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3,212,635,539,706 | arxiv |
\section{Introduction}
Scene text recognition (STR) has attracted great attention in recent years, whose goal is to translate a cropped scene text image into a string.
Thanks to the rapid development of deep learning, modern STR methods have achieved remarkable advancement on public benchmarks \cite{wrong}.
As the hi... |
3,212,635,539,707 | arxiv | \section{Introduction}
X-rays spectroscopy techniques are commonly used on several beamlines at synchrotron facilities to perform experiments in a large field of sciences such as Physics, Chemistry, Environmental Sciences, Biology, and Surface Material Science. During many years, the experiments were generally limited ... |
3,212,635,539,708 | arxiv | \section{Introduction}
Unmanned aerial vehicles (UAVs) have been experiencing a boom in interest lately from industry and research. Indeed, several new applications that rely on UAVs have emerged in recent years in connection with the evolution of wireless networks into 5G and beyond. UAVs have been deployed for aeria... |
3,212,635,539,709 | arxiv |
\section{Introduction}
\input{01-intro}
\section{Related Works}
\noindent\textbf{Mesh-based representation and rendering.}
In computer vision and graphics, polygon mesh has been widely used in 3D scene modeling and rendering~\cite{izadi2011kinectfusion,akenine2019real,liu2019soft}.
Traditional methods utilize mu... |
3,212,635,539,710 | arxiv | \section{Introduction}
\label{intro}
By colliding heavy ions at high energies one hopes to heat and/or compress the matter to energy densities
at which the production of the Quark-Gluon Plasma (QGP) begins~\cite{QGP1,QGP2}.
Lattice QCD calculations can study this
non-perturbative regime of QCD~\cite{LatticeQCD} and a... |
3,212,635,539,711 | arxiv | \section{INTRODUCTION}
\label{sec.introduction}
As the Internet of Things~(IoT) is becoming mainstream, the number of connected devices is growing at an exponential rate~\cite{gartner21billion}.
In this paradigm, IoT devices, which are often geographically distributed at the edge of the network, will generate a mass... |
3,212,635,539,712 | arxiv | \section{Introduction}\label{se:int}
Kernel
methods have been widely used to extend the applicability of many well-known algorithms,
such as the Perceptron~\cite{aizerman65}, Support Vector Machines~\cite{cortes95}, or Principal Component Analysis~\cite{zelenkoAR03}.
Tree kernels are interesting approaches in areas of ... |
3,212,635,539,713 | arxiv | \section{Introduction}
\label{sec_intro}
As 5G continues to roll out across the globe, the world of wireless communications continues to expand and grow. According to a report published by Ericsson in November of 2021, the monthly global data traffic is predicted to grow exponentially over the next five years \cite{er... |
3,212,635,539,714 | arxiv | \section{Introduction}
The last decade has witnessed the development of lattice structures for trapped ultracold neutral atoms or ions, where they can be coherently controlled and manipulated. These lattices have already been very successful as platforms to simulate a large variety of quantum phenomena, including qua... |
3,212,635,539,715 | arxiv | \section{ABSTRACT}
The study of the rotation curves of spiral galaxies reveals a nearly
constant cored density distribution of Cold Dark Matter. N-body simulations
however lead to a cuspy distribution on the galactic scale, with a central
peak. A Bose-Einstein condensate (BEC) of light particles naturally solves
this ... |
3,212,635,539,716 | arxiv | \section{\label{intro} Introduction}
A fundamental problem in quantum chemistry is the dynamics of a quantum system (S) interacting continuously with its bath (B) environments. One outstanding challenge is the description of non-Markovian dynamics, which arises when there is a lack of separation of time scales between... |
3,212,635,539,717 | arxiv | \section{Introduction}
Rings are common attributes of S0 galaxies by the definition of this morphological type. As it
was mentioned by \citet{devauc59}, ''Hubble distinguished two groups of S0 objects:
S0 (1), smooth lens and envelope;... S0 (2): some structure in the envelope in the form of a dark zone and ring...'... |
3,212,635,539,718 | arxiv | \section{Introduction}
Weak gravitational lensing surveys have become a powerful tool for
testing cosmological theories. Until recently, the majority of weak
lensing surveys have only used shape information from a single color.
Some surveys such as
the Sloan Digital Sky Survey (SDSS)\footnote{http://www.sdss.org/}, ... |
3,212,635,539,719 | arxiv | \section{Introduction}
The interest in large and complete synthetic spectral libraries of normal
stars ranges over many different application areas, including ($a$)
automatic analysis and classification of large volumes of data, like those
collected by ongoing spectral surveys, ($b$) derivation of radial velocities
vi... |
3,212,635,539,720 | arxiv | \section{Introduction}
Majorana fermion, which often arises as a quasi-particle excitation in
condensed matter systems, is being studied intensively due to its
indispensable utility in defect-free topological quantum
computation~\cite{Alicea2011}. The Majorana bound state (MBS)
naturally exists in spin-triplet chiral ... |
3,212,635,539,721 | arxiv | \section{Introduction}
The weak neutral current (WNC) was the primary prediction to be
tested in the electroweak $SU(2)\times U(1)$ standard model (SM).
The flavor-conserving structure of the WNC has been verified with
high precision in many processes \cite{pdg}. In the SM, there are no
flavor changing neutral coupling... |
3,212,635,539,722 | arxiv | \section{Introduction}
At sufficiently high temperatures, various gross properties of QCD matter are quite different from the respective properties at zero temperature.
Namely, deconfinement of quarks and gluons, restoration of the isovector chiral symmetry and color screening are the key properties of the thermal ... |
3,212,635,539,723 | arxiv | \section{Introduction}
Since November 2019, the pandemic COVID-19 is still expanding in the world.
The time dependence of the number of daily confirmed new cases, which I call an infection curve for simplicity,
shows clearly a wavy structure in some countries like USA, Japan, Luxembourg and Sweden \cite{JHU}.
Si... |
3,212,635,539,724 | arxiv | \section{Introduction}
Ionized gas in planetary nebulae (PNe) expands with typical velocities
between 10 and 40~\relax \ifmmode {\,\rm km\,s}^{-1}\else \,km\,s$^{-1}$\fi\ (cf. Weinberger 1989; Corradi \& Schwarz 1995),
values which are similar or only slightly larger than those of the winds
from their AGB progenitors,... |
3,212,635,539,725 | arxiv | \part{title}
\documentclass[aps,pre,twocolumn,showpacs]{revtex4-1}
\usepackage{epsfig,graphicx}
\usepackage{natbib}
\usepackage[nooneline]{subfigure}
\begin{document}
\title{Occupation times on a comb with ramified teeth}
\author{A. Rebenshtok, E. Barkai}
\affiliation{Department of Physics, Bar Ilan University, ... |
3,212,635,539,726 | arxiv | \section{Introduction}
The observed velocity of a galaxy consists of two components. The first is its recessional velocity due to the expansion of the universe, i.e., the Hubble flow. This portion of the observed velocity is simply given by the Hubble constant times its distance ($\mathrm{H_{0}}D$). The second componen... |
3,212,635,539,727 | arxiv | \section{Approximating the genus --- Overview}%
\subsection{The graph genus problem}
For a simple graph $G$, let $\mathsf{g}(G)$ be the {\em genus} of $G$, that is, the minimum $h$ such that $G$ embeds into the orientable surface $\mathbb{S}_h$ of genus $h$, and let $\widetilde{\mathsf{g}}(G)$ be the {\em non-orienta... |
3,212,635,539,728 | arxiv |
\section{Baseline methodologies}
\label{sec:baselines}
\noindent In this section, we discuss three baseline methodologies
for identifying need-tweets and availability-tweets.
\subsection{Pattern matching baselines} \label{sub:pattern-match-baselines}
\noindent As stated earlier, most prior studies have used pa... |
3,212,635,539,729 | arxiv | \section*{Introduction}
Iterated integrals as a tool of differential topology have been introduced in the nineteen-fifties \cite{ItInt}.
They have been applied to many problems, including the construction of Hodge-structures on fundamental groups \cite{Hain} and the description of knot invariants \cite{Kont}, just to ... |
3,212,635,539,730 | arxiv | \section{Introduction}
Extremal combinatorics is largely concerned with the extent to which global statistics of an object (such as its \emph{volume} or \emph{density}) control the existence of local substructures. Classical examples include Szemer\'edi's theorem on arithmetic progressions in dense subsets of the integ... |
3,212,635,539,731 | arxiv | \section{Introduction} \label{sec-intro}
The purpose of this work is to understand acoustic wave propagation through a liquid containing bubbles. Our motivation is the use of bubbles in medical ultrasonic imaging as strong sound scatterers at particular frequencies known as Minnaert resonances. Many interesting phys... |
3,212,635,539,732 | arxiv | \section{Introduction}
The sector of the standard model that contains right-handed neutrinos (RHNs) appears, up to this time, to be incomplete. RHNs are necessary for introducing masses. Thus right-handed neutrinos are incorporated in Dirac and Majorana mass terms of the original Lagrangian and when gauge states are re... |
3,212,635,539,733 | arxiv | \section{Introduction}
Hidden Markov models (HMMs; \cite{hmm_seminal}) are commonly used for modeling disease progression, because they capture complex and noisy clinical measurements as originating from a smaller set of latent health states.
When fit to patient data, HMMs yield \textit{state transition probabilities} ... |
3,212,635,539,734 | arxiv | \section{Introduction}
Due to recent developments in information technologies, high-dimensional data, especially time-dependent data, have been routinely collected from a wide range of scientific areas, including economics, finance, neuroscience, genomics, meteorology, among others \citep{Gorrostieta2012, HL13, DP16}.... |
3,212,635,539,735 | arxiv | \section{Introduction}
One of the most important problems in quantum field theory (QFT) is to determine phase structures in the space of parameters.
It is connected to significant information
such as symmetries, energy gap, critical phenomena, topological order, etc.
In particular, second-order phase transitions are es... |
3,212,635,539,736 | arxiv | \section{Introduction}
\label{sec:intro}
Understanding theoretically
the patterns of masses and mixings of ordinary fermions is one of the
long aimed goals in particle physics. Of the 56 parameters in the
Standard Model (SM) Yukawa sector (including Majorana neutrinos) only
22 can be measured at low energy and just 17... |
3,212,635,539,737 | arxiv | \section{Introduction}
Aggregation underlies numerous phenomena ranging from polymerization \cite{Flory} and aerosol behavior \cite{skf} to formation of clouds \cite{cloud} and celestial matters where aggregation plays a significant role in planet and star formation (and perhaps even leads to compositeness of dark mat... |
3,212,635,539,738 | arxiv | \section{Introduction}
The goal of the FASTSUM collaboration \cite{fastsum} is to study spectral properties in thermal QCD using Wilson-type fermions on anisotropic lattices, with $a_\tau/a_s\ll 1$. We employ a fixed-scale approach, in which the temperature is varied by changing $N_\tau$, using the standard relation $... |
3,212,635,539,739 | arxiv | \section{Introduction}
\TabObservations{} \FigContext{} The interstellar medium (ISM) was discovered in
1907 by studying atomic absorption lines (from NaI and CaII) seen in the visible
spectrum of bright stars. The first interstellar molecules (CN, CH, and \chem{CH^{+}}{})
were also detected in the same way in the yea... |
3,212,635,539,740 | arxiv | \section{Introduction}\label{sec:intro}
Increased access to visualizations on mobile devices in contexts like online media~\cite{Fedeli2018,Lu2017} demands knowledge and tools for transitioning communicative visualization designs across display sizes.
The process of designing for multiple display sizes, specifically f... |
3,212,635,539,741 | arxiv | \section{Introduction}
The non-Fermi liquid (NFL)
is one of the most fascinating phenomena in modern condensed matter physics. It violates
the fundamental
Landau paradigm
that quasiparticles must become weakly damped at low enough energies.
The key feature of a NFL
is a power-law form of the ferm... |
3,212,635,539,742 | arxiv | \section{Introduction}
The study of the physical properties of the dust and gas at the
centres of active galaxies is of great observational interest. Its
significance is inextricably linked to the activity observed in these
sources since it is the gas and the dust that is ultimately the fuel
for the activity. The du... |
3,212,635,539,743 | arxiv | \section{Introduction. }
Maldacena's $AdS/CFT$ correspondence
\cite{MAL} has spurred interest in Anti-de
Sitter supergravity theories. A particularly interesting case is the
$AdS_3/CFT_2$ correspondence \cite{MALSTR,MAR,BOER,SEIKUTGIV,DMW}.
In this case string theory on $AdS_3\times S^3\times M_4$
with $RR$ flux is... |
3,212,635,539,744 | arxiv | \section{INTRODUCTION}
As a well-established tracer of the newly formed massive stars and star
associations and clusters, the distribution of H {\sc ii} regions has sparked a
long interest since the pioneering investigations in nearby spiral galaxies, as
reviewed by \citet{Kennicutt92}. Extensive statistical analys... |
3,212,635,539,745 | arxiv | \section{Introduction}
Since initial observations of the spin Seebeck effect \cite{Uchida2008Nature, Uchida2010NatMaterspinSeebeck, Jaworski2010NatMaterspinSeebeck, Uchida2010APLspinSeebeck}, the conversion between spin and heat currents has been actively investigated, which has opened up an emerging research area cal... |
3,212,635,539,746 | arxiv | \section{The typical differential operators}
{\footnotesize Operators on a manifold with singularities (of conical, edge, or corner type), expressed in stretched coordinates, are degenerate in a typical way. We illustrate that for the case of differential operators, motivated by the shape of Laplacians belonging to co... |
3,212,635,539,747 | arxiv |
\subsection{Dataset}
In our experiments, the dataset we employ is the public available dataset UK Domestic Application Level Electric (UK-DALE) to perform the experiment. UK-DALE records 5 houses, all of the appliance-level power data is active power sampled every 6 seconds, while the aggregate power data is a mixtu... |
3,212,635,539,748 | arxiv | \section{Introduction}
In this paper we provide general position techniques that fully
utilize a general position characterization of codimension one
manifold factors of dimension $n\geq 4$.
A {\it codimension one manifold
factor} is a space $X$ such that $X \times \mathbb{R}$ is a manifold.
The famous Cell-like Appro... |
3,212,635,539,749 | arxiv | \section{\label{intro}Introduction}
Heavy fermion (HF) behavior has mostly been seen in \textit{f}-electron metals. Such compounds are called heavy fermions because in these materials the current carriers behave as if they have a large mass ($\sim$ 10$^{2}$--$10^{3}$ times the free electron mass). ${\rm LiV_2O_4}$, fi... |
3,212,635,539,750 | arxiv | \subsection{\label{subsec:GUE_GOE_GSE}Example: Scaling of the gap when local
terms are from canonical Gaussian ensembles}
We first answer the following question: What is the probability that
all the eigenvalues of an instance of an $n\times n$ G(O/U/S)E matrix
are $\epsilon-$close? In other words, what is the probabili... |
3,212,635,539,751 | arxiv | \section{Introduction}
\subsection{Classical exponents of approximation} \label{intro}
Let $n\geq 1$ be an integer and $\ux=(\xi_{1},\ldots,\xi_{n})\in\mathbb{R}^n$
with $\{1,\xi_{1},\ldots,\xi_{n}\}$ linearly independent over $\mathbb{Q}$.
Let the (possibly infinite) exponents of approximation
$\om$ and $\wo... |
3,212,635,539,752 | arxiv | \section{Exciton Optics}
The close relationship between optics and excitonics represents the primary and most versatile avenue for probing and manipulating excitons in transition metal dichalcogenides\,\cite{Wang18, Mueller18}. Excitons in semiconducting TMDs are typically generated via optical excitation\,\cite{mak10,... |
3,212,635,539,753 | arxiv | \section{Introduction}\label{one}
Can we prove that quantum dynamics must be linear? That the Schrodinger equation must be linear? What assumptions are needed? Is there a reason in principle that quantum dynamics is linear? If not, quantum dynamics could be a linear approximation of a nonlinear theory; then experiments... |
3,212,635,539,754 | arxiv | \section{Introduction}
Modern Internet services, such as those at Google, Yahoo!, and Amazon,
serve large numbers of users simultaneously;
for example, both eBay and Facebook claim over 300 million users
worldwide.\footnote{eBay: Franco Travostino and Randy Shoup, Invited
talk at workshop on Large Scale Distribu... |
3,212,635,539,755 | arxiv | \section{Introduction}
Spin ladder systems have attracted considerable attention from both experimentalists and theoreticians alike~\cite{ED, review}.
One of the most striking features of the simple spin-$\case12$ Heisenberg ladder is that the spin excitations are gapful (gapless) when the
number of legs is even (odd... |
3,212,635,539,756 | arxiv | \section{Introduction}
Nowadays an overwhelming, direct and indirect, observational
evidence supports the idea that the Universe is currently
undergoing a phase of accelerated expansion. The most recent and
precise confirmation of this rather unexpected feature (see,
however \cite{Turner97,Priester}) was provided by ... |
3,212,635,539,757 | arxiv | \section{Introduction}
The biggest challenge for all the schemes that quantize gravity (in particular the
background-independent schemes),
beside obtaining a solid description of the fundamental
degrees of freedom for quantum spacetime, is to produce the testable
predictions \cite{aaa,do}.
In the background-indepe... |
3,212,635,539,758 | arxiv |
\section{NEW Outline}
\section{Introduction} \label{sec:intro}
In this paper, we consider fluid-structure interaction (FSI) of incompressible fluids
and bulk elastic solids. FSI arises in many scientific and engineering applications
including flow-induced vibrations of structures (i.e.,~aircraft wings, under... |
3,212,635,539,759 | arxiv | \section{Introduction}
\label{sec:intro}
Multidimensional hydrodynamical effects are crucial to power the explosion of massive stars, known as core-collapse supernovae (CCSNe). The gravitational contraction of the iron core of the progenitor into a proto-neutron star triggers a bounce of the core which produces a stal... |
3,212,635,539,760 | arxiv | \section{Introduction}
The $B_c$ meson, first observed by the CDF Collaboration \cite{Abe:1998wi}, is interesting since it has the structure of the heavy quarkonium but it decays weakly. Therefore, this meson is well suited to study both quarkonium and weak interaction features within the same hadronic system. As ... |
3,212,635,539,761 | arxiv |
\section{%
\@startsection
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{%
\normalfont\small\bfseries
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\def\@hangfrom@section#1#2#3{\@hangfrom{#1#2}\MakeTextUppercase{#3}}%
\def\subsection{%
\@startsection
{subsection}%
{2}%
{\z... |
3,212,635,539,762 | arxiv | \section{\label{sec:level1} Introduction}
Recent success in detecting the charge order Bragg peaks in many different classes of high $T_c$ cuprates based on modern x-ray scattering techniques \cite{Comin_Review} has led to renewed interest in the charge order in La$_2$CuO$_4$-based cuprates. In the case of Nd$^{3+}$ c... |
3,212,635,539,763 | arxiv | \section{The main trichotomy}
Let $X$ be a smooth complex projective variety. There are three main types
of varieties. (Not every variety is of one of these three types, but minimal
model theory relates every variety to one of these extreme types.)
{\it Fano. }This means that $-K_X$ is ample. (We recall the definitio... |
3,212,635,539,764 | arxiv | \section{Introduction}
Simulating quantum dynamics of interacting many-body systems is one of the main potential applications of quantum
computing, going back to Feynman's visionary work on simulating physics with quantum computers~\cite{
feynman_quantum_simulators}. For quantum many-body systems evolving under a gener... |
3,212,635,539,765 | arxiv | \section{Introduction}
A quantum bit (qubit) is a quantum system with a two-dimensional
Hilbert space, capable of existing in a superposition of Boolean states
and of being entangled with the states of other qubits [1].
More precisely a qubit is the amount of the information which is contained
in a pure quant... |
3,212,635,539,766 | arxiv | \section{Introduction}
It is well established that dark matter exists in our universe and corresponds to 26.4\% of its total energy
content~\cite{PhysRevD.98.030001}.
Weakly Interacting Massive Particles (WIMPs) are dark matter candidate particles that are frequently considered
because of the balance among their inferr... |
3,212,635,539,767 | arxiv | \section{Introduction }
Much attention has long been devoted to finding macroscopic
magnetic ordering phenomena in organic materials. Experimentally,
ferromagnetism has been discovered in pure carbon systems, such as
carbon foam, graphite, oxidized C$_{60}$ and polymerized
rhombohedral C$_{60}$ \cite{r1,r2,r3,r4,r5}, ... |
3,212,635,539,768 | arxiv | \section{Introduction}
The acceleration of the late-time universe is one of
the most important problems in cosmology.
Within the framework of general relativity, the acceleration
is supposed to be caused by unknown
dark energy. The simplest option for dark energy is
vacuum energy, but it is hard to explain why the... |
3,212,635,539,769 | arxiv | \section{Introduction}
Hydrogen(H)-deficient Post-Asymptotic Giant Branch (AGB) stars
display
a wide variety of surface abundances, ranging from the
almost pure
helium atmospheres of O(He) stars to the helium(He)-
carbon(C)- and
oxygen(O)- rich surfaces of WR-CSPN and PG1159 stars
(see Werner \&
Herwig 2006 for a... |
3,212,635,539,770 | arxiv | \section{Introduction}
Observations indicate that stars born at present time in magnetized rotating cores of molecular clouds~\citep{shu87, dudorov91, dudorov95, mckee07}. Centrifugal and electromagnetic forces lead to the formation of a disk-like structure during the gravitational collapse of the molecular cloud core... |
3,212,635,539,771 | arxiv | \subsection{Statistics of Benchmark Data Sets}
In this section, we summarize the statistics of the four natural language processing datasets used in our experiments in Table \ref{table:datastats}.
For SQuAD, since the dataset does not annotate supporting facts, we approximately estimate supporting facts by counting to... |
3,212,635,539,772 | arxiv | \section{Introduction}
Cross sections at collider experiments can often be reliably calculated within the framework of
perturbative Quantum Chromodynamics (pQCD). The crucial foundation for such computations
are so-called factorization theorems that allow for a systematic separation of perturbative
and non-perturbati... |
3,212,635,539,773 | arxiv | \section{Introduction}
\label{intro}
For nearly eight decades it has been recognized that superconducting
properties can leak out from a superconductor into a neighboring
metallic region\cite{Holm1932:ZP,parks,Wolf:1985} which by itself
would not be superconducting.
This phenomenon is known as the superconducting
p... |
3,212,635,539,774 | arxiv | \section{Introduction}
The complete stellar life cycle is significantly shaped by its mass, which is in-turn determined by the less understood evolutionary stages of star formation and its related processes (\citealt{doi:10.1146/annurev-astro-081811-125528, 2015arXiv150906382A,article} and references therein).
As low-... |
3,212,635,539,775 | arxiv |
\section{Introduction}
\label{sec:introduction}
Videos hold a great potential to communicate educational and scientific information. This is, for instance, reflected by e-Learning platforms such as Udacity (https://udacity.com) or Coursera (http://www.coursera.org). Another type of Web portals offers also access to ... |
3,212,635,539,776 | arxiv | \section{Introduction}
\label{introduction}
Web users have been exposed to a wide variety of privacy intrusions since the introduction of third-party cookies in 1994 \cite{schwartzGivingWebMemory2001}. In the ensuing years there has been a steady increase in the prevalence and sophistication of web tracking to the poi... |
3,212,635,539,777 | arxiv |
\section{Introduction} \label{sec:introduction}
Technical debt (TD) was first mentioned as a concept by Cunningham close to 30 years ago \cite{10.1145/157709.157715}, when he wrote the following lines: \emph{``Shipping first time code is like going into debt. A little debt speeds development so long as it is paid bac... |
3,212,635,539,778 | arxiv | \section{Introduction}
We study a decentralized decision-making problem with restricted communication between three agents with non-aligned objectives.
As depicted in Fig. \ref{fig:Cascademulti}, we consider a Cascade channel where information travels from a strategic encoder to a decoder through a strategic relay. ... |
3,212,635,539,779 | arxiv | \section{Introduction.}
In recent years, there has been considerable interest
in different dynamical models which can evolve without any
tuning of parameters to the {\it Self-Organized Critical}
(SOC) state.
The concept of Self-Organized Criticality has been introduced
by Bak, Tang, and Wiesenfeld~\cite{BTW}, through... |
3,212,635,539,780 | arxiv | \section{Introduction}
Low-mass X-ray binaries consist of either a neutron star or a black hole that accretes matter from a low-mass companion star, where mass transfer occurs because the donor star overflows its Roche-lobe. The soft X-ray transients form a sub-group of low-mass X-ray binaries. The vast majority of t... |
3,212,635,539,781 | arxiv | \section{\label{intro}Introduction}
One of the outstanding questions in extragalactic astronomy is how matter in the universe assembled into the structures we see today. An approach to tackle this question is to study the formation and evolution of galaxies, since they are luminous beacons of the baryon content of the... |
3,212,635,539,782 | arxiv | \section{\label{ackno} Acknowledgments}
This work is partially supported by the Scientific and Technological Research
Council of Turkey (T{\"U}B\.{I}TAK). B.T. is also partially supported by the
T{\"U}B\.{I}TAK Kariyer Grant 104T177.
|
3,212,635,539,783 | arxiv | \section{Introduction}\label{sec:introduction}}
\IEEEPARstart{A}{recent} study~\cite{DBLP:conf/ndss/KotziasBVC19} shows that it takes more than 200 days for an enterprise to
align 90\% of their machines with the latest (not known to be
vulnerable) software version given the need to perform regression testing~\cite{DB... |
3,212,635,539,784 | arxiv | \section{\label{}}
\section{INTRODUCTION}
Black holes with a wide range of masses could have formed in the early Universe as a result of the great compression associated with the Big Bang \cite{h71,zn}. A
comparison of the cosmological density at a time $t$ after the Big Bang with the density associated with a black... |
3,212,635,539,785 | arxiv | \section{Supplemental Material}
\end{document}
\section{Introduction}
\thispagestyle{plain}
\emph{Conversational search} is concerned with creating agents that fulfill an information need by means of a \emph{mixed-initiative} conversation, rather than the traditional turn-taking interaction models exhibited in search... |
3,212,635,539,786 | arxiv |
\section{Property closure}
\label{sec:property-closure}
\subsection{Cooperative winning set}
\label{sec:cooperative-winning-set}
In the following, we will present an algorithm for computing pairs of specifications that allow players to cooperate.
For that purpose, some definitions are needed.
Let $\Sigma$ be a suit... |
3,212,635,539,787 | arxiv | \section{Introduction}
Central to probability theory are Gaussian and Poisson distributions.
In ergodic theory, they both play a singular role through canonical
constructions we briefly recall:
\begin{itemize}
\item Starting from a symmetric Borel measure $\sigma$ on $\mathbb{T}$, there exists
a unique centered statio... |
3,212,635,539,788 | arxiv | \section{Introduction}
\label{Introduction}
The discovery of a Higgs-like field at the CERN Large Hadron Collider \cite{ATLAS:2012oga}
provides a verification of the reality of the electroweak vacuum energy, and consequently
of the cosmological constant problem. The latter is nothing more than the simple statem... |
3,212,635,539,789 | arxiv | \section{Introduction}
It is known (see, e.g., \cite{MK}, \cite{S}) that the light propagation
through
diffraction gratings may exibit strong resonances at certain frequencies.
This is useful in applications. In this paper we study electromagnetic
(EM) wave scattering by many small impedance particles $D_m$,
$... |
3,212,635,539,790 | arxiv | \section{Introduction}
Candidate fractional quantum Hall (FQH) states which exhibit non-Abelian quasiparticle excitations have been predicted to appear in the second Landau level (LL) for certain filling fractions.~\cite{mooreread,readrezayi}
Recent proposals for performing intrinsic fault-tolerant quantum computation ... |
3,212,635,539,791 | arxiv | \subsubsection{Coherence Estimation\label{sec:CohEst}}
The coherency between two zero mean jointly
stationary time series $x(t)$ and $y(t)$ is defined as
\begin{equation} \label{eq:coh}
\rho(f) = \frac{S_{xy}(f)}{\sqrt{S_x(f) S_y(f)}},
\end{equation}
where $S_x(f)$ denotes the spectrum of the process $x(t)$, $S_y(f)... |
3,212,635,539,792 | arxiv | \section{Introduction}\label{sec:intro}
\textbf{Overview:}
Underwater networks enable various applications such as oceanographic data collection, pollution monitoring~\cite{Sadhu2018ucomms}, and disaster prevention using static nodes~\cite{rahmati2017unisec} and/or mobile vehicles~\cite{rahmati2018probabilistic}. In m... |
3,212,635,539,793 | arxiv | \section{Introduction}
3D scene understanding using point clouds has been an essential and challenging task for many robotics applications, including autonomous driving systems. One of the key tasks in 3D scene understanding is 3D Panoptic segmentation (PS), with two sub-tasks, semantic and instance segmentation. The ... |
3,212,635,539,794 | arxiv | \section{The extended TNS model for the cross power spectrum}
\label{sec:xTNS}
\subsection{Preliminaries}
\label{sec:preliminaries}
Throughout the report, we work with the distant-observer limit, and assume that the line-of-sight direction is parallel to the $z$-axis. Then the {\it observed} redshift space may be writ... |
3,212,635,539,795 | arxiv | \section{Introduction} \label{intro}
As the first Local Group supernova
in the era of modern instrumentation, Supernova 1987A (SN 1987A) is at the center of the
investigation into supernova explosions and their aftermath, and into
the formation of compact objects; see review articles by \citet{mcc93} and \citet{arn89}... |
3,212,635,539,796 | arxiv | \section*{Introducci\'on}
\section{Introducción}
Durante la segunda mitad del siglo XIX y los inicios del siglo XX comenzaron a establecerse por todo el mundo las primeras sociedades matemáticas \cite{FUR2}. Entre ellas, la \textit{London Mathematical Society} en 1865, la \textit{Societé Mathématique de France} en 187... |
3,212,635,539,797 | arxiv | \section{Introduction}
\label{subsec:text-normalization}
\label{subsec:goals}
The research in natural language processing (NLP) has traditionally focused in the resolution of the \emph{big problems}, such as automatic translation, understanding, summarizing and text generation. However, there are plenty of not so wel... |
3,212,635,539,798 | arxiv |
\section{Conversations Gone Awry}
An interesting avenue of work that has been investigated recently is the ability to preempt a conversation if you know further discussion will result in a personal attack \cite{zhang_2018_ConversationsGoneAwry, chang_2019_TroubleHorizonForecasting}.
This differs from other frameworks... |
3,212,635,539,799 | arxiv | \section{Introduction} \label{sec:intro}
One of the most-studied variants of the two-dimensional Ising
model is the case of random bonds.
While realizations of Ising models that include randomness
come much closer to approximating reality, they are very
much harder to study at any level. Even in two dimensions
exact r... |
3,212,635,539,800 | arxiv | \section{Introduction}
${\cal N}=4$ SYM has been the subject of great attention over the last decade and substantial progress has been made. Most of the progress, however, has been restricted either to perturbation theory, the planar limit (where integrability techniques can be used) or super-symmetric/protected obser... |
3,212,635,539,801 | arxiv | \section{Introduction}
Parton distribution functions (PDFs) of the proton cannot be predicted from first principle and they used to be determined in deep inelastic scattering (DIS) experiments using point-like beams of charged or neutral leptons to probe the proton or other nucleon targets, in earlier fixed target mode... |
3,212,635,539,802 | arxiv | \section{Introduction}
Modern life, with its increasing reliance on digital technologies, is opening unanticipated opportunities for the study of human behavior and large scale societal trends. Cell phones have been playing a pivotal role in this revolution, serving as ubiquitous sensors, and the default point of cont... |
3,212,635,539,803 | arxiv | \section{Introduction}
\medskip
Firms increasingly belong to a variety of inter-organizational networks such as complex supply chains, strategic alliances, or other types of partnerships. Membership in these networks can evidently yield economic benefits, but they also necessitate substantial additional security inv... |
3,212,635,539,804 | arxiv | \section{#1}
\setcounter{equation}{0}}
\renewcommand{\subjclassname}{%
\textup{2000} Mathematics Subject Classification}
\begin{document}
\title[$L_p$-regularity of stochastic singular integral operators]
{Boundedness of stochastic singular integral operators
and its application to stochastic partial di... |
3,212,635,539,805 | arxiv |
\section{Introduction}
A \textit{K\"ahler group} is a group which can be realized as fundamental group of a compact K\"ahler manifold. K\"ahler groups form an intriguing class of groups. A fundamental problem in the field is Serre's question of ``which" finitely presented groups are K\"ahler. While on one side there ... |
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