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\section{Introduction and Main results}
Consider the stable solution of the following equation
\begin{equation}\label{8LE}
(-\Delta)^s u=|u|^{p-1}u\;\;\;\;\hbox{in}\;\;\;\;\; \R^n,
\end{equation}
where $(-\Delta)^s$ is the fractional Laplacian operator for $2<s<3$.
\vskip0.1in
The motivation of ... | {'timestamp': '2016-09-05T02:06:08', 'yymm': '1609', 'arxiv_id': '1609.00705', 'language': 'en', 'url': 'https://arxiv.org/abs/1609.00705'} |
\subsection{#2}{#4}\par\hfill{\arx{#1}}\par\hfill\emph{#3}}
\nc{\arXiv}[3]{\subsection{#2} {#3}, \arx{#1}\par\hfill}
\nc{\DOIpaper}[5]{\subsection{#2}{#4}\par\hfill{\url{http://dx.doi.org/#1}}\par\hfill\emph{#3}}
\nc{\AMSPaper}[5]{\subsection{#3}{#5}\par\hfill{\url{#1}}\par\hfill\emph{#4}\par\hfill{#2}}
\nc{\nAMSPa... | {'timestamp': '2016-12-23T02:00:36', 'yymm': '1612', 'arxiv_id': '1612.07354', 'language': 'en', 'url': 'https://arxiv.org/abs/1612.07354'} |
\section{Introduction}
Extreme value theory is used in understanding unlikely observations. It provides a theoretical framework that classifies distributions according to their tail behavior and explains asymptotic properties of the extreme order statistics. It also provides statistical estimators for different intere... | {'timestamp': '2016-01-13T02:10:47', 'yymm': '1511', 'arxiv_id': '1511.08627', 'language': 'en', 'url': 'https://arxiv.org/abs/1511.08627'} |
\section{Introduction}
In the geometric theory of holomorphic functions on complex manifolds, the
concept of invariant metrics plays an important role.
Invariant metrics refer to Finsler or Hermitian metrics which are invariant with respect to biholomorphic mappings.
Within the theory of several complex variables ... | {'timestamp': '2022-02-14T02:08:49', 'yymm': '2202', 'arxiv_id': '2202.05473', 'language': 'en', 'url': 'https://arxiv.org/abs/2202.05473'} |
\section{Introduction}
Polynomial interpolation is a classical computational problem considered in numerical mathematics: given a set of points and values find a polynomial of a given degree
that assumes given values at given points. A common interpretation is that a polynomial is fitted to some observational data. It... | {'timestamp': '2019-07-25T02:01:38', 'yymm': '1907', 'arxiv_id': '1907.09371', 'language': 'en', 'url': 'https://arxiv.org/abs/1907.09371'} |
\section{Introduction}
Security on Android is enforced via permissions giving access to
resources on the device. These permissions are often too coarse and
their attribution is based on an all-or-nothing decision in the vast
majority of Android versions in actual use. Additional security policies can be
prescribed... | {'timestamp': '2016-12-23T02:05:08', 'yymm': '1612', 'arxiv_id': '1612.07586', 'language': 'en', 'url': 'https://arxiv.org/abs/1612.07586'} |
\section{Introduction}
A connection between string theory on $AdS_{5}\times S^{5}$ and super Yang Mills theory in
four dimensions was proposed by J. Maldacena some years ago \cite{Maldacena:1998re}. More
recently, this result gave rise to what is currently called the AdS/CFT conjecture. However
the name has been enlar... | {'timestamp': '2007-02-02T19:49:23', 'yymm': '0612', 'arxiv_id': 'hep-th/0612028', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-th/0612028'} |
\section{Appendix} \label{A2}
To simulate death times of annuitants, we notice that once a sample of the mortality intensity is obtained, the Cox process becomes an inhomogeneous Poisson process and the first jump times, which are interpreted as death times, can be simulated as follows (see e.g. \cite{BrigoMe07}):
\be... | {'timestamp': '2015-08-04T02:04:48', 'yymm': '1508', 'arxiv_id': '1508.00090', 'language': 'en', 'url': 'https://arxiv.org/abs/1508.00090'} |
\section{Introduction}\label{sec:introduction}
\setcounter{equation}{0}
{\it Introduction.} The Standard Model (SM) explanation for Electroweak Symmetry breaking
(EWSB) -- that one condensing Higgs boson doublet carries all burdens of elementary
particle mass generation -- remains speculative. Experimental result... | {'timestamp': '2006-12-18T21:50:41', 'yymm': '0612', 'arxiv_id': 'hep-ph/0612219', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-ph/0612219'} |
\section{Introduction}
Since the experimental discovery of the fractional quantum Hall effect, a tremendous effort has been devoted to the study of topologically ordered phases that can be realized in strongly correlated quantum many-body systems. In the past decade, substantial progress has been made in the character... | {'timestamp': '2020-08-06T02:05:32', 'yymm': '1911', 'arxiv_id': '1911.11867', 'language': 'en', 'url': 'https://arxiv.org/abs/1911.11867'} |
\section{Introduction}
Let $\mathbb{F}_q$ be the finite field with $q=p^s$ elements, where $p$ is an odd prime.
An important class of curves over finite fields is the class of Artin-Schreier curves. That are given by the equation $y^q-y=f(x)$ for some $f(x)\in \mathbb{F}_q[x]$. These curves have been extensively stu... | {'timestamp': '2022-11-22T02:27:40', 'yymm': '2211', 'arxiv_id': '2211.11371', 'language': 'en', 'url': 'https://arxiv.org/abs/2211.11371'} |
\section{Introduction \label{sec:intro}}
Many of iron-based superconductors, which include pnictides and chalcogenides, have high critical temperatures $T_c>50$~K allowing to refer to them as high-$T_c$ superconductors. The basic element is always a square lattice of Fe, though in some cases with orthorhombic distorti... | {'timestamp': '2018-09-28T02:02:19', 'yymm': '1803', 'arxiv_id': '1803.06736', 'language': 'en', 'url': 'https://arxiv.org/abs/1803.06736'} |
\section{Introduction}
Boolean satisfiability is a well known NP-complete problem that serves as the basis for many computationally hard tasks. Some of these applications, such as formal software verification and data mining, are well served by solvers which are capable of finding more than one satisfying assignment of... | {'timestamp': '2016-12-22T02:07:52', 'yymm': '1612', 'arxiv_id': '1612.07258', 'language': 'en', 'url': 'https://arxiv.org/abs/1612.07258'} |
\section{Coherent state in a QD pump under a strong magnetic field}
We show that in a 2D QD formed by time-dependent confinement potential, the evolution of a Gaussian state with spatial width $\simeq l_B$
follows the classical equation of motion of a coherent state
under the strong-magnetic-field conditions that the ... | {'timestamp': '2016-10-25T02:08:15', 'yymm': '1610', 'arxiv_id': '1610.07293', 'language': 'en', 'url': 'https://arxiv.org/abs/1610.07293'} |
\section{Introduction}
The outburst of V445 Pup was discovered on 30 December 2000 by Kanatsu
\citep{kan00}. The outburst shows unique properties such as
absence of hydrogen, unusually strong carbon emission lines as well as
strong emission lines of Na, Fe, Ti, Cr, Si, Mg etc. \citep{ash03,iij08}.
The spectral fea... | {'timestamp': '2008-05-16T16:09:36', 'yymm': '0805', 'arxiv_id': '0805.2540', 'language': 'en', 'url': 'https://arxiv.org/abs/0805.2540'} |
\section{Introduction}
Inspired by Shannon’s classic information theory \cite{shannon1948mathematical}, Weaver and Shannon proposed a more general definition of a communication system involving three different levels of problems, namely, (i) transmission of bits (the technical problem); (ii) semantic exchange of trans... | {'timestamp': '2022-10-19T02:01:36', 'yymm': '2210', 'arxiv_id': '2210.09372', 'language': 'en', 'url': 'https://arxiv.org/abs/2210.09372'} |
\section{Introduction}\label{sec:intro}
\subsection{Motivation}
Let $G$ be a finite graph on the vertex set $\{1,2,\ldots,n\}$.
There are many profitable ways to associate a polytope to $G$.
One well-known example is the \emph{edge polytope} of $G$, obtained by taking the convex hull of the vectors $e_i+e_j$ for each ... | {'timestamp': '2017-06-23T02:00:53', 'yymm': '1706', 'arxiv_id': '1706.07085', 'language': 'en', 'url': 'https://arxiv.org/abs/1706.07085'} |
\section{surface passivation}
In the wurtzite structure, each atom has 4 nearest neighbor (nn) dissimilar atoms and hence 4 bonds, each hosting 2 electrons. Using boron nitride (BN) as an example, by the ECM, each B atom (with three valence electrons) contributes 3/4 = 0.75 electrons to the bond, whereas each N atom (... | {'timestamp': '2021-09-01T02:25:42', 'yymm': '2108', 'arxiv_id': '2108.13950', 'language': 'en', 'url': 'https://arxiv.org/abs/2108.13950'} |
\section{Introduction}\label{Intro}
The central limit theorem (CLT) for partial sums $S_n=\sum_{j=1}^{n}X_j$ of stationary real-valued random variables $\{X_j\}$, exhibiting some type of ``weak dependence", is one of the main topics in probability theory, stating that $(S_n-{\mathbb E}[S_n])/\sqrt{Var(S_n)}$ converges ... | {'timestamp': '2021-11-25T02:07:49', 'yymm': '2005', 'arxiv_id': '2005.02915', 'language': 'en', 'url': 'https://arxiv.org/abs/2005.02915'} |
\section{Avant propos}
Le but de cet article est de pr\'esent\'e un exemple d'int\'eraction entre la th\'eorie des nombres
et la physique {\it exp\'erimentale}. J'insiste sur l'aspect exp\'erimental, car il n'est pas rare de trouver des
applications de la th\'eorie des nombres en physique th\'eorique, ou plus g\'en\'e... | {'timestamp': '2005-09-26T02:07:28', 'yymm': '0509', 'arxiv_id': 'math-ph/0509053', 'language': 'fr', 'url': 'https://arxiv.org/abs/math-ph/0509053'} |
\section{Introduction}
After receiving paper reviews, authors may optionally submit a rebuttal to address the reviewers' comments, which will be limited to a {\bf one page} PDF file.
Please follow the steps and style guidelines outlined below for submitting your author response.
The author rebuttal is optional and, f... | {'timestamp': '2021-12-16T02:13:30', 'yymm': '2112', 'arxiv_id': '2112.06226', 'language': 'en', 'url': 'https://arxiv.org/abs/2112.06226'} |
\section{Introduction}
\subsection{Canonical partition functions for log-Coulomb gases}\label{1_1}
Let $X$ be a topological space endowed with a metric $d$ and a finite positive Borel measure $\mu$ satisfying $\mu^N\{(x_1,\dots,x_N)\in X^N:x_i=x_j\text{ for some $i\neq j$}\}=0$ for every $N\geq 1$. A \emph{log-Coulomb ... | {'timestamp': '2021-10-18T02:11:14', 'yymm': '2110', 'arxiv_id': '2110.07854', 'language': 'en', 'url': 'https://arxiv.org/abs/2110.07854'} |
\section{Introduction}
The AdS/CFT correspondence \cite{MGW} has been explored beyond the
supergravity approximation \cite{BMN,GKP}. In the BMN limit \cite{BMN}
for the $\mathcal{N} = 4$ super Yang-Mills (SYM) theory the perturbative
scaling dimensions of gauge invariant near-BPS operators with large
R-charge can be ... | {'timestamp': '2005-09-28T02:05:20', 'yymm': '0509', 'arxiv_id': 'hep-th/0509195', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-th/0509195'} |
\section{Introduction}
\qquad The uncapacitated facility location (UFL) problem has received lots of attention due to its connection to operational research and infrastructure planning. In the UFL problem, we are given a set of potential facility locations $F$, each $i\in F$ with a facility cost $f_i$, a set of clien... | {'timestamp': '2016-10-25T02:10:55', 'yymm': '1610', 'arxiv_id': '1610.07434', 'language': 'en', 'url': 'https://arxiv.org/abs/1610.07434'} |
\section{Introduction}
Coronal mass ejections (CMEs) are energetic expulsions
of plasma from the solar corona that are driven by the
release of magnetic energy typically in the range of $10^{32-33}$ ergs.
The majority of CMEs originate from the eruption of pre-existing
large-scale helmet streamers \citep[]{WM_hundhause... | {'timestamp': '2008-12-18T17:58:32', 'yymm': '0812', 'arxiv_id': '0812.3589', 'language': 'en', 'url': 'https://arxiv.org/abs/0812.3589'} |
\section{Introduction}
The use of hybrid density functionals \cite{Becke1993}, which include
a portion of Hartree-Fock exchange (HF-exchange), has proven to be
an invaluable approach to density functional theory (DFT). Within
the solid-state community, the one proposed by Heyd, Scuseria and
Ernzerhof \cite{Heyd2003,Kr... | {'timestamp': '2019-02-04T02:10:50', 'yymm': '1902', 'arxiv_id': '1902.00281', 'language': 'en', 'url': 'https://arxiv.org/abs/1902.00281'} |
\section{Introduction}
The requirement of reproducible computational research is becoming increasingly important and mandatory across the sciences~\cite{national2019reproducibility}. Because reproducibility implies a certain level of openness and sharing of data and code, parts of the scientific community have devel... | {'timestamp': '2020-06-18T02:04:36', 'yymm': '2005', 'arxiv_id': '2005.02985', 'language': 'en', 'url': 'https://arxiv.org/abs/2005.02985'} |
\section{Linear $k_\perp$ factorization is broken}
Heavy nuclei are strongly absorbing targets and bring a new scale into
the perturbative QCD (pQCD) description of hard processes \cite{Mueller}.
This has severe consequences for the relations between various
hard scattering observables. In a regime of small absorptio... | {'timestamp': '2008-12-19T16:49:09', 'yymm': '0812', 'arxiv_id': '0812.3802', 'language': 'en', 'url': 'https://arxiv.org/abs/0812.3802'} |
\section{Introduction}
The emergence of IPv6 in the Internet offers interesting possibilities for studies to compare IPv6 and IPv4 structures and attributes in the Internet.
Interesting questions are, \textit{e.g.,}\xspace whether and to what extent IPv6 addresses are co-deployed on existing IPv4 hardware,... | {'timestamp': '2017-05-03T02:06:00', 'yymm': '1610', 'arxiv_id': '1610.07251', 'language': 'en', 'url': 'https://arxiv.org/abs/1610.07251'} |
\section{Introduction}
A system of second order ordinary differential equations (SODE), whose
coefficients functions are positively two-homogeneous, can be
identified with a second order vector field, which is called a
spray. If such a system represents the variational (Euler-Lagrange)
equations of the energy of... | {'timestamp': '2015-11-18T02:07:42', 'yymm': '1412', 'arxiv_id': '1412.5282', 'language': 'en', 'url': 'https://arxiv.org/abs/1412.5282'} |
\section{Introduction}\label{sec:intro}
Social media posts with false claims have led to real-world threats on many aspects such as politics~\citep{pizzagate}, social order~\citep{salt}, and personal health~\citep{shuanghuanglian}.
To tackle this issue, over 300 fact-checking projects have been launched, such as Snopes... | {'timestamp': '2021-12-21T02:24:56', 'yymm': '2112', 'arxiv_id': '2112.10322', 'language': 'en', 'url': 'https://arxiv.org/abs/2112.10322'} |
\section{Introduction}
Deep neural networks have achieved superior performance on numerous vision tasks \cite{Zisserman1,Zisserman2,semanticsegmentation}. However, they contain complicated black boxes with huge, unexplainable parameters that begin with random initialization and reach another unpredictable (still) sub-... | {'timestamp': '2022-07-13T02:11:00', 'yymm': '2207', 'arxiv_id': '2207.05374', 'language': 'en', 'url': 'https://arxiv.org/abs/2207.05374'} |
\section{Introduction}
In adsorbed nematics, surfaces often determine the favoured director orientation, which then propagates into the bulk
\cite{Jerome}. When a nematic is subject to orientations propagating from different surfaces, elasticity theory predicts
a distorted director configuration, with an associated e... | {'timestamp': '2014-02-04T02:15:53', 'yymm': '1402', 'arxiv_id': '1402.0363', 'language': 'en', 'url': 'https://arxiv.org/abs/1402.0363'} |
\section{Introduction}
Wave turbulence is observed in the interaction of nonlinear dispersive waves in many physical processes, see the review \cite{newell} and references therein. Zakharov and Filonenko \cite{Zakh} proposed a theory of weak turbulence of capillary waves on the surface of a liquid. According to which, ... | {'timestamp': '2020-02-21T02:11:48', 'yymm': '2002', 'arxiv_id': '2002.08698', 'language': 'en', 'url': 'https://arxiv.org/abs/2002.08698'} |
\section{Introduction}
In recent years, tremendous advances in the study of algebraic $\K$-theory have been facilitated by the trace method approach,
in which algebraic $\K$-theory is approximated by invariants from homological algebra and their topological analogues. For a ring $R$, the Dennis trace map relates its al... | {'timestamp': '2021-11-16T02:03:42', 'yymm': '2111', 'arxiv_id': '2111.06970', 'language': 'en', 'url': 'https://arxiv.org/abs/2111.06970'} |
\section{Introduction}
A billiard ball, i.e.\ a point mass, moves inside a polyhedron $P$
with unit speed along a straight line until it reaches the
boundary $\partial{P}$, then it instantaneously changes direction
according to the mirror law, and continues along the new line.
Label the faces of $P$ by symbols from a ... | {'timestamp': '2012-05-01T02:05:24', 'yymm': '1204', 'arxiv_id': '1204.6556', 'language': 'en', 'url': 'https://arxiv.org/abs/1204.6556'} |
\section{Introduction}
\subsection{Summary of our model's theoretical foundations}
We have set forth in the first part of this work \cite{Guevel2019a} the theoretical foundations of CPFM. This is an extended PFM based on a non-equilibrium thermodynamic framework, contact thermodynamics, incorporating for now chemo-m... | {'timestamp': '2019-07-02T02:30:24', 'yymm': '1907', 'arxiv_id': '1907.00698', 'language': 'en', 'url': 'https://arxiv.org/abs/1907.00698'} |
\section{#1}\label{sec:#2}}
\newcommand{\mysubsection}[2]{\subsection{#1}\label{sec:#2}}
\newcommand{\mysubsubsection}[2]{\subsubsection{#1}\label{sec:#2}}
| {'timestamp': '2019-04-17T02:27:27', 'yymm': '1904', 'arxiv_id': '1904.07615', 'language': 'en', 'url': 'https://arxiv.org/abs/1904.07615'} |
\section{Introduction}\label{sec:intro}
Neutron stars are promising compact objects
to obtain the information on
the equation of state of dense matter
and investigate physics of strong gravity.
The direct detections of gravitational waves
from merging compact objects
opened up a new window to access
such informati... | {'timestamp': '2022-04-22T02:20:58', 'yymm': '2204', 'arxiv_id': '2204.09943', 'language': 'en', 'url': 'https://arxiv.org/abs/2204.09943'} |
\section{Introduction
\noindent
Future experimental programs at
the High-Luminosity Large Hadron
Collider (HL-LHC)~\cite{ATLAS:2013hta,
CMS:2013xfa} and the International
Linear Collider (ILC)~\cite{Baer:2013cma}
aim to measure precisely the properties
of Higgs boson, top quark and vector
bosons for discovering t... | {'timestamp': '2019-04-22T02:13:56', 'yymm': '1904', 'arxiv_id': '1904.07430', 'language': 'en', 'url': 'https://arxiv.org/abs/1904.07430'} |
\section{\@startsection{section}{1}{\z@}{3.5ex plus 1ex minus
.2ex}{2.3ex plus .2ex}{\bf}}
\def\subsection{\@startsection{subsection}{2}{\z@}{3.25ex plus 1ex minus
.2ex}{1.5ex plus .2ex}{\bf}}
\def\bf Appendix B: {\Roman{section}.}
\def\Alph{subsection}.{\Alph{subsection}.}
\def\arabic{subsubsection}.{\arabic{sub... | {'timestamp': '1992-05-24T14:29:59', 'yymm': '9205', 'arxiv_id': 'hep-ph/9205231', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-ph/9205231'} |
\section{Introduction}
Supermassive black holes (SMBHs) in active galactic nuclei (AGNs) are known to have luminous accretion discs
(Shakura \& Sunyeav 1973; Kato et al. 2008 and reference therein).
Various evidences of mass outflows from a luminous disc are frequently observed, but their origins and dynamics are not... | {'timestamp': '2021-05-18T02:10:25', 'yymm': '2105', 'arxiv_id': '2105.07223', 'language': 'en', 'url': 'https://arxiv.org/abs/2105.07223'} |
\section{Introduction}
\label{sec:Introduction}
Dealing with renewable energy sources requires internalizing their stochasticity into optimization and market-clearing tools used in power system operations.
To this end, stochastic \cite{shiina2004stochastic} and robust \cite{jabr2013adjustable} optimization metho... | {'timestamp': '2021-10-06T02:27:52', 'yymm': '2110', 'arxiv_id': '2110.02152', 'language': 'en', 'url': 'https://arxiv.org/abs/2110.02152'} |
\section{Introduction}
Following the isolation of single layer graphene,~\cite{NovoselovNat2007} studies on the electrical,~\cite{RevModPhys.81.109,Novoselov10222004,ISI:000248194700033,ISI:000233133500043,cresti} optical,~\cite{ISI:000274338800035,ISI:000256441100035} thermal,~\cite{Seol04092010, doi:10.1021/nl073187... | {'timestamp': '2012-08-20T02:02:04', 'yymm': '1208', 'arxiv_id': '1208.3607', 'language': 'en', 'url': 'https://arxiv.org/abs/1208.3607'} |
\section{INTRODUCTION}
Optical and X-ray studies (e.g. Geller \& Beers\markcite{14} 1982;
Forman {et~al.}~\markcite{12} 1981; Dressler \& Shectman 1988; Jones \&
Forman\markcite{19} 1992; Mohr et al. 1994; Bird 1994; Slezak et
al. 1994) have shown that galaxy clusters are dynamically evolving
systems exhibiting a var... | {'timestamp': '1997-12-22T20:08:05', 'yymm': '9712', 'arxiv_id': 'astro-ph/9712299', 'language': 'en', 'url': 'https://arxiv.org/abs/astro-ph/9712299'} |
\section{Summary}
\input{sections/7.summary}
\section*{Acknowledgements}
This research received funding from the Flemish Government under the ``Onderzoeksprogramma Artificiële Intelligentie (AI) Vlaanderen'' programme.
The authors thank Maurice Bruynooghe for his review of the drafts of this paper.
\... | {'timestamp': '2022-02-15T02:08:31', 'yymm': '2202', 'arxiv_id': '2202.00898', 'language': 'en', 'url': 'https://arxiv.org/abs/2202.00898'} |
\section{Introduction}
The Bekenstein-Hawking entropies of the BPS saturated
black holes have been studied in four-, five-
and ten-dimensions from the nonperturbative aspects of string theory
\cite{CY,CT,SV,HS,MS,Tsey,GKT,BB}.
The black holes in ten-dimensions are constructed
by the intersecting D-branes.
The blac... | {'timestamp': '1998-07-06T07:04:09', 'yymm': '9712', 'arxiv_id': 'hep-th/9712224', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-th/9712224'} |
\section{Introduction}
In a cold dark matter (CDM) universe, dark matter haloes form hierarchically through accretion and merging(for a recent review, see \citet{Frenk2012}).
Many rigorous and reliable predictions for the halo mass function and subhalo mass functions in CDM are provided by numerical simulations\citep... | {'timestamp': '2016-03-16T01:08:32', 'yymm': '1507', 'arxiv_id': '1507.01464', 'language': 'en', 'url': 'https://arxiv.org/abs/1507.01464'} |
\section{Introduction}
Very High Energy (VHE) $\gamma$-ray astronomy \cite{ong} is still
in its infancy. Operating in the energy
range from $\sim$\,100 GeV to 30 TeV and beyond, this subfield of
astronomy represents an exciting,
relatively unsampled region of the electromagnetic spectrum, and a
tremendous challen... | {'timestamp': '1998-12-08T19:48:44', 'yymm': '9812', 'arxiv_id': 'astro-ph/9812153', 'language': 'en', 'url': 'https://arxiv.org/abs/astro-ph/9812153'} |
\section{Introduction}
The eleven-dimensional interpretation of the massive Type IIA
supergravity of Romans \cite{Romans} has devoted a lot of
attention recently.
It was shown in \cite{BDHS} that it is not possible
to construct a covariant
supergravity theory in eleven dimensions with cosmological
constant.
One mi... | {'timestamp': '1999-02-12T15:58:43', 'yymm': '9812', 'arxiv_id': 'hep-th/9812188', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-th/9812188'} |
\section{Introduction}
Stories are central to human culture and communication. However, it seems that stories are easier said than generated. Despite incredible recent progress in natural language processing generation of longer texts is still a challenge \cite{van2019narrative, rashkin2020plotmachines}. \citet{osterm... | {'timestamp': '2021-09-30T02:19:50', 'yymm': '2109', 'arxiv_id': '2109.14396', 'language': 'en', 'url': 'https://arxiv.org/abs/2109.14396'} |
\section{Introduction}
\label{sec:intro}
As a classic
vision task, single-image-super-resolution (SISR) restores the original high-resolution (HR) image based on a down-sampled low-resolution (LR) one. It can be applied in various applications, such as low-resolution media data enhancement or video/image upscaling ... | {'timestamp': '2022-07-27T02:05:57', 'yymm': '2207', 'arxiv_id': '2207.12577', 'language': 'en', 'url': 'https://arxiv.org/abs/2207.12577'} |
\section{Introduction}
We consider a model that generalizes many previously studied optimization problems in the framework of scheduling and (minimization) load balancing problems on parallel machines. We use this generalization in order to exhibit that there is a standard way to design efficient polynomial time appr... | {'timestamp': '2018-02-28T02:08:34', 'yymm': '1802', 'arxiv_id': '1802.09828', 'language': 'en', 'url': 'https://arxiv.org/abs/1802.09828'} |
\section{Introduction}\label{sec:intro}
M-dwarfs ($M_{\star}\lesssim0.6{\rm M}_{\odot}$) constitute more than seventy
per cent of the Galactic stellar population \citep{Hen97} and
consequently, they influence a wide-range of astrophysical phenomena,
from the total baryonic content of the universe, to the shape of the
s... | {'timestamp': '2012-06-14T02:02:30', 'yymm': '1206', 'arxiv_id': '1206.2773', 'language': 'en', 'url': 'https://arxiv.org/abs/1206.2773'} |
\section{Introduction}
The behavior of the Riemann zeta function on the critical line has been intensively studied, in particular in relation with the Riemann hypothesis. A natural question concerns the order of magnitude of the moments of $\zeta$:
$$\mu_k(T) := \frac{1}{T} \int_0^T |\zeta (1/2 + it)|^{2k} dt = \mathb... | {'timestamp': '2019-09-17T02:11:51', 'yymm': '1804', 'arxiv_id': '1804.00343', 'language': 'en', 'url': 'https://arxiv.org/abs/1804.00343'} |
\section{Introduction}
When two black holes spiral together and coalesce, they emit
gravitational radiation which in general possesses net linear
momentum. This accelerates (i.e., ``kicks'') the coalescence remnant
relative to the initial binary center of mass. Analytical calculations
have determined the accumulated k... | {'timestamp': '2007-04-13T00:54:12', 'yymm': '0703', 'arxiv_id': 'astro-ph/0703054', 'language': 'en', 'url': 'https://arxiv.org/abs/astro-ph/0703054'} |
\section*{Introduction}
Let $C$ be a nonempty convex set in a (real) normed linear space $X$. A
function $f\colon C\to\mathbb{R}$ is called {\em d.c.}\ (or ``delta-convex'')
if it can be represented as a difference of two continuous convex
functions on $C$. An extension of this notion, the notion of a {\em d.c.\ mappi... | {'timestamp': '2008-10-08T15:40:06', 'yymm': '0810', 'arxiv_id': '0810.1433', 'language': 'en', 'url': 'https://arxiv.org/abs/0810.1433'} |
\section{Introduction}
$\delta$ Scuti stars are a class of pulsating stars located
on the Hertzsprung-Russell Diagram on or
around the Main Sequence and intersecting the instability strip.
They are 1.5 - 2.5 $M_{\odot}$ stars pulsating often in one main
dominant oscillation mode or many lower a... | {'timestamp': '2008-10-15T18:15:06', 'yymm': '0810', 'arxiv_id': '0810.2191', 'language': 'en', 'url': 'https://arxiv.org/abs/0810.2191'} |
\section{Introduction}
Uncertainty relations place fundamental limits on the precision achievable in measuring non-commuting observables. The original idea of uncertainty relation was first introduced by Heisenberg~\cite{heis} for position and momentum observables $Q$, $P$. Subsequently, a mathematically precis... | {'timestamp': '2021-03-30T02:56:23', 'yymm': '2103', 'arxiv_id': '2103.15731', 'language': 'en', 'url': 'https://arxiv.org/abs/2103.15731'} |
\section{#1}\setcounter{equation}{0}}
\newcommand{\leavevmode\hbox{\rm{\small1\kern-3.8pt\normalsize1}}}{\leavevmode\hbox{\rm{\small1\kern-3.8pt\normalsize1}}}
\def{\hbox{$\sqcup$}\llap{\hbox{$\sqcap$}}}{{\hbox{$\sqcup$}\llap{\hbox{$\sqcap$}}}}
\begin{document}
\addtolength{\baselineskip}{1.5mm}
\renewcommand{\thefo... | {'timestamp': '1999-02-16T17:56:10', 'yymm': '9812', 'arxiv_id': 'gr-qc/9812032', 'language': 'en', 'url': 'https://arxiv.org/abs/gr-qc/9812032'} |
\section{INTRODUCTION}
Our sun has an eleven-year magnetic activity cycle, which is thought to be
sustained by the dynamo motion of internal ionized plasma,
i.e., a transformation of kinetic energy to magnetic energy
\citep{1955ApJ...122..293P}. Our understanding of the solar dynamo has
significantly improved during th... | {'timestamp': '2011-07-15T02:00:29', 'yymm': '1107', 'arxiv_id': '1107.2685', 'language': 'en', 'url': 'https://arxiv.org/abs/1107.2685'} |
\section{Introduction}
\subsection{Igusa's zeta function and the Monodromy Conjecture}
For a prime $p$, we denote by \Qp\ the field of $p$-adic numbers and by \Zp\ its subring of $p$-adic integers. We denote by $|\cdot|$ the $p$-adic norm on \Qp. Let $n\in\Zplusnul$ and denote by $|dx|=|dx_1\wedge\cdots\wedge dx_n|$ ... | {'timestamp': '2013-06-26T02:02:59', 'yymm': '1306', 'arxiv_id': '1306.6012', 'language': 'en', 'url': 'https://arxiv.org/abs/1306.6012'} |
\section{I. Introduction}
Most materials expand upon heating, while those that shrink are much less common. Recent interest in these materials with negative thermal expansion (NTE) is also driven by technological applications that require materials with zero thermal expansion across a desired temperature range \cite{n... | {'timestamp': '2018-07-10T02:04:55', 'yymm': '1804', 'arxiv_id': '1804.06790', 'language': 'en', 'url': 'https://arxiv.org/abs/1804.06790'} |
\section{}
\label{app:pf}
\subsection{Proof of Theorem~\ref{thm:chernoff}}
\label{app:pfThmChernoff}
\begin{proof}
We present the proof of~\eqref{eqn:chernoffUpper}. The proof of~\eqref{eqn:chernoffLower} is similar and is omitted. For any $n\geq 2$, denote by $\mathcal{F}_n$ the $\sigma$-algebra generated by $Z_1, \... | {'timestamp': '2021-03-29T02:01:46', 'yymm': '1907', 'arxiv_id': '1907.00304', 'language': 'en', 'url': 'https://arxiv.org/abs/1907.00304'} |
\section{Introduction}
At its core, general relativity is a theory of gravity phrased operationally in terms of measurements of distances and time using classical rulers and clocks. Quantizing these notions has been a major problem of theoretical physics for the past century and, as of today, there is still no comple... | {'timestamp': '2022-02-24T02:00:18', 'yymm': '2202', 'arxiv_id': '2202.11108', 'language': 'en', 'url': 'https://arxiv.org/abs/2202.11108'} |
\section{\label{sec:level1}First-level heading:\protect\\ The line
break was forced \lowercase{via} \textbackslash\textbackslash}
This sample document demonstrates proper use of REV\TeX~4.2 (and
\LaTeXe) in manuscripts prepared for submission to AIP
journals. Further information can be found in the documentation inclu... | {'timestamp': '2022-02-17T02:22:31', 'yymm': '2202', 'arxiv_id': '2202.08071', 'language': 'en', 'url': 'https://arxiv.org/abs/2202.08071'} |
\section{Introduction}
The concept of a "point rotation reference frame", i.e., the frame with the
axis of rotation at every point, arises in optics. However, this concept is
also applicable to other areas of physics. An example of such a frame is the
optical indicatrix (index ellipsoid) \cite{Born}.\ Any rotatin... | {'timestamp': '2013-11-12T02:08:07', 'yymm': '1307', 'arxiv_id': '1307.7354', 'language': 'en', 'url': 'https://arxiv.org/abs/1307.7354'} |
\section{Introduction}
Many problems in financial mathematics, economics, and engineering may be cast in the form of a stochastic optimisation problem, and typically the agent's optimal control depends on the underlying (dynamic) model assumptions. Models, however, are approximations of the world, whether they are pur... | {'timestamp': '2021-08-25T02:04:35', 'yymm': '2108', 'arxiv_id': '2108.10403', 'language': 'en', 'url': 'https://arxiv.org/abs/2108.10403'} |
\section{Introduction}
\label{intro}
Optimization problems with constraints which require the solution of a
partial differential equation (PDE) arise widely in many areas of the sciences and
engineering, in particular in problems of design. The development, analysis and implementation of efficient and robust numeri... | {'timestamp': '2020-01-08T02:14:19', 'yymm': '2001', 'arxiv_id': '2001.02118', 'language': 'en', 'url': 'https://arxiv.org/abs/2001.02118'} |
\section{Algorithms}
\subsection{Algorithm A}
\subsubsection{Complexity}
The pseudo code of the algorithm would be to long to be displayed in a single page, thus, we divided it into two parts. The first part, corresponding to the preparation of the weighted network between the tags and the building of local hierarchie... | {'timestamp': '2014-01-23T02:11:04', 'yymm': '1401', 'arxiv_id': '1401.5741', 'language': 'en', 'url': 'https://arxiv.org/abs/1401.5741'} |
\section{\label{sec:introduction}Introduction}
Optomechanical systems are widely used in experiments of precise measurements~\cite{Aspelmeyer:2013lha}.
In particular, optomechanical systems consisting of massive oscillators are suitable for testing macroscopic quantum mechanics~\cite{Chen:2013sgs}, investing Newtonian ... | {'timestamp': '2022-07-28T02:14:35', 'yymm': '2110', 'arxiv_id': '2110.13507', 'language': 'en', 'url': 'https://arxiv.org/abs/2110.13507'} |
\section{Introduction}
\noindent This paper is devoted to the study of perturbations of the Crapper waves through gravity and concentrated vorticity. The problem that we analyze is the free-boundary stationary Euler equation with vorticity
\begin{subequations}\label{v-euler}
\begin{align}[left=\empheqlbrace\,]
&v\cdot... | {'timestamp': '2021-07-01T02:14:32', 'yymm': '2106', 'arxiv_id': '2106.15923', 'language': 'en', 'url': 'https://arxiv.org/abs/2106.15923'} |
\section{The bi-criteria objective}
\label{sec-bicriteria}
In this section we state our results with respect to the bi-criteria objective, for both deterministic and randomized benchmarks. Recall that our bi-criteria objective focuses on the worst-case error rates.
We only consider the case of uniform costs. Let $k\g... | {'timestamp': '2013-05-21T02:03:39', 'yymm': '1302', 'arxiv_id': '1302.3268', 'language': 'en', 'url': 'https://arxiv.org/abs/1302.3268'} |
\section{Introduction}
Leptophilic gauge bosons are popular candidates for physics beyond the Standard Model (SM).
As opposed to new gauge bosons interacting with quarks, which are strongly constrained by LHC searches~\cite{ATLAS:2017eqx,CMS:2018mgb,ATLAS:2019erb,CMS:2021ctt}, those coupling solely to leptons are only... | {'timestamp': '2021-11-10T02:00:26', 'yymm': '2111', 'arxiv_id': '2111.04744', 'language': 'en', 'url': 'https://arxiv.org/abs/2111.04744'} |
\section{Introduction}
Generative Adversarial Models (GANs)\cite{Goodfellow:2014:GAN:2969033.2969125} have been found to produce images of very high quality on some datasets \cite{DBLP:conf/iclr/KarrasALL18, DBLP:journals/corr/abs-1812-04948}. However, their results on other datasets, while impressive, still lag behin... | {'timestamp': '2019-07-08T02:03:56', 'yymm': '1907', 'arxiv_id': '1907.02662', 'language': 'en', 'url': 'https://arxiv.org/abs/1907.02662'} |
\section{Introduction}
\label{sec:intro}
Cosmological inflation \cite{Starobinsky:1980te, Sato:1980yn, Guth:1980zm, Linde:1981mu, Albrecht:1982wi, Linde:1983gd} is a phase of accelerated expansion that took place at high energy in the primordial universe. It explains its homogeneity and isotropy at large scales. Furthe... | {'timestamp': '2021-05-03T02:23:31', 'yymm': '2101', 'arxiv_id': '2101.05741', 'language': 'en', 'url': 'https://arxiv.org/abs/2101.05741'} |
\section{Introduction}
Emerging advanced accelerator concepts require precise control over the longitudinal phase space (LPS) of charged particle beams. Efficient beam-driven acceleration, for example, relies on longitudinally-tailored electron bunch profiles which can be produced with an appropriate energy modulation ... | {'timestamp': '2020-09-28T02:10:34', 'yymm': '2009', 'arxiv_id': '2009.12123', 'language': 'en', 'url': 'https://arxiv.org/abs/2009.12123'} |
\section{Introduction}
Recently, the interplay of chaos and quantum
interference in $ballistic$ quantum dots has intrigued experimentalists and theorists
alike.
The quantum interference effects, $e.g$., ballistic weak localization (BWL) ~\cite{rf:Baranger} and
ballistic
conductance fluctuation ~\cite{rf:Jalabert} in... | {'timestamp': '2000-02-05T06:22:24', 'yymm': '9707', 'arxiv_id': 'cond-mat/9707087', 'language': 'en', 'url': 'https://arxiv.org/abs/cond-mat/9707087'} |
\section{Introduction}
The dynamics of non-abelian gauge fields at finite temperature has
attracted some attention recently~\cite{grigoriev}--\cite{son}.
A lot of work on this subject has been
done in perturbation theory. However, some physical quantities
of interest are non-perturbative and the only known method o... | {'timestamp': '1997-10-15T06:43:25', 'yymm': '9707', 'arxiv_id': 'hep-ph/9707489', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-ph/9707489'} |
\section{Summary}
\label{sec:conclusion}
In this work, we explored the transferability of HINTS on different computational domains for differential equations. Specifically, we considered two methods: (1) directly employ the HINTS for an equation defined in an unseen domain; (2) adopt the transfer operator learning to ... | {'timestamp': '2022-11-01T01:28:54', 'yymm': '2210', 'arxiv_id': '2210.17392', 'language': 'en', 'url': 'https://arxiv.org/abs/2210.17392'} |
\section{Task and Dataset}
\label{sec:task_and_data}
Below, we describe the CONSTRAINT 2022 shared task and the corresponding dataset provided by the task organizers. More detail can be found in the shared task report \cite{sharma2022report}.
\subsection{Task}
\label{ssec:Task}
The CONSTRAINT 2022 shared task asked ... | {'timestamp': '2022-05-10T02:42:23', 'yymm': '2205', 'arxiv_id': '2205.04402', 'language': 'en', 'url': 'https://arxiv.org/abs/2205.04402'} |
\section{Introduction}
Van der Waals complexes containing open-shell species are of great
current interest. In particular, complexes containing atoms or
molecules with orbital angular momentum necessarily involve
multiple electronic states.\cite{DUBERNET:1991,
DUBERNET:open:1994} They provide a test-bed for studying
e... | {'timestamp': '2006-10-11T11:57:18', 'yymm': '0610', 'arxiv_id': 'physics/0610079', 'language': 'en', 'url': 'https://arxiv.org/abs/physics/0610079'} |
\section{Introduction}
Monopoles in Yang-Mills-Higgs theories are known to posses a spectrum of excitations called dyons. In the
simplest of these theories the gauge group is ${\cal G}=SU(2)$ spontaneously broken to ${\cal H}=U(1)$ by a non-zero vacuum
expectation value of the Higgs field. Gauss' Law implies that the ... | {'timestamp': '1997-07-11T18:05:32', 'yymm': '9707', 'arxiv_id': 'hep-th/9707117', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-th/9707117'} |
\section{Introduction}\label{se:intro}
Let $n\ge 3$ and $M$ be a smooth $n$-dimensional manifold. For a Riemannian metric $g$ and a scalar-valued function $u$ on $M$, $n\ge 3$, we define the \emph{static vacuum operator}
\begin{align} \label{eq:static}
S(g, u) := \big(-u \mathrm{Ric}_g + \nabla^2_g u, \Delta_g u\bi... | {'timestamp': '2022-06-02T02:02:39', 'yymm': '2206', 'arxiv_id': '2206.00079', 'language': 'en', 'url': 'https://arxiv.org/abs/2206.00079'} |
\section{Introduction}
\label{Introduction}
In relativistic quantum field theory,
the nature of the field modes associated
with the spontaneous breaking of an internal symmetry
is now standard lore.
When a global internal symmetry is spontaneously broken,
one or more massless modes called Nambu-Goldstone (NG) modes ap... | {'timestamp': '2008-02-14T17:00:48', 'yymm': '0712', 'arxiv_id': '0712.4119', 'language': 'en', 'url': 'https://arxiv.org/abs/0712.4119'} |
\section{introduction}
Experimental data on the quark and lepton masses and mixing provide
important clues to the nature of new physics beyond the Standard
Model(SM). However, in SM the Yukawa coupling constants which are
responsible for the fermion masses and mixing, can be freely
adjusted without disturbing the inter... | {'timestamp': '2008-08-11T15:45:12', 'yymm': '0803', 'arxiv_id': '0803.2278', 'language': 'en', 'url': 'https://arxiv.org/abs/0803.2278'} |
\section{Introduction}
Total variation (TV) denoising is a nonlinear filtering method based on
the assumption that the underlying signal is piecewise constant
(equivalently, the derivative of the underlying signal is \emph{sparse}) \cite{ROF_1992}.
Such signals arise in geoscience, biophysics, and other areas \cite{Li... | {'timestamp': '2017-01-03T02:08:02', 'yymm': '1701', 'arxiv_id': '1701.00439', 'language': 'en', 'url': 'https://arxiv.org/abs/1701.00439'} |
\section{Introduction}
\label{sec:intro}
The gravitational scattering of classical objects at large impact parameter $b$ is relevant for the study of the inspiral phase of black-hole binaries since it can be used to determine the parameters of the Effective-One-Body description (see~\cite{Damour:2016gwp} and reference... | {'timestamp': '2021-04-15T02:01:08', 'yymm': '2101', 'arxiv_id': '2101.05772', 'language': 'en', 'url': 'https://arxiv.org/abs/2101.05772'} |
\section{Introduction}
The mediation of supersymmetry breaking to the observable sector via
supersymmetric gauge interactions (GMSB) has already been proposed
during the very early days of super\-symmetric model building
\cite{early1,earlyoraif}. The essential ingredients of this class of
models are a sequestered sec... | {'timestamp': '2008-04-02T18:15:38', 'yymm': '0803', 'arxiv_id': '0803.2962', 'language': 'en', 'url': 'https://arxiv.org/abs/0803.2962'} |
\subsubsection*{\bibname}}
\usepackage{graphicx}
\usepackage{times}
\usepackage{ifpdf}
\usepackage{amsthm}
\usepackage{algorithm}
\usepackage[algo2e, ruled, vlined]{algorithm2e}
\newcommand{\ignore}[1]{}
\newcommand{\notinproc}[1]{#1}
\newcommand{\onlyinproc}[1]{}
\def\textsf{E}{\textsf{E}}
\def\textsf{Exp}{\textsf{Ex... | {'timestamp': '2021-04-01T02:31:57', 'yymm': '2010', 'arxiv_id': '2010.13048', 'language': 'en', 'url': 'https://arxiv.org/abs/2010.13048'} |
\section{Introduction}
The main difference between open and isolated systems, is the lack of
conservation laws in the former, the most common one being the energy
conservation. For open quantum
systems~\cite{Petruccione,Weiss,Schaller}, another peculiar but less
uniquely defined quantity, quantum coherence, is being l... | {'timestamp': '2017-04-12T02:08:23', 'yymm': '1611', 'arxiv_id': '1611.06720', 'language': 'en', 'url': 'https://arxiv.org/abs/1611.06720'} |
\section{Introduction}\label{intro}
The motion for a compressible viscous, heat-conductive, isotropic Newtonian fluid is described by the system of equations
\begin{equation}\label{1.1}
\left\{
\begin{aligned}
& \rho_t+\nabla\cdot(\rho\bm{u})=0 \\
& \rho\bm{u}_t+\rho\bm{u}\cdot\nabla\bm{u}+\nabla p-\Big(\mu'-\frac{2}{... | {'timestamp': '2021-11-30T02:19:30', 'yymm': '2111', 'arxiv_id': '2111.14136', 'language': 'en', 'url': 'https://arxiv.org/abs/2111.14136'} |
\section{Introduction}
The importance of the corrections due to the mass of the heavy quark in the
jet-production in $e^+e^-$-collisions has been already seen
in the early tests of the
flavour independence of the strong coupling constant \cite{delphi,lep}. The
final high
precision of the LEP/SLC experiments requ... | {'timestamp': '1999-01-24T22:08:14', 'yymm': '9811', 'arxiv_id': 'hep-ph/9811464', 'language': 'en', 'url': 'https://arxiv.org/abs/hep-ph/9811464'} |
\section{Introduction}
\label{sec:int}
Located at a distance of $6.98\Mpc$ \citep{Tully2013}, NGC 5474 is a local star forming galaxy, classified as SAcd pec, belonging to the M 101 Group. With an absolute blue magnitude $\Magn_B\simeq-18.4$, it is among the most luminous satellites of M 101, also known as the Pinwhee... | {'timestamp': '2020-11-26T02:00:49', 'yymm': '2011', 'arxiv_id': '2011.12322', 'language': 'en', 'url': 'https://arxiv.org/abs/2011.12322'} |
\section{The maximal complex subbundle of the tangent bundle}\label{mcs}
Let $\bar{M}$ be a K\"{a}hler manifold with K\"{a}hler structure $J$ and K\"{a}hler metric $g$. We always assume $n = \dim_\mathbb{C}(\bar{M}) \geq 2$. Let $M$ be a real hypersurface in $\bar{M}$. We will denote the induced Riemannian metric on $... | {'timestamp': '2022-03-08T02:36:15', 'yymm': '2203', 'arxiv_id': '2203.03205', 'language': 'en', 'url': 'https://arxiv.org/abs/2203.03205'} |
\section{Introduction}
\label{sec:introduction}
Single stars with main-sequence masses $M \lesssim 100\, M_\odot$ end
their nuclear-burning lives as electron-degenerate objects or with
central electron-degenerate cores. More specifically, the end state is
a carbon-oxygen or oxygen-neon white dwarf (WD) in the case of
... | {'timestamp': '2009-10-14T22:00:04', 'yymm': '0910', 'arxiv_id': '0910.2703', 'language': 'en', 'url': 'https://arxiv.org/abs/0910.2703'} |
\section{Introduction}
Future wireless networks are expected to face unprecedented demands for continuous and ubiquitous connectivity due to the increasing number of mobile users, the evolving deployment of \ac{IoT} networks, and the growing number of novel use cases. Increasing \ac{BS} density and using relays may be... | {'timestamp': '2022-07-26T02:11:35', 'yymm': '2207', 'arxiv_id': '2207.11576', 'language': 'en', 'url': 'https://arxiv.org/abs/2207.11576'} |
\section{Proof of Proposition~\ref{perp-path0}} \label{multi}
The purpose of this section is to lift the framework to \imp{multi-designs}, in order to prove properties of the path recording the interaction between multi-designs (thus in particular, between designs). We show:
\begin{itemize}
\item the existence and uni... | {'timestamp': '2017-07-28T02:08:23', 'yymm': '1707', 'arxiv_id': '1707.08925', 'language': 'en', 'url': 'https://arxiv.org/abs/1707.08925'} |
\section{Introduction}
\label{sec:intro}
The two main goals of non-equilibrium statistical mechanics are the derivation of macroscopic equations from microscopic dynamics and the calculation of
transport coefficients~\cite{Balescu1975, balescu97, ResibDeLeen77}. The starting
point is a kinetic equation that governs th... | {'timestamp': '2010-02-22T13:22:50', 'yymm': '1002', 'arxiv_id': '1002.4103', 'language': 'en', 'url': 'https://arxiv.org/abs/1002.4103'} |
\section{Introduction}
For large-scale inverse problems, which often arise in real life applications, the solution of the corresponding forward and adjoint problems is generally computed using an iterative solver, such as (preconditioned) fixed point or Krylov subspace methods. Indeed, the corresponding linear systems... | {'timestamp': '2022-07-27T02:10:40', 'yymm': '2207', 'arxiv_id': '2207.10372', 'language': 'en', 'url': 'https://arxiv.org/abs/2207.10372'} |
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