E.', ''], dtype=object) array(['Fernandez', 'E.', ''], dtype=object) array(['Finley', 'D. A.', ''], dtype=object) array(['Flaugher', 'B.', ''], dtype=object) array(['Gaztanaga', 'E.', ''], dtype=object) array(['Gerdes', 'D.', ''], dtype=object) array(['Girardi', 'L.', ''], dtype=object) array(['Gladders', 'M.', ''], dtype=object) array(['Gruen', 'D.', ''], dtype=object) array(['Gutierrez', 'G.', ''], dtype=object) array(['Hao', 'J.', ''], dtype=object) array(['Honscheid', 'K.', ''], dtype=object) array(['Jain', 'B.', ''], dtype=object) array(['James', 'D.', ''], dtype=object) array(['Kent', 'S.', ''], dtype=object) array(['Kron', 'R.', ''], dtype=object) array(['Kuehn', 'K.', ''], dtype=object) array(['Kuropatkin', 'N.', ''], dtype=object) array(['Lahav', 'O.', ''], dtype=object) array(['Li', 'T. S.', ''], dtype=object) array(['Lin', 'H.', ''], dtype=object) array(['Makler', 'M.', ''], dtype=object) array(['March', 'M.', ''], dtype=object) array(['Marshall', 'J.', ''], dtype=object) array(['Martini', 'P.', ''], dtype=object) array(['Merritt', 'K. W.', ''], dtype=object) array(['Miller', 'C.', ''], dtype=object) array(['Miquel', 'R.', ''], dtype=object) array(['Mohr', 'J.', ''], dtype=object) array(['Neilsen', 'E.', ''], dtype=object) array(['Nichol', 'R.', ''], dtype=object) array(['Nord', 'B.', ''], dtype=object) array(['Ogando', 'R.', ''], dtype=object) array(['Peoples', 'J.', ''], dtype=object) array(['Petravick', 'D.', ''], dtype=object) array(['Plazas', 'A. A.', ''], dtype=object) array(['Romer', 'A. K.', ''], dtype=object) array(['Roodman', 'A.', ''], dtype=object) array(['Sako', 'M.', ''], dtype=object) array(['Sanchez', 'E.', ''], dtype=object) array(['Scarpine', 'V.', ''], dtype=object) array(['Schubnell', 'M.', ''], dtype=object) array(['Smith', 'R. C.', ''], dtype=object) array(['Soares-Santos', 'M.', ''], dtype=object) array(['Sobreira', 'F.', ''], dtype=object) array(['Suchyta', 'E.', ''], dtype=object) array(['Swanson', 'M. E. C.', ''], dtype=object) array(['Tarle', 'G.', ''], dtype=object) array(['Thaler', 'J.', ''], dtype=object) array(['Thomas', 'D.', ''], dtype=object) array(['Wester', 'W.', ''], dtype=object) array(['Zuntz', 'J.', ''], dtype=object)]
19,345
0911.0948
Achilles Tertikas
Adimurthi, Stathis Filippas, Achilles Tertikas
On the best constant of Hardy-Sobolev Inequalities
null
null
null
null
math.AP math.FA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We obtain the sharp constant for the Hardy-Sobolev inequality involving the distance to the origin. This inequality is equivalent to a limiting Caffarelli-Kohn-Nirenberg inequality. In three dimensions, in certain cases the sharp constant coincides with the best Sobolev constant.
[{'version': 'v1', 'created': 'Wed, 4 Nov 2009 22:42:29 GMT'}]
2009-11-06
[array(['Adimurthi', '', ''], dtype=object) array(['Filippas', 'Stathis', ''], dtype=object) array(['Tertikas', 'Achilles', ''], dtype=object)]
19,346
1603.08957
Elmo Tempel
E. Tempel, R. S. Stoica, R. Kipper, E. Saar
Bisous model - detecting filamentary patterns in point processes
12 pages, 6 figures, accepted by Astronomy and Computing
null
null
null
astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The cosmic web is a highly complex geometrical pattern, with galaxy clusters at the intersection of filaments and filaments at the intersection of walls. Identifying and describing the filamentary network is not a trivial task due to the overwhelming complexity of the structure, its connectivity and the intrinsic hierarchical nature. To detect and quantify galactic filaments we use the Bisous model, which is a marked point process built to model multi-dimensional patterns. The Bisous filament finder works directly with the galaxy distribution data and the model intrinsically takes into account the connectivity of the filamentary network. The Bisous model generates the visit map (the probability to find a filament at a given point) together with the filament orientation field. Using these two fields, we can extract filament spines from the data. Together with this paper we publish the computer code for the Bisous model that is made available in GitHub. The Bisous filament finder has been successfully used in several cosmological applications and further development of the model will allow to detect the filamentary network also in photometric redshift surveys, using the full redshift posterior. We also want to encourage the astro-statistical community to use the model and to connect it with all other existing methods for filamentary pattern detection and characterisation.
[{'version': 'v1', 'created': 'Tue, 29 Mar 2016 20:39:49 GMT'}]
2016-03-31
[array(['Tempel', 'E.', ''], dtype=object) array(['Stoica', 'R. S.', ''], dtype=object) array(['Kipper', 'R.', ''], dtype=object) array(['Saar', 'E.', ''], dtype=object)]
19,347
cond-mat/9601066
Yurii Barash
Yu.S.Barash, and A.A.Svidzinsky (P.N.Lebedev Physics Institute, Moscow)
On the low temperature properties and specific anisotropy of pure anisotropically paired superconductors
20 pages
null
10.1103/PhysRevB.53.15254
null
cond-mat
null
Dependences of low temperature behavior and anisotropy of various physical quantities for pure unconventional superconductors upon a particular form of momentum direction dependence for the superconducting order parameter (within the framework of the same symmetry type of superconducting pairing) are considered. A special attention is drawn to the possibility of different multiplicities of the nodes of the order parameter under their fixed positions on the Fermi surface, which are governed by symmetry. The problem of an unambiguous identification of a type of superconducting pairing on the basis of corresponding experimental results is discussed. Quasiparticle density of states at low energy for both homogeneous and mixed states, the low temperature dependences of the specific heat, penetration depth and thermal conductivity, the I-V curves of SS and NS tunnel junctions at low voltages are examined. A specific anisotropy of the boundary conditions for unconventional superconducting order parameter near $T_c$ for the case of specular reflection from the boundary is also investigated.
[{'version': 'v1', 'created': 'Wed, 17 Jan 1996 15:29:11 GMT'}]
2009-10-28
[array(['Barash', 'Yu. S.', '', 'P.N.Lebedev Physics Institute,\n Moscow'], dtype=object) array(['Svidzinsky', 'A. A.', '', 'P.N.Lebedev Physics Institute,\n Moscow'], dtype=object)]
19,348
1006.0663
Gaurav Khanna
Rakesh Ginjupalli and Gaurav Khanna
High-Precision Numerical Simulations of Rotating Black Holes Accelerated by CUDA
6 pages, 1 figure, 1 table, Accepted for publication in the International Conference on High Performance Computing Systems (HPCS 2010)
null
null
null
physics.comp-ph gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Hardware accelerators (such as Nvidia's CUDA GPUs) have tremendous promise for computational science, because they can deliver large gains in performance at relatively low cost. In this work, we focus on the use of Nvidia's Tesla GPU for high-precision (double, quadruple and octal precision) numerical simulations in the area of black hole physics -- more specifically, solving a partial-differential-equation using finite-differencing. We describe our approach in detail and present the final performance results as compared with a single-core desktop processor and also the Cell BE. We obtain mixed results -- order-of-magnitude gains in overall performance in some cases and negligible gains in others.
[{'version': 'v1', 'created': 'Thu, 3 Jun 2010 14:30:31 GMT'}]
2010-06-04
[array(['Ginjupalli', 'Rakesh', ''], dtype=object) array(['Khanna', 'Gaurav', ''], dtype=object)]
19,349
1404.3000
Alan Stapledon
Eric Katz, Alan Stapledon
Tropical geometry, the motivic nearby fiber and limit mixed Hodge numbers of hypersurfaces
40 pages
Res. Math. Sci. 3 (2014), 1-36
null
null
math.AG math.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The motivic nearby fiber is an invariant obtained from degenerating a complex variety over a disc. It specializes to the Euler characteristic of the original variety but also contains information on the variation of Hodge structure associated to the degeneration which is encoded as a limit mixed Hodge structure. However, this invariant is difficult to compute in practice. Using the techniques of tropical geometry we present a new formula for the motivic nearby fiber. Moreover, since there is a range of available software implementing the main algorithms in tropical geometry, our formula can be computed in practice. We specialize to the case of families of sch\"{o}n complex hypersurfaces of tori where we provide explicit formulas describing the action of the unipotent part of monodromy on the graded pieces (with respect to the Deligne weight filtration) of the cohomology with compact supports. These families are described combinatorially by a polyhedral subdivision of the associated Newton polytope. We develop new mixed Hodge theory-inspired combinatorial invariants of such subdivisions, among them the `refined limit mixed $h^*$-polynomial'. These invariants are related to Stanley's combinatorial study of subdivisions: in a companion combinatorial paper whose results are applied here, we situate our invariants in Stanley's theory where they become multi-variable extensions of his invariants. Our results generalize work of Danilov and Khovanski{\u\i} and Batyrev and Borisov on the Hodge numbers of hypersurfaces. We also present analogous formulas describing the action of the unipotent part of monodromy on the intersection cohomology groups of a family of sch\"on hypersurfaces of a projective toric variety.
[{'version': 'v1', 'created': 'Fri, 11 Apr 2014 04:51:25 GMT'} {'version': 'v2', 'created': 'Tue, 2 Dec 2014 00:19:11 GMT'}]
2021-10-05
[array(['Katz', 'Eric', ''], dtype=object) array(['Stapledon', 'Alan', ''], dtype=object)]
19,350
math/0204202
Vladimir Pestov
Vladimir Pestov
Remarks on actions on compacta by some infinite-dimensional groups
19 pages, LaTeX with World Scientific macros, to appear in Proc. Conf. on Infinite-Dimensional Lie Groups in Geometry and Representation Theory (Howard Univ., Washington, D.C., August 2000)
in: Infinite-Dimensional Lie Groups in Geometry and Representation Theory (Washington, D.C., 2000), World Sci. Publishing, River Edge, NJ, 2002, pp. 145-163.
null
null
math.DS
null
We discuss some techniques related to equivariant compactifications of uniform spaces and amenability of topological groups. In particular, we give a new proof of a recent result by Glasner and Weiss describing the universal minimal flow of the infinite symmetric group ${\mathfrak S}_\infty$ with the standard Polish topology, and extend Bekka's concept of an amenable representation, enabling one to deduce non-amenability of the Banach--Lie groups $\GL(L_p)$ and $\GL(\ell_p)$, $1\leq p <\infty$.
[{'version': 'v1', 'created': 'Tue, 16 Apr 2002 09:26:24 GMT'} {'version': 'v2', 'created': 'Tue, 23 Apr 2002 22:53:11 GMT'}]
2007-09-03
[array(['Pestov', 'Vladimir', ''], dtype=object)]
19,351
2104.08428
Kaiqi Fu
Kaiqi Fu and Jones Lin and Dengfeng Ke and Yanlu Xie and Jinsong Zhang and Binghuai Lin
A Full Text-Dependent End to End Mispronunciation Detection and Diagnosis with Easy Data Augmentation Techniques
Submitted to INTERSPEECH2021
null
null
null
cs.CL
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Recently, end-to-end mispronunciation detection and diagnosis (MD&D) systems has become a popular alternative to greatly simplify the model-building process of conventional hybrid DNN-HMM systems by representing complicated modules with a single deep network architecture. In this paper, in order to utilize the prior text in the end-to-end structure, we present a novel text-dependent model which is difference with sed-mdd, the model achieves a fully end-to-end system by aligning the audio with the phoneme sequences of the prior text inside the model through the attention mechanism. Moreover, the prior text as input will be a problem of imbalance between positive and negative samples in the phoneme sequence. To alleviate this problem, we propose three simple data augmentation methods, which effectively improve the ability of model to capture mispronounced phonemes. We conduct experiments on L2-ARCTIC, and our best performance improved from 49.29% to 56.08% in F-measure metric compared to the CNN-RNN-CTC model.
[{'version': 'v1', 'created': 'Sat, 17 Apr 2021 03:11:41 GMT'}]
2021-04-20
[array(['Fu', 'Kaiqi', ''], dtype=object) array(['Lin', 'Jones', ''], dtype=object) array(['Ke', 'Dengfeng', ''], dtype=object) array(['Xie', 'Yanlu', ''], dtype=object) array(['Zhang', 'Jinsong', ''], dtype=object) array(['Lin', 'Binghuai', ''], dtype=object)]
19,352
hep-ph/9411292
Ed Yao
York-Peng Yao
${1\over m_b}$ and ${1\over m_t}$ Expansion of the Weak Mixing Matrix
A set of references has been added to ealier related work
Phys.Rev.D51:5240-5244,1995
10.1103/PhysRevD.51.5240
UM-TH-94-33
hep-ph
null
We perform a $1/m_b$ and $1/m_t$ expansion of the Cabibbo-Kobayashi- Maskawa mixing matrix. Data suggest that the dominant parts of the Yukawa couplings are factorizable into sets of numbers $\vert r>$, $\vert s>$, and $\vert s'>$, associated, respectively, with the left-handed doublets, the right-handed up singlets, and the right- handed down singlets. The first order expansion is consistent with Wolfenstein parameterization, which is an expansion in $sin \theta _c$ to third order. The mixing matrix elements in the present approach are partitioned into factors determined by the relative orientations of $\vert r>$, $\vert s>$, and $\vert s'>$ and the dynamics provided by the subdominant mass matrices. A short discussion is given of some experimental support and a generalized Fritzsch model is used to contrast our approach.
[{'version': 'v1', 'created': 'Mon, 14 Nov 1994 19:26:31 GMT'} {'version': 'v2', 'created': 'Sun, 20 Nov 1994 20:01:47 GMT'}]
2010-11-01
[array(['Yao', 'York-Peng', ''], dtype=object)]
19,353
1701.05619
Yani Zhao
Yani Zhao, Mateusz Chwastyk and Marek Cieplak
Topological transformations in proteins: effects of heating and proximity of an interface
7 figures
Scientific Reports 7, 39851 (2017)
null
null
q-bio.BM
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Using a structure-based coarse-grained model of proteins, we study the mechanism of unfolding of knotted proteins through heating. We find that the dominant mechanisms of unfolding depend on the temperature applied and are generally distinct from those identified for folding at its optimal temperature. In particular, for shallowly knotted proteins, folding usually involves formation of two loops whereas unfolding through high-temperature heating is dominated by untying of single loops. Untying the knots is found to generally precede unfolding unless the protein is deeply knotted and the heating temperature exceeds a threshold value. We then use a phenomenological model of the air-water interface to show that such an interface can untie shallow knots, but it can also make knots in proteins that are natively unknotted.
[{'version': 'v1', 'created': 'Thu, 19 Jan 2017 22:05:03 GMT'}]
2017-01-23
[array(['Zhao', 'Yani', ''], dtype=object) array(['Chwastyk', 'Mateusz', ''], dtype=object) array(['Cieplak', 'Marek', ''], dtype=object)]
19,354
1610.00164
Alina Bucur
Alina Bucur, Edgar Costa, Chantal David, Jo\~ao Guerreiro and David Lowry-Duda
Traces, high powers and one level density for families of curves over finite fields
24 pages
null
null
null
math.NT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The zeta function of a curve $C$ over a finite field may be expressed in terms of the characteristic polynomial of a unitary matrix $\Theta_C$. We develop and present a new technique to compute the expected value of $\mathrm{Tr}(\Theta_C^n)$ for various moduli spaces of curves of genus $g$ over a fixed finite field in the limit as $g$ is large, generalizing and extending the work of Rudnick and Chinis. This is achieved by using function field zeta functions, explicit formulae, and the densities of prime polynomials with prescribed ramification types at certain places as given by Bucur, David, Feigon, Kaplan, Lal\'in and Wood [BDF$^+$16] and by Zhao. We extend [BDF$^+$16] by describing explicit dependence on the place and give an explicit proof of the Lindel\"{o}f bound for function field Dirichlet $L$-functions $L(1/2 + it, \chi)$. As applications, we compute the one-level density for hyperelliptic curves, cyclic $\ell$-covers, and cubic non-Galois covers.
[{'version': 'v1', 'created': 'Sat, 1 Oct 2016 18:15:06 GMT'}]
2016-10-04
[array(['Bucur', 'Alina', ''], dtype=object) array(['Costa', 'Edgar', ''], dtype=object) array(['David', 'Chantal', ''], dtype=object) array(['Guerreiro', 'João', ''], dtype=object) array(['Lowry-Duda', 'David', ''], dtype=object)]
19,355
math-ph/0605032
Alice Barbara Tumpach
Alice Barbara Tumpach
Infinite-dimensional hyperkaehler manifolds associated with Hermitian-symmetric affine coadjoint orbits
20 pages, 1 figure
null
null
null
math-ph math.MP math.SG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper is devoted to the construction of a hyperkaehler structure on the complexification of any Hermitian-symmetric affine coadjoint orbit O of a semi-simple L*-group of compact type, which is compatible with the complex symplectic form of Kirillov-Kostant-Souriau and restricts to the Kaehler structure of O. By the identification of the complexification of O with the cotangent space of O induced by Mostow's Decomposition Theorem, this leads to the existence of a hyperkaehler structure on the cotangent space of O compatible with Liouville's symplectic form and whose restriction to the zero section is the Kaehler structure of O. Explicit formulas of the metric in terms of the complexified orbit and of the cotangent space are given.
[{'version': 'v1', 'created': 'Tue, 9 May 2006 13:24:09 GMT'} {'version': 'v2', 'created': 'Tue, 15 Jul 2008 13:30:27 GMT'}]
2008-07-15
[array(['Tumpach', 'Alice Barbara', ''], dtype=object)]
19,356
nucl-ex/9906009
Birger B. Back
Birger B. Back
Fission Characteristics of Heavy Nuclei: Statics and Dynamics
11 pages, 7 figures, Symp. on "Nuclear Shapes and Motions" in honor of Ray Nix., Santa Fe, NM, October 25-27, 1998
Heavy Ion Phys.10:209-220,1999
null
null
nucl-ex
null
This paper presents a selective historical perspective of fission research over the last thirty-five years while Ray Nix has made central contributions to the field. The emphasis is placed on early studies of the shell stabilized secondary minimum in the static fission barrier and on the dynamic properties of fission of hot nuclei, which have recently been the focus of intense study.
[{'version': 'v1', 'created': 'Mon, 14 Jun 1999 15:27:33 GMT'}]
2011-04-15
[array(['Back', 'Birger B.', ''], dtype=object)]
19,357
2211.06239
Bradley Eck
Bradley Eck and Duygu Kabakci-Zorlu and Yan Chen and France Savard and Xiaowei Bao
A monitoring framework for deployed machine learning models with supply chain examples
8 pages, 9 figures, IEEE Big Data 2022
null
null
null
cs.LG stat.AP
http://creativecommons.org/licenses/by/4.0/
Actively monitoring machine learning models during production operations helps ensure prediction quality and detection and remediation of unexpected or undesired conditions. Monitoring models already deployed in big data environments brings the additional challenges of adding monitoring in parallel to the existing modelling workflow and controlling resource requirements. In this paper, we describe (1) a framework for monitoring machine learning models; and, (2) its implementation for a big data supply chain application. We use our implementation to study drift in model features, predictions, and performance on three real data sets. We compare hypothesis test and information theoretic approaches to drift detection in features and predictions using the Kolmogorov-Smirnov distance and Bhattacharyya coefficient. Results showed that model performance was stable over the evaluation period. Features and predictions showed statistically significant drifts; however, these drifts were not linked to changes in model performance during the time of our study.
[{'version': 'v1', 'created': 'Fri, 11 Nov 2022 14:31:38 GMT'}]
2022-11-14
[array(['Eck', 'Bradley', ''], dtype=object) array(['Kabakci-Zorlu', 'Duygu', ''], dtype=object) array(['Chen', 'Yan', ''], dtype=object) array(['Savard', 'France', ''], dtype=object) array(['Bao', 'Xiaowei', ''], dtype=object)]
19,358
1711.07564
Chaoxu Zhou
Jose Blanchet, Donald Goldfarb, Garud Iyengar, Fengpei Li, Chaoxu Zhou
Unbiased Simulation for Optimizing Stochastic Function Compositions
null
null
null
null
math.OC stat.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we introduce an unbiased gradient simulation algorithms for solving convex optimization problem with stochastic function compositions. We show that the unbiased gradient generated from the algorithm has finite variance and finite expected computation cost. We then combined the unbiased gradient simulation with two variance reduced algorithms (namely SVRG and SCSG) and showed that the proposed optimization algorithms based on unbiased gradient simulations exhibit satisfactory convergence properties. Specifically, in the SVRG case, the algorithm with simulated gradient can be shown to converge linearly to optima in expectation and almost surely under strong convexity. Finally, for the numerical experiment,we applied the algorithms to two important cases of stochastic function compositions optimization: maximizing the Cox's partial likelihood model and training conditional random fields.
[{'version': 'v1', 'created': 'Mon, 20 Nov 2017 21:58:01 GMT'}]
2017-11-22
[array(['Blanchet', 'Jose', ''], dtype=object) array(['Goldfarb', 'Donald', ''], dtype=object) array(['Iyengar', 'Garud', ''], dtype=object) array(['Li', 'Fengpei', ''], dtype=object) array(['Zhou', 'Chaoxu', ''], dtype=object)]
19,359
hep-ph/0502086
Jeff Forshaw
J.R. Forshaw, A. Kyrieleis, M.H. Seymour
Gaps between Jets in the High Energy Limit
29 pages, 9 figures, minor corrections to text and improved figures
JHEP 0506:034,2005
10.1088/1126-6708/2005/06/034
null
hep-ph
null
We use perturbative QCD to calculate the parton level cross section for the production of two jets that are far apart in rapidity, subject to a limitation on the total transverse momentum Q0 in the interjet region. We specifically address the question of how to combine the approach which sums all leading logarithms in Q/Q0 (where Q is the jet transverse momentum) with the BFKL approach, in which leading logarithms of the scattering energy are summed. This paper constitutes progress towards the simultaneous summation of all important logarithms. Using an "all orders" matching, we are able to obtain results for the cross section which correctly reproduce the two approaches in the appropriate limits.
[{'version': 'v1', 'created': 'Wed, 9 Feb 2005 14:37:22 GMT'} {'version': 'v2', 'created': 'Fri, 10 Jun 2005 17:31:16 GMT'}]
2010-03-12
[array(['Forshaw', 'J. R.', ''], dtype=object) array(['Kyrieleis', 'A.', ''], dtype=object) array(['Seymour', 'M. H.', ''], dtype=object)]
19,360
2302.03449
Florinda Capone Prof.
Florinda Capone and Roberta De Luca and Isabella Torcicollo
Turing patterns in a Leslie-Gower predator prey model
null
null
null
null
q-bio.PE math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A reaction-diffusion Leslie-Gower predator-prey model, incorporating the fear effect and prey refuge, with Beddington-DeAngelis functional response, is introduced. A qualitative analysis of the solutions of the model and the stability analysis of the coexistence equilibrium, are performed. Sufficient conditions guaranteeing the occurrence of Turing instability have been determined either in the case of self-diffusion or in the case of cross-diffusion. Different types of Turing patterns, representing a spatial redistribution of population in the environment, emerge for different values of the model parameters.
[{'version': 'v1', 'created': 'Tue, 7 Feb 2023 13:06:15 GMT'}]
2023-02-08
[array(['Capone', 'Florinda', ''], dtype=object) array(['De Luca', 'Roberta', ''], dtype=object) array(['Torcicollo', 'Isabella', ''], dtype=object)]
19,361
2304.01821
Emil Njor
Emil Njor, Jan Madsen, Xenofon Fafoutis
Data Aware Neural Architecture Search
Accepted as a full paper by the TinyML Research Symposium 2023
null
null
null
cs.NE
http://creativecommons.org/licenses/by/4.0/
Neural Architecture Search (NAS) is a popular tool for automatically generating Neural Network (NN) architectures. In early NAS works, these tools typically optimized NN architectures for a single metric, such as accuracy. However, in the case of resource constrained Machine Learning, one single metric is not enough to evaluate a NN architecture. For example, a NN model achieving a high accuracy is not useful if it does not fit inside the flash memory of a given system. Therefore, recent works on NAS for resource constrained systems have investigated various approaches to optimize for multiple metrics. In this paper, we propose that, on top of these approaches, it could be beneficial for NAS optimization of resource constrained systems to also consider input data granularity. We name such a system "Data Aware NAS", and we provide experimental evidence of its benefits by comparing it to traditional NAS.
[{'version': 'v1', 'created': 'Tue, 4 Apr 2023 14:20:36 GMT'}]
2023-04-05
[array(['Njor', 'Emil', ''], dtype=object) array(['Madsen', 'Jan', ''], dtype=object) array(['Fafoutis', 'Xenofon', ''], dtype=object)]
19,362
astro-ph/0405316
Szymczak Marian
M. Szymczak, E. Gerard
Polarimetric observations of OH masers in proto-planetary nebulae
Accepted for publication in A&A; 11 pages, 7 figures
Astron.Astrophys. 423 (2004) 209-219
10.1051/0004-6361:20040461
null
astro-ph
null
The 1612 and 1667 MHz OH maser lines have been measured in all four Stokes parameters in 47 proto-planetary nebula (PPN) candidates. Out of 42 objects detected, 40 and 34 are 1612 and 1667 MHz emitters, respectively. The spectral extent of the 1667 MHz line overshoots that of the 1612 MHz line in about 80% of the targets. 52% and 26% of the 1612 and 1667 MHz sources, respectively, show linear polarization in at least some features. Circular polarization is more frequent, occurring in 78% and 32% of sources of the respective OH lines. The percentage polarization is usually small (<15%) reaching up to 50-80% in a few sources. Features of linearly polarized emission are usually weak (0.5-4Jy) and narrow (0.3-0.5kms^{-1}). The strength of magnetic field inferred from likely Zeeman pairs in two sources of a few mG is consistent with values reported elsewhere for those classes of objects. An upper limit of the electron density in the envelope of OH17.7-2.0 derived from the difference in the position angle of polarization vectors for the two OH lines is about 1cm^{-3}. Distinct profiles of polarization position angle at 1612 and 1667 MHz are seen in about one third of the sources and strongly suggest that the envelopes are permeated with structured magnetic fields. The geometry of the magnetic field is implicated as an important cause of the depolarization found in some PPN candidates. For the subset of targets which show axisymmetric shells in the optical or radio images we found a dominance of magnetic field components which are orthogonal to the long axis of the nebulae. This finding supports the hypothesis that such bipolar lobes are shaped by the magnetic field.
[{'version': 'v1', 'created': 'Mon, 17 May 2004 13:01:43 GMT'}]
2009-11-10
[array(['Szymczak', 'M.', ''], dtype=object) array(['Gerard', 'E.', ''], dtype=object)]
19,363
hep-lat/0304015
Takanori Sugihara
Takanori Sugihara (RIKEN BNL)
Lattice chiral symmetry with hopping interactions
4 pages, 4 figures, revtex, published version
Phys.Rev. D68 (2003) 034502
10.1103/PhysRevD.68.034502
null
hep-lat
null
We formulate Dirac fermions on a (1+1)-dimensional lattice based on a Hamiltonian formalism. The species doubling problem of the lattice fermion is resolved by introducing hopping interactions that mix left- and right-handed fermions around the momentum boundary. Approximate chiral symmetry is realized on the lattice. The deviation of the fermion propagator from the continuum one is small.
[{'version': 'v1', 'created': 'Tue, 22 Apr 2003 18:05:51 GMT'} {'version': 'v2', 'created': 'Mon, 2 Jun 2003 14:13:31 GMT'} {'version': 'v3', 'created': 'Tue, 12 Aug 2003 14:54:19 GMT'}]
2009-11-10
[array(['Sugihara', 'Takanori', '', 'RIKEN BNL'], dtype=object)]
19,364
hep-th/0102181
null
V.P. Nair, A.P. Polychronakos
On Level Quantization for the Noncommutative Chern-Simons Theory
6 pages, Latex, no figures
Phys.Rev.Lett. 87 (2001) 030403
10.1103/PhysRevLett.87.030403
CCNY-HEP-01-01, RU-01-3-B
hep-th
null
We show that the coefficient of the three-dimensional Chern-Simons action on the noncommutative plane must be quantized. Similar considerations apply in other dimensions as well.
[{'version': 'v1', 'created': 'Mon, 26 Feb 2001 20:46:29 GMT'}]
2009-11-07
[array(['Nair', 'V. P.', ''], dtype=object) array(['Polychronakos', 'A. P.', ''], dtype=object)]
19,365
physics/0602104
Flavio Cruz
Flavio C. Cruz, Matthew C. Stowe, and Jun Ye
Tapered semiconductor amplifiers for optical frequency combs in the near infrared
3 pages, 4 figures, to appear in Optics Letters
null
10.1364/OL.31.001337
null
physics.optics physics.atom-ph
null
A tapered semiconductor amplifier is injection seeded by a femtosecond optical frequency comb at 780 nm from a mode-locked Ti:sapphire laser. Energy gains over 17 dB (12 dB) are obtained for 1 mW (20 mW) of average input power when the input pulses are stretched into the picosecond range. A spectral window of supercontinuum light generated in a photonic fiber has also been amplified. Interferometric measurements show sub-hertz linewidths for a heterodyne beat between the input and amplified comb components, yielding no detectable phase-noise degradation under amplification. These amplifiers can be used to boost the infrared power in f-to-2f interferometers used to determine the carrier-to-envelope offset frequency, with clear advantages for stabilization of octave-spanning femtosecond lasers and other supercontinuum light sources with very limited power in the infrared.
[{'version': 'v1', 'created': 'Wed, 15 Feb 2006 11:27:54 GMT'}]
2009-11-11
[array(['Cruz', 'Flavio C.', ''], dtype=object) array(['Stowe', 'Matthew C.', ''], dtype=object) array(['Ye', 'Jun', ''], dtype=object)]
19,366
1410.0551
Nynke Vlietstra
N. Vlietstra, M. Isasa, J. Shan, J. Ben Youssef, F. Casanova, B.J. van Wees
Simultaneous detection of the spin-Hall magnetoresistance and the spin-Seebeck effect in Platinum and Tantalum on Yttrium Iron Garnet
9 pages, 6 figures
Phys. Rev. B 90, 174436 (2014)
10.1103/PhysRevB.90.174436
null
cond-mat.mes-hall
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The spin-Seebeck effect (SSE) in platinum (Pt) and tantalum (Ta) on yttrium iron garnet (YIG) has been investigated by both externally heating the sample (using an on-chip Pt heater on top of the device) as well as by current-induced heating. For SSE measurements, external heating is the most common method to obtain clear signals. Here we show that also by current-induced heating it is possible to directly observe the SSE, separate from the also present spin-Hall magnetoresistance (SMR) signal, by using a lock-in detection technique. Using this measurement technique, the presence of additional 2nd order signals at low applied magnetic fields and high heating currents is revealed. These signals are caused by current-induced magnetic fields (Oersted fields) generated by the used AC-current, resulting in dynamic SMR signals.
[{'version': 'v1', 'created': 'Thu, 2 Oct 2014 13:44:48 GMT'} {'version': 'v2', 'created': 'Thu, 27 Nov 2014 13:01:45 GMT'}]
2014-12-01
[array(['Vlietstra', 'N.', ''], dtype=object) array(['Isasa', 'M.', ''], dtype=object) array(['Shan', 'J.', ''], dtype=object) array(['Youssef', 'J. Ben', ''], dtype=object) array(['Casanova', 'F.', ''], dtype=object) array(['van Wees', 'B. J.', ''], dtype=object)]
19,367
2101.08328
John Salzer
Joseph D. Watkins, John J. Salzer, Angela Van Sistine, Ana Hayslip, Eric Hoar, Rayna Rampalli
The H$\alpha$ Dots Survey. IV. A Fourth List of Faint Emission-Line Objects
Accepted for publication in the Astrophysical Journal Supplement Series
null
10.3847/1538-4365/abdf4b
null
astro-ph.GA
http://creativecommons.org/licenses/by/4.0/
We present the fourth catalog of serendipitously discovered compact extragalactic emission-line sources -- H$\alpha$ Dots. A total of 454 newly discovered objects are included in the current survey list. These objects have been detected in searches of moderately deep narrow-band images acquired for the ALFALFA H$\alpha$ project (Van Sistine et al. 2016). The catalog of H-alpha Dots presented in the current paper was derived from searches carried out using ALFALFA H$\alpha$ images obtained with the KPNO 2.1 m telescope. This results in a substantially deeper sample of Dots compared to our previous lists, which were all discovered in images taken with the WIYN 0.9 m telescope. The median R-band magnitude of the current catalog is 21.59, more than 1.6 magnitudes fainter than the median for the 0.9~m sample (factor of 4.4x fainter). Likewise, the median emission-line flux of the detected sources is a factor of 4.3x fainter. The line-flux completeness limit of the current sample is approximately 3 x 10$^{-16}$ erg/s/cm$^2$. We present accurate coordinates, apparent magnitudes and narrow-band line fluxes for each object in the sample. Unlike our previous lists of H$\alpha$ Dots, the current sample does not include follow-up spectroscopy.
[{'version': 'v1', 'created': 'Wed, 20 Jan 2021 21:24:08 GMT'}]
2021-03-24
[array(['Watkins', 'Joseph D.', ''], dtype=object) array(['Salzer', 'John J.', ''], dtype=object) array(['Van Sistine', 'Angela', ''], dtype=object) array(['Hayslip', 'Ana', ''], dtype=object) array(['Hoar', 'Eric', ''], dtype=object) array(['Rampalli', 'Rayna', ''], dtype=object)]
19,368
2112.14231
Davood Rafiei Karkevandi
Davood Rafiei Karkevandi, Soroush Shakeri, Violetta Sagun and Oleksii Ivanytskyi
Tidal Deformability as a Probe of Dark Matter in Neutron Stars
The article is prepared for the proceedings of the sixteenth Marcel Grossmann meeting (MG16)
Published by the World Scientific, Proceedings of the MG16 Meeting, pp. 3713-3731 (2023)
10.1142/9789811269776_0307
null
astro-ph.HE gr-qc hep-ph nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The concept of boson stars (BSs) was first introduced by Kaup and Ruffini-Bonazzola in the 1960s. Following this idea, we investigate an effect of self-interacting asymmetric bosonic dark matter (DM) according to Colpi et al. model for BSs (1986) on different observable properties of neutron stars (NSs). In this paper, the bosonic DM and baryonic matter (BM) are mixed together and interact only through gravitational force. The presence of DM as a core of a compact star or as an extended halo around it is examined by applying different boson masses and DM fractions for a fixed coupling constant. The impact of DM core/halo formations on a DM admixed NS properties is probed through the maximum mass and tidal deformability of NSs. Thanks to the recent detection of Gravitational-Waves (GWs) and the latest X-ray observations, the DM admixed NS's features are compared to LIGO/Virgo and NICER results.
[{'version': 'v1', 'created': 'Tue, 28 Dec 2021 17:36:29 GMT'}]
2023-02-08
[array(['Karkevandi', 'Davood Rafiei', ''], dtype=object) array(['Shakeri', 'Soroush', ''], dtype=object) array(['Sagun', 'Violetta', ''], dtype=object) array(['Ivanytskyi', 'Oleksii', ''], dtype=object)]
19,369
1210.7913
Mikael Vejdemo-Johansson
Mikael Vejdemo-Johansson
Interleaved equivalence of categories of persistence modules
9 pages
null
null
null
math.AT cs.CG math.CT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We demonstrate that an equivalence of categories using $\varepsilon$-interleavings as a fundamental component exists between the model of persistence modules as graded modules over a polynomial ring and the model of persistence modules as modules over the total order of the real numbers.
[{'version': 'v1', 'created': 'Tue, 30 Oct 2012 07:13:53 GMT'}]
2012-10-31
[array(['Vejdemo-Johansson', 'Mikael', ''], dtype=object)]
19,370
2011.07412
Sebastian Paeckel
Jan Stolpp, Thomas K\"ohler, Salvatore R. Manmana, Eric Jeckelmann, Fabian Heidrich-Meisner and Sebastian Paeckel
Comparative Study of State-of-the-Art Matrix-Product-State Methods for Lattice Models with Large Local Hilbert Spaces
ancillary data files provided
Computer Physics Communications, Volume 269, December 2021, 108106
10.1016/j.cpc.2021.108106
null
cond-mat.str-el cond-mat.other hep-lat quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Lattice models consisting of high-dimensional local degrees of freedom without global particle-number conservation constitute an important problem class in the field of strongly correlated quantum many-body systems. For instance, they are realized in electron-phonon models, cavities, atom-molecule resonance models, or superconductors. In general, these systems elude a complete analytical treatment and need to be studied using numerical methods where matrix-product states (MPS) provide a flexible and generic ansatz class. Typically, MPS algorithms scale at least quadratic in the dimension of the local Hilbert spaces. Hence, tailored methods, which truncate this dimension, are required to allow for efficient simulations. Here, we describe and compare three state-of-the-art MPS methods each of which exploits a different approach to tackle the computational complexity. We analyze the properties of these methods for the example of the Holstein model, performing high-precision calculations as well as a finite-size-scaling analysis of relevant ground-state obervables. The calculations are performed at different points in the phase diagram yielding a comprehensive picture of the different approaches.
[{'version': 'v1', 'created': 'Sat, 14 Nov 2020 23:24:46 GMT'} {'version': 'v2', 'created': 'Tue, 24 Aug 2021 21:43:26 GMT'} {'version': 'v3', 'created': 'Mon, 20 Sep 2021 11:01:49 GMT'} {'version': 'v4', 'created': 'Thu, 30 Sep 2021 19:04:50 GMT'}]
2021-10-04
[array(['Stolpp', 'Jan', ''], dtype=object) array(['Köhler', 'Thomas', ''], dtype=object) array(['Manmana', 'Salvatore R.', ''], dtype=object) array(['Jeckelmann', 'Eric', ''], dtype=object) array(['Heidrich-Meisner', 'Fabian', ''], dtype=object) array(['Paeckel', 'Sebastian', ''], dtype=object)]
19,371
1808.09127
Touqir Sajed
Touqir Sajed, Wesley Chung, Martha White
High-confidence error estimates for learned value functions
Presented at (UAI) Uncertainty in Artificial Intelligence 2018
null
null
null
stat.ML cs.LG
http://creativecommons.org/licenses/by/4.0/
Estimating the value function for a fixed policy is a fundamental problem in reinforcement learning. Policy evaluation algorithms---to estimate value functions---continue to be developed, to improve convergence rates, improve stability and handle variability, particularly for off-policy learning. To understand the properties of these algorithms, the experimenter needs high-confidence estimates of the accuracy of the learned value functions. For environments with small, finite state-spaces, like chains, the true value function can be easily computed, to compute accuracy. For large, or continuous state-spaces, however, this is no longer feasible. In this paper, we address the largely open problem of how to obtain these high-confidence estimates, for general state-spaces. We provide a high-confidence bound on an empirical estimate of the value error to the true value error. We use this bound to design an offline sampling algorithm, which stores the required quantities to repeatedly compute value error estimates for any learned value function. We provide experiments investigating the number of samples required by this offline algorithm in simple benchmark reinforcement learning domains, and highlight that there are still many open questions to be solved for this important problem.
[{'version': 'v1', 'created': 'Tue, 28 Aug 2018 05:39:48 GMT'}]
2018-08-29
[array(['Sajed', 'Touqir', ''], dtype=object) array(['Chung', 'Wesley', ''], dtype=object) array(['White', 'Martha', ''], dtype=object)]
19,372
1908.05333
Artour Tomberg
Artour Tomberg
Families of stable bundles on the fibres of the hyperk\"ahler twistor projection
29 pages
null
null
null
math.AG math.DG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Given a holomorphic vector bundle $E$ on the twistor space $\mathrm{Tw}(M)$ of a simple hyperk\"ahler manifold $M$, we view it as a family of bundles $\left\{E_I\right\}$ on the fibres $\pi^{-1}(I)$ of the twistor projection $\pi : \mathrm{Tw}(M) \to \mathbb{CP}^1$, and study the relationship between stability of $E$ and its fibrewise stability. We verify that the argument of Teleman establishing the Zariski openness of stability and semi-stability in families of bundles applies in the case of the family $\left\{E_I\right\}$. We prove a partial converse to a result of Kaledin and Verbitsky, showing that an irreducible bundle $E$ on $\mathrm{Tw}(M)$ is generically fibrewise stable if the rank of $E$ is 2 or 3, or at least one element of the family $\left\{E_I\right\}$ is a simple bundle, in the sense that $\mathrm{Hom}(E_I, E_I) = \mathbb{C}$.
[{'version': 'v1', 'created': 'Wed, 14 Aug 2019 20:10:51 GMT'}]
2019-08-16
[array(['Tomberg', 'Artour', ''], dtype=object)]
19,373
astro-ph/0011557
Robert Nichol
R. Nichol, C. Miller, A. Connolly, S. Chong, C. Genovese, A. Moore, D. Reichart, J. Schneider, L. Wasserman, J. Annis, J. Brinkman, H. Bohringer, F. Castander, R. Kim, T. McKay, M. Postman, E. Sheldon, I. Szapudi, K. Romer, W. Voges
SDSS-RASS: Next Generation of Cluster-Finding Algorithms
To appear in Proceedings of MPA/MPE/ESO Conference "Mining the Sky", July 31 - August 4, 2000, Garching, Germany
null
10.1007/10849171_81
null
astro-ph
null
We outline here the next generation of cluster-finding algorithms. We show how advances in Computer Science and Statistics have helped develop robust, fast algorithms for finding clusters of galaxies in large multi-dimensional astronomical databases like the Sloan Digital Sky Survey (SDSS). Specifically, this paper presents four new advances: (1) A new semi-parametric algorithm - nicknamed ``C4'' - for jointly finding clusters of galaxies in the SDSS and ROSAT All-Sky Survey databases; (2) The introduction of the False Discovery Rate into Astronomy; (3) The role of kernel shape in optimizing cluster detection; (4) A new determination of the X-ray Cluster Luminosity Function which has bearing on the existence of a ``deficit'' of high redshift, high luminosity clusters. This research is part of our ``Computational AstroStatistics'' collaboration (see Nichol et al. 2000) and the algorithms and techniques discussed herein will form part of the ``Virtual Observatory'' analysis toolkit.
[{'version': 'v1', 'created': 'Thu, 30 Nov 2000 00:06:10 GMT'}]
2009-10-31
[array(['Nichol', 'R.', ''], dtype=object) array(['Miller', 'C.', ''], dtype=object) array(['Connolly', 'A.', ''], dtype=object) array(['Chong', 'S.', ''], dtype=object) array(['Genovese', 'C.', ''], dtype=object) array(['Moore', 'A.', ''], dtype=object) array(['Reichart', 'D.', ''], dtype=object) array(['Schneider', 'J.', ''], dtype=object) array(['Wasserman', 'L.', ''], dtype=object) array(['Annis', 'J.', ''], dtype=object) array(['Brinkman', 'J.', ''], dtype=object) array(['Bohringer', 'H.', ''], dtype=object) array(['Castander', 'F.', ''], dtype=object) array(['Kim', 'R.', ''], dtype=object) array(['McKay', 'T.', ''], dtype=object) array(['Postman', 'M.', ''], dtype=object) array(['Sheldon', 'E.', ''], dtype=object) array(['Szapudi', 'I.', ''], dtype=object) array(['Romer', 'K.', ''], dtype=object) array(['Voges', 'W.', ''], dtype=object)]
19,374
astro-ph/9905014
Antonino Del Popolo
A. Del Popolo and E. Spedicato and M. Gambera
Kuiper Belt evolution due to dynamical friction
10 pages, 4 encapsulated figures; accepted by A&A
null
null
null
astro-ph
null
In this paper we study the role of dynamical friction on the evolution of a population of large objects ($m>10^{22}$ g) at heliocentric distances $>70$ AU in the Kuiper Belt. We show that the already flat distribution of these objects must flatten further due to non-spherically symmetric distribution of matter in the Kuiper Belt. Moreover the dynamical drag, produced by dynamical friction, causes objects of masses $\geq 10^{24} g$ to lose angular momentum and to fall through more central regions in a timescale $\approx 10^9 yr$. This mechanism is able to transport inwards objects of the size of Pluto, supposing it was created beyond 50 AU, according to a Stern & Colwell's (1997b) suggestion.
[{'version': 'v1', 'created': 'Mon, 3 May 1999 18:52:41 GMT'} {'version': 'v2', 'created': 'Tue, 4 May 1999 10:22:16 GMT'}]
2007-05-23
[array(['Del Popolo', 'A.', ''], dtype=object) array(['Spedicato', 'E.', ''], dtype=object) array(['Gambera', 'M.', ''], dtype=object)]
19,375
1809.02254
Robin Kothari
Mark Bun, Robin Kothari, Justin Thaler
Quantum algorithms and approximating polynomials for composed functions with shared inputs
v2: 31 pages; 1 figure. This update includes an additional result on lower bounds for AC$^0 \circ \oplus$ computing the Inner Product function on average. v3: Minor changes. Accepted to Quantum
Quantum 5, 543 (2021)
10.22331/q-2021-09-16-543
null
quant-ph cs.CC
http://creativecommons.org/licenses/by/4.0/
We give new quantum algorithms for evaluating composed functions whose inputs may be shared between bottom-level gates. Let $f$ be an $m$-bit Boolean function and consider an $n$-bit function $F$ obtained by applying $f$ to conjunctions of possibly overlapping subsets of $n$ variables. If $f$ has quantum query complexity $Q(f)$, we give an algorithm for evaluating $F$ using $\tilde{O}(\sqrt{Q(f) \cdot n})$ quantum queries. This improves on the bound of $O(Q(f) \cdot \sqrt{n})$ that follows by treating each conjunction independently, and our bound is tight for worst-case choices of $f$. Using completely different techniques, we prove a similar tight composition theorem for the approximate degree of $f$. By recursively applying our composition theorems, we obtain a nearly optimal $\tilde{O}(n^{1-2^{-d}})$ upper bound on the quantum query complexity and approximate degree of linear-size depth-$d$ AC$^0$ circuits. As a consequence, such circuits can be PAC learned in subexponential time, even in the challenging agnostic setting. Prior to our work, a subexponential-time algorithm was not known even for linear-size depth-3 AC$^0$ circuits. As an additional consequence, we show that AC$^0 \circ \oplus$ circuits of depth $d+1$ require size $\tilde{\Omega}(n^{1/(1- 2^{-d})}) \geq \omega(n^{1+ 2^{-d}} )$ to compute the Inner Product function even on average. The previous best size lower bound was $\Omega(n^{1+4^{-(d+1)}})$ and only held in the worst case (Cheraghchi et al., JCSS 2018).
[{'version': 'v1', 'created': 'Thu, 6 Sep 2018 23:58:47 GMT'} {'version': 'v2', 'created': 'Sun, 29 Mar 2020 22:11:31 GMT'} {'version': 'v3', 'created': 'Fri, 10 Sep 2021 17:58:37 GMT'}]
2021-09-22
[array(['Bun', 'Mark', ''], dtype=object) array(['Kothari', 'Robin', ''], dtype=object) array(['Thaler', 'Justin', ''], dtype=object)]
19,376
2204.06344
Elie Atallah
Elie Atallah, Nazanin Rahnavard, and Qiyu Sun
CoDGraD: A Code-based Distributed Gradient Descent Scheme for Decentralized Convex Optimization
15 pages, 4 figures
null
null
null
eess.SY cs.SY math.OC
http://creativecommons.org/licenses/by/4.0/
In this paper, we consider a large network containing many regions such that each region is equipped with a worker with some data processing and communication capability. For such a network, some workers may become stragglers due to the failure or heavy delay on computing or communicating. To resolve the above straggling problem, a coded scheme that introduces certain redundancy for every worker was recently proposed, and a gradient coding paradigm was developed to solve convex optimization problems when the network has a centralized fusion center. In this paper, we propose an iterative distributed algorithm, referred as Code-Based Distributed Gradient Descent algorithm (CoDGraD), to solve convex optimization problems over distributed networks. In each iteration of the proposed algorithm, an active worker shares the coded local gradient and approximated solution of the convex optimization problem with non-straggling workers at the adjacent regions only. In this paper, we also provide the consensus and convergence analysis for the CoDGraD algorithm and we demonstrate its performance via numerical simulations.
[{'version': 'v1', 'created': 'Wed, 13 Apr 2022 12:51:22 GMT'}]
2022-04-14
[array(['Atallah', 'Elie', ''], dtype=object) array(['Rahnavard', 'Nazanin', ''], dtype=object) array(['Sun', 'Qiyu', ''], dtype=object)]
19,377
1909.01994
Jacob Rafati
Jacob Rafati and Roummel F. Marcia
Quasi-Newton Optimization Methods For Deep Learning Applications
arXiv admin note: substantial text overlap with arXiv:1811.02693
null
null
null
cs.LG math.OC stat.ML
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Deep learning algorithms often require solving a highly non-linear and nonconvex unconstrained optimization problem. Methods for solving optimization problems in large-scale machine learning, such as deep learning and deep reinforcement learning (RL), are generally restricted to the class of first-order algorithms, like stochastic gradient descent (SGD). While SGD iterates are inexpensive to compute, they have slow theoretical convergence rates. Furthermore, they require exhaustive trial-and-error to fine-tune many learning parameters. Using second-order curvature information to find search directions can help with more robust convergence for non-convex optimization problems. However, computing Hessian matrices for large-scale problems is not computationally practical. Alternatively, quasi-Newton methods construct an approximate of the Hessian matrix to build a quadratic model of the objective function. Quasi-Newton methods, like SGD, require only first-order gradient information, but they can result in superlinear convergence, which makes them attractive alternatives to SGD. The limited-memory Broyden-Fletcher-Goldfarb-Shanno (L-BFGS) approach is one of the most popular quasi-Newton methods that construct positive definite Hessian approximations. In this chapter, we propose efficient optimization methods based on L-BFGS quasi-Newton methods using line search and trust-region strategies. Our methods bridge the disparity between first- and second-order methods by using gradient information to calculate low-rank updates to Hessian approximations. We provide formal convergence analysis of these methods as well as empirical results on deep learning applications, such as image classification tasks and deep reinforcement learning on a set of ATARI 2600 video games. Our results show a robust convergence with preferred generalization characteristics as well as fast training time.
[{'version': 'v1', 'created': 'Wed, 4 Sep 2019 15:52:08 GMT'}]
2019-09-06
[array(['Rafati', 'Jacob', ''], dtype=object) array(['Marcia', 'Roummel F.', ''], dtype=object)]
19,378
astro-ph/0311541
Nuno C. Santos
N. C. Santos (1 and 2), G. Israelian (3), M. Mayor (2) ((1) Observatorio Astronomico de Lisboa, Portugal (2) Observatoire de Geneve, Switzerland (3) Instituto de Astrofisia de Canarias, Spain)
Spectroscopic [Fe/H] for 98 extra-solar planet-host stars: Exploring the probability of planet formation
15 pages, 9 figures, Accepted for publication in A&A; Replaced after language editing
Astron.Astrophys.415:1153-1166,2004
10.1051/0004-6361:20034469
null
astro-ph
null
We present stellar parameters and metallicities, obtained from a detailed spectroscopic analysis, for a large sample of 98 stars known to be orbited by planetary mass companions (almost all known targets), as well as for a volume-limited sample of 41 stars not known to host any planet. For most of the stars the stellar parameters are revised versions of the ones presented in our previous works. However, we also present parameters for 18 stars with planets not previously published, and a compilation of stellar parameters for the remaining 4 planet-hosts for which we could not obtain a spectrum. A comparison of our stellar parameters with values of Teff, log(g), and [Fe/H] available in the literature shows a remarkable agreement. The derived [Fe/H] values are then used to confirm the previously known result that planets are more prevalent around metal-rich stars. Furthermore, we confirm that the frequency of planets is a strongly rising function of the stellar metallicity, at least for stars with [Fe/H]>0. While only about 3% of the solar metallicity stars in the CORALIE planet search sample were found to be orbited by a planet, this number increases to more than 25% for stars with [Fe/H] above +0.3. Curiously, our results also suggest that these percentages might remain relatively constant for values of [Fe/H] lower than about solar, increasing then linearly with the mass fraction of heavy elements. These results are discussed in the context of the theories of planetary formation.
[{'version': 'v1', 'created': 'Mon, 24 Nov 2003 17:55:13 GMT'} {'version': 'v2', 'created': 'Wed, 26 Nov 2003 09:44:50 GMT'}]
2011-05-05
[array(['Santos', 'N. C.', '', '1 and 2'], dtype=object) array(['Israelian', 'G.', ''], dtype=object) array(['Mayor', 'M.', ''], dtype=object)]
19,379
1211.7097
Velimir Ilic
Velimir M. Ilic, Miomir S. Stankovic, and Edin H. Mulalic
Comments on "Generalization of Shannon-Khinchin axioms to nonextensive systems and the uniqueness theorem for the nonextensive entropy"
4 pages
null
null
null
math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Recently, Suyari has proposed a generalization of Shannon-Khinchin axioms, which determines a class of entropies containing the well-known Tsalis and Havrda-Charvat entropies [H. Suyari, IEEE Trans. Inf. Theory, vol. 50, pp. 1783-1787, Aug. 2004]. In this comment we show that the class of entropy functions determined by Suyari's axioms is wider than the one proposed by Suyari and give a counterexample. Additionally, we generalize Suyari's axioms characterizing recently introduced class of entropies obtained by averaging pseudoadditive information content introduced in [V. Ilic and M. Stankovic, "Comments on "Nonextensive Entropies derived from Form Invariance of Pseudoadditivity"" Submited, 2012].
[{'version': 'v1', 'created': 'Thu, 29 Nov 2012 21:36:12 GMT'}]
2012-12-03
[array(['Ilic', 'Velimir M.', ''], dtype=object) array(['Stankovic', 'Miomir S.', ''], dtype=object) array(['Mulalic', 'Edin H.', ''], dtype=object)]
19,380
2206.04818
Richard K Bowles
Josh M. Gramlich, Mahdi Zarif and Richard K. Bowles
Is there a Granular Potential?
11 Pages, 7 Figures. Extended Introduction and Discussion. New section on Measuring granular potential
null
null
null
cond-mat.soft cond-mat.stat-mech
http://creativecommons.org/licenses/by/4.0/
Granular materials, such as sand or grain, exhibit many structural and dynamic characteristics similar to those observed in molecular systems, despite temperature playing no role in their properties. This has led to an effort to develop a statistical mechanics for granular materials that has focused on establishing an equivalent to the microcanonical ensemble and a temperature-like thermodynamic variable. Here, we expand on these ideas by introducing a granular potential into the Edwards ensemble, as an analogue to the chemical potential, and explore its properties using a simple model of a granular system. A simple kinetic Monte Carlo simulation of the model shows the effect of mass transport leading to equilibrium and how this is connected to the redistribution of volume in the system. An exact analytical treatment of the model shows that the compactivity and the ratio of the granular potential to the compactivity determine the equilibrium between two open systems that are able to exchange volume and particles, and that mass moves from high to low values of this ratio. Analysis of the granular potential shows that adding a particle to the system increases the entropy at high compactivity, but decreases the entropy at low compactivity. Finally, we demonstrate the use of a small system thermodynamics method for the measurement of granular potential differences.
[{'version': 'v1', 'created': 'Fri, 10 Jun 2022 00:29:08 GMT'} {'version': 'v2', 'created': 'Wed, 18 Jan 2023 04:25:43 GMT'}]
2023-01-19
[array(['Gramlich', 'Josh M.', ''], dtype=object) array(['Zarif', 'Mahdi', ''], dtype=object) array(['Bowles', 'Richard K.', ''], dtype=object)]
19,381
2301.11489
Megan Leszczynski
Megan Leszczynski, Ravi Ganti, Shu Zhang, Krisztian Balog, Filip Radlinski, Fernando Pereira, Arun Tejasvi Chaganty
Generating Synthetic Data for Conversational Music Recommendation Using Random Walks and Language Models
null
null
null
null
cs.IR cs.CL
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Conversational recommendation systems (CRSs) enable users to use natural language feedback to control their recommendations, overcoming many of the challenges of traditional recommendation systems. However, the practical adoption of CRSs remains limited due to a lack of rich and diverse conversational training data that pairs user utterances with recommendations. To address this problem, we introduce a new method to generate synthetic training data by transforming curated item collections, such as playlists or movie watch lists, into item-seeking conversations. First, we use a biased random walk to generate a sequence of slates, or sets of item recommendations; then, we use a language model to generate corresponding user utterances. We demonstrate our approach by generating a conversational music recommendation dataset with over one million conversations, which were found to be consistent with relevant recommendations by a crowdsourced evaluation. Using the synthetic data to train a CRS, we significantly outperform standard retrieval baselines in offline and online evaluations.
[{'version': 'v1', 'created': 'Fri, 27 Jan 2023 01:54:16 GMT'}]
2023-01-30
[array(['Leszczynski', 'Megan', ''], dtype=object) array(['Ganti', 'Ravi', ''], dtype=object) array(['Zhang', 'Shu', ''], dtype=object) array(['Balog', 'Krisztian', ''], dtype=object) array(['Radlinski', 'Filip', ''], dtype=object) array(['Pereira', 'Fernando', ''], dtype=object) array(['Chaganty', 'Arun Tejasvi', ''], dtype=object)]
19,382
2106.13707
Rashed Shelim
Rashed Shelim and Ahmed S. Ibrahim
A Fast Graph Kernel Based Classification Method for Wireless Link Scheduling on Riemannian Manifold
null
null
null
null
eess.SP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we propose a novel graph kernel method for the wireless link scheduling problem in device-to-device (D2D) networks on Riemannian manifold. The link scheduling problem can be considered as a binary classification problem since each D2D pair can only hold the state active or inactive. Our goal is to learn a novel metric that facilitates the design of an efficient but less computationally demanding machine learning (ML) solution for the binary classification task of link scheduling problem that requires no channel state information (CSI) and a fewer number of training samples as opposed to other benchmark ML algorithms. To this aim, we first represent the wireless D2D network as a graph and model the features of each D2D pair, including its communication and interference links, as regularized (i.e., positively-shifted) Laplacian matrices which are symmetric positive definite (SPD) one. By doing so, we represent the feature information of each D2D pair as a point on the SPD manifold, and we analyze the topology through Riemannian geometry. We compute the Riemannian metric, e.g., Log-Euclidean metric (LEM), which are suitable distance measures between the regularized Laplacian matrices. The LEM is then utilized to define a positive definite graph kernel for the binary classification of the link scheduling decisions. Simulation results demonstrate that the proposed graph Kernel-based method is computationally less demanding and achieves a sum rate of more than 95% of benchmark algorithm FPLinQ [1] for 10 D2D pairs without using CSI and less than a hundred training network layouts.
[{'version': 'v1', 'created': 'Fri, 25 Jun 2021 15:46:26 GMT'}]
2021-06-28
[array(['Shelim', 'Rashed', ''], dtype=object) array(['Ibrahim', 'Ahmed S.', ''], dtype=object)]
19,383
1008.1585
Masatoshi Imanishi
Masatoshi Imanishi (1), Takao Nakagawa (2), Mai Shirahata (2), Yoichi Ohyama (3), Takashi Onaka (4) ((1) Subaru/NAOJ, (2) ISAS/JAXA, (3) ASIAA/Taiwan, (4) Univ. of Tokyo)
AKARI IRC infrared 2.5-5 micron spectroscopy of a large sample of luminous infrared galaxies
39 pages, 10 figures, accepted for publication in ApJ (September 20, 2010, V721 -1 issue)
null
10.1088/0004-637X/721/2/1233
null
astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We present the results of our systematic infrared 2.5-5 micron spectroscopy of 60 luminous infrared galaxies (LIRGs) with infrared luminosities L(IR) = 10^11-12 Lsun, and 54 ultraluminous infrared galaxies (ULIRGs) with L(IR) > 10^12 Lsun, using AKARI IRC. AKARI IRC slit-less spectroscopy allows us to probe the full range of emission from these galaxies, including spatially extended components. The 3.3 micron polycyclic aromatic hydrocarbon (PAH) emission features, hydrogen recombination emission lines, and various absorption features are detected and used to investigate the properties of these galaxies. Because of the relatively small effect of dust extinction in the infrared range, quantitative discussion of these dusty galaxy populations is possible. For sources with clearly detectable Br beta (2.63 micron) and Br alpha (4.05 micron) emission lines, the flux ratios are found to be similar to that predicted by case B theory. Starburst luminosities are estimated from both 3.3 micron PAH and Br alpha emission, which roughly agree with each other. In addition to the detected starburst activity, a significant fraction of the observed sources display signatures of obscured AGNs, such as low PAH equivalent widths, large optical depths of dust absorption features, and red continuum emission. The energetic importance of optically elusive buried AGNs in optically non-Seyfert galaxies tends to increase with increasing galaxy infrared luminosity, from LIRGs to ULIRGs.
[{'version': 'v1', 'created': 'Mon, 9 Aug 2010 20:04:37 GMT'} {'version': 'v2', 'created': 'Fri, 20 Aug 2010 00:50:46 GMT'}]
2015-05-19
[array(['Imanishi', 'Masatoshi', ''], dtype=object) array(['Nakagawa', 'Takao', ''], dtype=object) array(['Shirahata', 'Mai', ''], dtype=object) array(['Ohyama', 'Yoichi', ''], dtype=object) array(['Onaka', 'Takashi', ''], dtype=object)]
19,384
hep-ph/9409219
Klaus Geiger
Klaus Geiger
High Density QCD and Entropy Production at Heavy Ion Colliders
(CERN-TH. 7429/94), Latex file, 10 pages, with 6 figures available upon request. encoded with uufiles
null
null
null
hep-ph
null
The role of entropy production in the context of probing QCD properties at high densities and finite temperatures in ultra-relativistic collisions of heavy nuclei is inspected. It is argued that the entropy generated in these reactions provides a powerful tool to investigate the space-time evolution and the question whether and how a deconfined plasma of quarks and gluons is formed. I will address the questions how entropy is produced, and how it is measurable. The uncertainties in predicting the different contributions to the total entropy and particle multiplicities during the course of heavy ion collisions are also discussed.
[{'version': 'v1', 'created': 'Sun, 4 Sep 1994 17:18:19 GMT'}]
2009-09-25
[array(['Geiger', 'Klaus', ''], dtype=object)]
19,385
1307.3149
Maxim Zabzine
Jian Qiu and Maxim Zabzine
5D Super Yang-Mills on $Y^{p,q}$ Sasaki-Einstein manifolds
43 pages, typos and mistakes corrected
Commun.Math.Phys. 333 (2015) 861-904
10.1007/s00220-014-2194-7
null
hep-th math-ph math.MP math.SG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
On any simply connected Sasaki-Einstein five dimensional manifold one can construct a super Yang-Mills theory which preserves at least two supersymmetries. We study the special case of toric Sasaki-Einstein manifolds known as $Y^{p,q}$ manifolds. We use the localisation technique to compute the full perturbative part of the partition function. The full equivariant result is expressed in terms of certain special function which appears to be a curious generalisation of the triple sine function. As an application of our general result we study the large $N$ behaviour for the case of single hypermultiplet in adjoint representation and we derive the $N^3$-behaviour in this case.
[{'version': 'v1', 'created': 'Thu, 11 Jul 2013 15:52:54 GMT'} {'version': 'v2', 'created': 'Mon, 19 Aug 2013 12:30:47 GMT'} {'version': 'v3', 'created': 'Fri, 27 Feb 2015 12:48:40 GMT'}]
2015-03-02
[array(['Qiu', 'Jian', ''], dtype=object) array(['Zabzine', 'Maxim', ''], dtype=object)]
19,386
math/0410360
Tyler J. Jarvis
Tyler J. Jarvis, William E. Lang, Nansen Petrosyan, Gretchen Rimmasch, Julie Rogers, Erin D. Summers
Classification of Singular Fibres on Rational Elliptic Surfaces in Characteristic Three
40 Pages. Minor typos corrected
Communications in Algebra 33: 4533--4566 (2005)
10.1080/00927870500274861
null
math.AG
null
We determine and list all possible configurations of singular fibres on rational elliptic surfaces in characteristic three. In total, we find that 267 distinct configurations exist. This result complements Miranda and Persson's classification in characteristic zero, and Lang's classification in characteristic two.
[{'version': 'v1', 'created': 'Fri, 15 Oct 2004 23:32:07 GMT'} {'version': 'v2', 'created': 'Sat, 12 Mar 2005 21:51:32 GMT'}]
2007-05-23
[array(['Jarvis', 'Tyler J.', ''], dtype=object) array(['Lang', 'William E.', ''], dtype=object) array(['Petrosyan', 'Nansen', ''], dtype=object) array(['Rimmasch', 'Gretchen', ''], dtype=object) array(['Rogers', 'Julie', ''], dtype=object) array(['Summers', 'Erin D.', ''], dtype=object)]
19,387
2005.00947
Rui Sun
David Simchi-Levi, Rui Sun, Huanan Zhang
Online Learning and Optimization for Revenue Management Problems with Add-on Discounts
null
null
null
null
cs.DS cs.LG math.OC stat.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study in this paper a revenue management problem with add-on discounts. The problem is motivated by the practice in the video game industry, where a retailer offers discounts on selected supportive products (e.g. video games) to customers who have also purchased the core products (e.g. video game consoles). We formulate this problem as an optimization problem to determine the prices of different products and the selection of products with add-on discounts. To overcome the computational challenge of this optimization problem, we propose an efficient FPTAS algorithm that can solve the problem approximately to any desired accuracy. Moreover, we consider the revenue management problem in the setting where the retailer has no prior knowledge of the demand functions of different products. To resolve this problem, we propose a UCB-based learning algorithm that uses the FPTAS optimization algorithm as a subroutine. We show that our learning algorithm can converge to the optimal algorithm that has access to the true demand functions, and we prove that the convergence rate is tight up to a certain logarithmic term. In addition, we conduct numerical experiments with the real-world transaction data we collect from a popular video gaming brand's online store on Tmall.com. The experiment results illustrate our learning algorithm's robust performance and fast convergence in various scenarios. We also compare our algorithm with the optimal policy that does not use any add-on discount, and the results show the advantages of using the add-on discount strategy in practice.
[{'version': 'v1', 'created': 'Sat, 2 May 2020 23:54:17 GMT'}]
2020-05-05
[array(['Simchi-Levi', 'David', ''], dtype=object) array(['Sun', 'Rui', ''], dtype=object) array(['Zhang', 'Huanan', ''], dtype=object)]
19,388
1705.06589
Mortaza Abtahi Dr.
Mortaza Abtahi and Sara Farhangi
A Characterization of Polynomially Convex Sets in Banach Spaces
to appear in Results in Mathemarics
null
null
null
math.FA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Let $E$ be a Banach space and $\X$ be the closed unit ball of the dual space $E^*$. For a compact set $K$ in $E$, we prove that $K$ is polynomially convex in $E$ if and only if there exist a unital commutative Banach algebra $A$ and a continuous function $f:\X\to A$ such that (1) $A$ is generated by $f(\X)$, (2) the character space of $A$ is homeomorphic to $K$, and (3) $K=\vsp(f)$ the joint spectrum of $f$. In case $E=\c(X)$, where $X$ is a compact Hausdorff space, we will see that $\X$ can be replaced by $X$.
[{'version': 'v1', 'created': 'Mon, 15 May 2017 08:04:40 GMT'}]
2017-05-19
[array(['Abtahi', 'Mortaza', ''], dtype=object) array(['Farhangi', 'Sara', ''], dtype=object)]
19,389
quant-ph/0211183
Natalia Yakovleva
A.R. Kessel
Stabilization of Quantum Computer Calculation Basis by Qubit Encoding in Virtual Spin Representation
null
null
null
null
quant-ph
null
It is proposed to map the quantum information qubit not to individual spin 1/2 states, but to the collective spin states being eigenfunctions of the Hamiltonian including spin-spin interactions, which may be not small. Such an approach allows to introduce more stable calculation basis for quantum computer based on the solid state NMR systems.
[{'version': 'v1', 'created': 'Wed, 27 Nov 2002 15:57:43 GMT'}]
2007-05-23
[array(['Kessel', 'A. R.', ''], dtype=object)]
19,390
2112.10879
Tuomo Kuusi
Gohar Aleksanyan and Tuomo Kuusi
Quantitative homogenization for the obstacle problem and its free boundary
42 pages, 1 figure
null
null
null
math.AP
http://creativecommons.org/licenses/by/4.0/
In this manuscript we prove quantitative homogenization results for the obstacle problem with bounded measurable coefficients. As a consequence, large-scale regularity results both for the solution and the free boundary for the heterogeneous obstacle problem are derived.
[{'version': 'v1', 'created': 'Mon, 20 Dec 2021 21:46:36 GMT'}]
2021-12-22
[array(['Aleksanyan', 'Gohar', ''], dtype=object) array(['Kuusi', 'Tuomo', ''], dtype=object)]
19,391
1111.3376
Christopher Quinn
Dustin G. Mixon, Christopher J. Quinn, Negar Kiyavash, and Matthew Fickus
Fingerprinting with Equiangular Tight Frames
10 pages, 6 figures, presented in part at ICASSP 2011 and SPIE 2011
null
null
null
cs.IT cs.MM math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Digital fingerprinting is a framework for marking media files, such as images, music, or movies, with user-specific signatures to deter illegal distribution. Multiple users can collude to produce a forgery that can potentially overcome a fingerprinting system. This paper proposes an equiangular tight frame fingerprint design which is robust to such collusion attacks. We motivate this design by considering digital fingerprinting in terms of compressed sensing. The attack is modeled as linear averaging of multiple marked copies before adding a Gaussian noise vector. The content owner can then determine guilt by exploiting correlation between each user's fingerprint and the forged copy. The worst-case error probability of this detection scheme is analyzed and bounded. Simulation results demonstrate the average-case performance is similar to the performance of orthogonal and simplex fingerprint designs, while accommodating several times as many users.
[{'version': 'v1', 'created': 'Mon, 14 Nov 2011 21:44:55 GMT'}]
2011-11-16
[array(['Mixon', 'Dustin G.', ''], dtype=object) array(['Quinn', 'Christopher J.', ''], dtype=object) array(['Kiyavash', 'Negar', ''], dtype=object) array(['Fickus', 'Matthew', ''], dtype=object)]
19,392
chao-dyn/9405005
Bruce W. Roberts
Bruce W. Roberts, Eberhard Bodenschatz, and James P. Sethna
Defect--Defect Correlation Functions, Generic Scale Invariance, and the Complex Ginzburg--Landau Equation
12 pages and 3 included figures, RevTeX
null
null
CULASSP-4269
chao-dyn nlin.CD
null
We present a calculation of defect--defect correlation functions in the defect turbulence regime of the complex Ginzburg--Landau equation. Our results do not agree with the predictions of generic scale invariance. Using the topological nature of the defects, we prove that defect--defect correlations cannot decay as slowly as predicted by generic scale invariance
[{'version': 'v1', 'created': 'Wed, 11 May 1994 12:08:43 GMT'}]
2008-02-03
[array(['Roberts', 'Bruce W.', ''], dtype=object) array(['Bodenschatz', 'Eberhard', ''], dtype=object) array(['Sethna', 'James P.', ''], dtype=object)]
19,393
cond-mat/0504638
Pavel Rodin
Pavel Rodin and Igor Grekhov
Dynamic avalanche breakdown of a p-n junction: deterministic triggering of a plane streamer front
4 pages, 2 figures
Appl. Phys. Lett. 86, 243504 (2005)
10.1063/1.1947915
null
cond-mat.mtrl-sci
null
We discuss the dynamic impact ionization breakdown of high voltage p-n junction which occurs when the electric field is increased above the threshold of avalanche impact ionization on a time scale smaller than the inverse thermogeneration rate. The avalanche-to-streamer transition characterized by generation of dense electron-hole plasma capable to screen the applied external electric field occurs in such regimes. We argue that the experimentally observed deterministic triggering of the plane streamer front at the electric field strength above the threshold of avalanche impact ionization but yet below the threshold of band-to-band tunneling is generally caused by field-enhanced ionization of deep-level centers. We suggest that the process-induced sulfur centers and native defects such as EL2, HB2, HB5 centers initiate the front in Si and GaAs structures, respectively. In deep-level free structures the plane streamer front is triggered by Zener band-to-band tunneling.
[{'version': 'v1', 'created': 'Mon, 25 Apr 2005 17:29:32 GMT'}]
2009-11-11
[array(['Rodin', 'Pavel', ''], dtype=object) array(['Grekhov', 'Igor', ''], dtype=object)]
19,394
1308.4075
Atlas Publications
ATLAS Collaboration
Search for microscopic black holes in a like-sign dimuon final state using large track multiplicity with the ATLAS detector
10 pages plus author list (22 pages total), 7 figures, 4 tables, submitted to PRD, All figures including auxiliary figures are available at http://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/EXOT-2013-04/
Phys. Rev. D 88 (2013) 072001
10.1103/PhysRevD.88.072001
CERN-PH-EP-2013-120
hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A search is presented for microscopic black holes in a like-sign dimuon final state in proton--proton collisions at sqrt(s)= 8 TeV. The data were collected with the ATLAS detector at the Large Hadron Collider in 2012 and correspond to an integrated luminosity of 20.3 fb-1. Using a high track multiplicity requirement, 0.6 +- 0.2 background events from Standard Model processes are predicted and none observed. This result is interpreted in the context of low-scale gravity models and 95% CL lower limits on microscopic black hole masses are set for different model assumptions.
[{'version': 'v1', 'created': 'Mon, 19 Aug 2013 17:03:18 GMT'}]
2013-10-03
[array(['ATLAS Collaboration', '', ''], dtype=object)]
19,395
2010.00406
Aaron Defazio
Aaron Defazio
Momentum via Primal Averaging: Theoretical Insights and Learning Rate Schedules for Non-Convex Optimization
null
null
null
null
cs.LG math.OC stat.ML
http://creativecommons.org/licenses/by-sa/4.0/
Momentum methods are now used pervasively within the machine learning community for training non-convex models such as deep neural networks. Empirically, they out perform traditional stochastic gradient descent (SGD) approaches. In this work we develop a Lyapunov analysis of SGD with momentum (SGD+M), by utilizing a equivalent rewriting of the method known as the stochastic primal averaging (SPA) form. This analysis is much tighter than previous theory in the non-convex case, and due to this we are able to give precise insights into when SGD+M may out-perform SGD, and what hyper-parameter schedules will work and why.
[{'version': 'v1', 'created': 'Thu, 1 Oct 2020 13:46:32 GMT'} {'version': 'v2', 'created': 'Tue, 3 Nov 2020 22:05:04 GMT'} {'version': 'v3', 'created': 'Tue, 23 Feb 2021 19:49:57 GMT'} {'version': 'v4', 'created': 'Tue, 1 Jun 2021 17:53:38 GMT'}]
2021-06-02
[array(['Defazio', 'Aaron', ''], dtype=object)]
19,396
1701.02591
Kyle Augustson
Kyle Augustson
Dynamos and Differential Rotation: Advances at the Crossroads of Analytics, Numerics, and Observations
16 pages, 14 figures, Joint TASC2-KASC9 Workshop and SPACEINN-HELAS8 Conference: Seismology of the Sun and the Distant Stars 2016
null
10.1051/epjconf/201716002010
null
astro-ph.SR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The recent observational, theoretical, and numerical progress made in understanding stellar magnetism is discussed. Particularly, this review will cover the physical processes thought to be at the origin of these magnetic fields and their variability, namely dynamo action arising from the interaction between convection, rotation, radiation and magnetic fields. Some care will be taken to cover recent analytical advances regarding the dynamics and magnetism of radiative interiors, including some thoughts on the role of a tachocline. Moreover, recent and rapidly advancing numerical modeling of convective dynamos will be discussed, looking at rapidly rotating convective systems, grand minima and scaling laws for magnetic field strength. These topics are linked to observations or their observational implications.
[{'version': 'v1', 'created': 'Tue, 10 Jan 2017 13:56:59 GMT'}]
2017-11-08
[array(['Augustson', 'Kyle', ''], dtype=object)]
19,397
hep-ph/9703321
Koichi Yoshioka
Masako Bando, Joe Sato and Koichi Yoshioka
Infra-Red Fixed Points in an Asymptotically Non-Free Theory
12 pages + 8 eps figures, LaTeX, typos corrected, revised version to be published
Prog.Theor.Phys. 98 (1997) 169-176
10.1143/PTP.98.169
ICRR-Report-384-97-7, KUNS-1437
hep-ph
null
We investigate the infrared fixed point structure in asymptotically free and asymptotically non-free theory. We find that the ratios of couplings converge strongly to their infrared fixed points in the asymptotically non-free theory.
[{'version': 'v1', 'created': 'Fri, 14 Mar 1997 07:32:33 GMT'} {'version': 'v2', 'created': 'Thu, 10 Apr 1997 12:28:41 GMT'} {'version': 'v3', 'created': 'Mon, 9 Jun 1997 11:28:21 GMT'}]
2009-10-30
[array(['Bando', 'Masako', ''], dtype=object) array(['Sato', 'Joe', ''], dtype=object) array(['Yoshioka', 'Koichi', ''], dtype=object)]
19,398
0906.5060
R Doomun
Prof. Dhananjay R. Kalbande, Dr. G. T. Thampi, Mr. Manish Singh
Incidence Handling and Response System
8 Pages, International Journal of Computer Science and Information Security (IJCSIS)
IJCSIS June 2009 Issue, Vol. 2, No. 1
null
null
cs.CR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A computer network can be attacked in a number of ways. The security-related threats have become not only numerous but also diverse and they may also come in the form of blended attacks. It becomes difficult for any security system to block all types of attacks. This gives rise to the need of an incidence handling capability which is necessary for rapidly detecting incidents, minimizing loss and destruction, mitigating the weaknesses that were exploited and restoring the computing services. Incidence response has always been an important aspect of information security but it is often overlooked by security administrators. in this paper, we propose an automated system which will handle the security threats and make the computer network capable enough to withstand any kind of attack. we also present the state-of-the-art technology in computer, network and software which is required to build such a system.
[{'version': 'v1', 'created': 'Sat, 27 Jun 2009 10:10:18 GMT'}]
2009-06-30
[array(['Kalbande', 'Prof. Dhananjay R.', ''], dtype=object) array(['Thampi', 'Dr. G. T.', ''], dtype=object) array(['Singh', 'Mr. Manish', ''], dtype=object)]
19,399
math/0106200
Max Neumann-Coto
Max Neumann-Coto
A characterization of shortest geodesics on surfaces
Published by Algebraic and Geometric Topology at http://www.maths.warwick.ac.uk/agt/AGTVol1/agt-1-17.abs.html
Algebr. Geom. Topol. 1 (2001) 349-368
10.2140/agt.2001.1.349
null
math.GT math.MG
null
Any finite configuration of curves with minimal intersections on a surface is a configuration of shortest geodesics for some Riemannian metric on the surface. The metric can be chosen to make the lengths of these geodesics equal to the number of intersections along them.
[{'version': 'v1', 'created': 'Sun, 24 Jun 2001 14:09:30 GMT'}]
2014-10-01
[array(['Neumann-Coto', 'Max', ''], dtype=object)]