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\section{Introduction}
Let $\alpha>0$. For $1\le p<\infty$, we denote by $L\pla$ the space of all measurable functions $f$ on $\C$ such that
\[
\|f\|_{L\pla}^p:=\int_\C \left|f(z) e^{-\alpha|z|^{2\ell}/2}\right|^p \,d\nu(z) < \infty,
\]
where $d\nu$ denotes the Lebesgue measure on $\C$.
For $p=\infty$, $L... | {
"timestamp": "2017-12-15T02:08:35",
"yymm": "1712",
"arxiv_id": "1712.05250",
"language": "en",
"url": "https://arxiv.org/abs/1712.05250"
} |
\section{Introduction}
\label{intro}
Essentially all correlated electron high temperature superconductors display an anomalous metallic state at temperatures above the superconducting critical
temperature at optimal doping \cite{Keimer15,Matsuda2010,SK2011}. This metallic state has a `strange' linearly-increasing depe... | {
"timestamp": "2018-05-24T02:08:31",
"yymm": "1712",
"arxiv_id": "1712.05026",
"language": "en",
"url": "https://arxiv.org/abs/1712.05026"
} |
\section*{Potential items to be added in journal paper:}
\section{Introduction}
A key feature of the upcoming 5G technology is the support for Ultra-Reliable and Low Latency Communication (URLLC) \cite{carvalho2016random}. URLLC may be supported both through the 5G new air interface \cite{ji2017introduction} o... | {
"timestamp": "2017-12-15T02:05:54",
"yymm": "1712",
"arxiv_id": "1712.05148",
"language": "en",
"url": "https://arxiv.org/abs/1712.05148"
} |
\section{Introduction \label{Introduction}}
Supernova remnants (SNRs) are the visible manifestation of the interaction between material ejected in a supernova explosion (SN) and the surrounding circumstellar and interstellar medium. SNRs radiate across the entire magnetic spectrum from radio wavelengths to $\gamma$-ra... | {
"timestamp": "2017-12-15T02:10:29",
"yymm": "1712",
"arxiv_id": "1712.05331",
"language": "en",
"url": "https://arxiv.org/abs/1712.05331"
} |
\section{Introduction}
In \cite{FLZalternating} Friedl, Livingston and Zentner studied the knot concordance
group $\mathcal{C}$ modulo the subgroup $\mathcal{C}_\text{alt} \subset \mathcal{C}$
spanned by alternating knots. In particular they ask the following question.
\begin{Question}
Which sums of torus knots are ... | {
"timestamp": "2019-01-17T02:16:03",
"yymm": "1712",
"arxiv_id": "1712.05252",
"language": "en",
"url": "https://arxiv.org/abs/1712.05252"
} |
\section{Introduction}
This work is devoted to the analysis of nonlinear damped wave equations for positive operators acting in Hilbert spaces. More precisely, for a densely defined positive operator ${\mathcal L}$ in a separable Hilbert space ${\mathcal H}$ we consider the Cauchy problem
\begin{equation}\label{EQ: No... | {
"timestamp": "2017-12-15T02:01:32",
"yymm": "1712",
"arxiv_id": "1712.05009",
"language": "en",
"url": "https://arxiv.org/abs/1712.05009"
} |
\section{Introduction}
Higher-order derivative interactions naturally appear
in effective field theories.
In particular, in the system with gravity,
we need to take into account such terms
since various higher-order corrections can be
relevant to the dynamics.
However, higher-derivative interactions often lead to... | {
"timestamp": "2018-05-21T02:03:32",
"yymm": "1712",
"arxiv_id": "1712.05017",
"language": "en",
"url": "https://arxiv.org/abs/1712.05017"
} |
\section{Introduction}
Cosmic strings are one-dimensional topological defects formed by spontaneous symmetry breaking in the early universe. They were first proposed in the 1970s \cite{Kibble:1976sj} and have evoked ongoing cosmological interest (see Ref. \cite{Vilenkin:2000} for review). The initially formed defects ... | {
"timestamp": "2018-02-07T02:03:46",
"yymm": "1712",
"arxiv_id": "1712.05060",
"language": "en",
"url": "https://arxiv.org/abs/1712.05060"
} |
\section{Introduction} \label{sec:intro}
The history of formation of the Mars' moons Phobos and Deimos is still an open question. It has been the subject of several studies which point to a capture origin, in-situ or impact generated formation \citep[and references therein]{2011A&ARv..19...44R,2015Icar..252..334C,201... | {
"timestamp": "2017-12-18T02:05:24",
"yymm": "1712",
"arxiv_id": "1712.05154",
"language": "en",
"url": "https://arxiv.org/abs/1712.05154"
} |
\section*{Acknowledgements}
We thank Giacomo Bighin and Luca Salasnich for stimulating discussions. We also thank Stefano Giorgini and Tomoki Ozawa for useful comments. This work has been supported by the QUIC grant of the European Horizon2020 FET program and by Provincia Autonoma di Trento.
\par
| {
"timestamp": "2017-12-15T02:01:52",
"yymm": "1712",
"arxiv_id": "1712.05022",
"language": "en",
"url": "https://arxiv.org/abs/1712.05022"
} |
\section{Relativistic heavy-ion collisions}
\label{sec:1}
\sectionmark{Relativistic heavy-ion collision}
The relativistic heavy-ion collision experiments are a perfect tool for studying, in a controlled and reproducible manner, the properties of strongly interacting matter at high energies. Unlike the collisions of mor... | {
"timestamp": "2017-12-15T02:07:30",
"yymm": "1712",
"arxiv_id": "1712.05213",
"language": "en",
"url": "https://arxiv.org/abs/1712.05213"
} |
\section{Introduction}\label{sec:1}
Black holes in more than four spacetime dimensions have been one of the most interesting subjects of general relativity in the last two decades. For example, the statistical counting of black-hole entropy was performed in string theory~\cite{Strominger:1996sh}, which needs higher-dim... | {
"timestamp": "2018-01-12T02:05:44",
"yymm": "1712",
"arxiv_id": "1712.05132",
"language": "en",
"url": "https://arxiv.org/abs/1712.05132"
} |
\section{Proposed Algorithm}
\label{sec:proposed}
We claim that an action can be recognized from a video by identifying a set of key segments presenting important action components. So we design a neural network that learns to measure the importance of each segment in a video and automatically selects a sparse subset ... | {
"timestamp": "2018-04-04T02:12:23",
"yymm": "1712",
"arxiv_id": "1712.05080",
"language": "en",
"url": "https://arxiv.org/abs/1712.05080"
} |
\section{Introduction}
The research field of anomalous diffusion and transport \cite{Shlesinger74,Scher75,Bouchaud1990,AvrahamHavlin,Hughes, BouchaudAnnPhys90,Bouchaud92,Metzler01,FractDyn2011,GoychukACP12,MetzlerPCCP} currently flourishes getting ever more experimental support and manifestations in such diverse resea... | {
"timestamp": "2018-11-12T02:09:40",
"yymm": "1712",
"arxiv_id": "1712.05238",
"language": "en",
"url": "https://arxiv.org/abs/1712.05238"
} |
\section{Introduction}
General theory of relativity is widely regarded to be the best theory of gravity as over the years it has passed many observational tests with flying colors. Significant observational aspects such as the perihelion precission of Mercury's orbit, gravitational lensing, redshift in the light spectr... | {
"timestamp": "2018-04-11T02:12:37",
"yymm": "1712",
"arxiv_id": "1712.05149",
"language": "en",
"url": "https://arxiv.org/abs/1712.05149"
} |
\section{Introduction}
Quantum simulators~\cite{feynman82} provide the opportunity for a controlled quantum system to emulate the behavior of another system whose properties we would like to better understand. Progress towards building quantum simulators is occurring rapidly, with demonstrations up to and beyond 50 qub... | {
"timestamp": "2017-12-15T02:09:14",
"yymm": "1712",
"arxiv_id": "1712.05282",
"language": "en",
"url": "https://arxiv.org/abs/1712.05282"
} |
\section{INTRODUCTION}
The study of small bodies of the solar system was changed forever in 1977, with the discovery of a large icy object moving on an orbit between those of Saturn and Uranus \citep{1979IAUS...81..245K}. That object was subsequently named Chiron. It was soon realised that its orbit was dynamically uns... | {
"timestamp": "2017-12-15T02:01:02",
"yymm": "1712",
"arxiv_id": "1712.04995",
"language": "en",
"url": "https://arxiv.org/abs/1712.04995"
} |
\section{Introduction}\label{sec:1}
It has been noted for almost two decades \citep{1998Natur.395..670G} that many long-duration GRBs show the presence of an associated unusually energetic supernova (SN) of type Ic (hypernova, HN) as well as of a long-lasting X-ray afterglow \citep{Costa1997}. Such HNe are unique in t... | {
"timestamp": "2018-10-25T02:02:39",
"yymm": "1712",
"arxiv_id": "1712.05000",
"language": "en",
"url": "https://arxiv.org/abs/1712.05000"
} |
\section
In Quantum field theory (QFT) existence of a given theory means, that we can control its
behavior at some scales (short or large distances) by
renormalization theory \cite{Collins}. If the theory exists, than
we want to solve it, which means to determine what happens on
other
scales. This is the problem (... | {
"timestamp": "2017-12-15T02:02:37",
"yymm": "1712",
"arxiv_id": "1712.05056",
"language": "en",
"url": "https://arxiv.org/abs/1712.05056"
} |
\section{Introduction}
College sports organized The National Collegiate Athletic Association(NCAA) are very popular in the United States. And the most popular sports include football and men's basketball. According to a survey conducted by Harris Interactive, NCAA's inter-college competition is attracting around 47 per... | {
"timestamp": "2017-12-15T02:04:18",
"yymm": "1712",
"arxiv_id": "1712.05112",
"language": "en",
"url": "https://arxiv.org/abs/1712.05112"
} |
\section{Introduction and Background}
The classical braid groups $B_n$ on the plane were introduced by Artin \cite{name}. Geometrically, elements of such braid groups appear as a collection of $n$ paths emanating from a set of $n$ distinct points on the plane which wind around each other and return to some permutation... | {
"timestamp": "2017-12-15T02:02:37",
"yymm": "1712",
"arxiv_id": "1712.05057",
"language": "en",
"url": "https://arxiv.org/abs/1712.05057"
} |
\section{Introduction}
In 2010, the CREMA (Charge Radius Experiment with Muonic Atoms) collaboration extracted the proton charge radius from measurements of the $2S-2P$ transition in muonic hydrogen ($\mu$H), a proton orbited by a muon. It was found to deviate by about
7$\sigma$~\cite{Pohl:2010zza, Antognini:1900ns... | {
"timestamp": "2017-12-15T02:06:55",
"yymm": "1712",
"arxiv_id": "1712.05187",
"language": "en",
"url": "https://arxiv.org/abs/1712.05187"
} |
\section{Introduction}
The Landau Fermi liquid (FL) theory is one of the corner-stones of condensed matter physics that explains most of the basic properties of materials~\cite{paper47}.
Another known generic liquid is the Luttinger liquid~\cite{paper48}, which seems to be another fixed point of interacting fermionic ... | {
"timestamp": "2019-03-05T02:03:59",
"yymm": "1712",
"arxiv_id": "1712.05303",
"language": "en",
"url": "https://arxiv.org/abs/1712.05303"
} |
\section{Introduction}
Market timing is an investment technique whereby an investment manager
(professional or individual) attempts to anticipate the price movement
of asset classes of securities, such as stocks and bonds, and to
switch investment money away from assets with lower anticipated
returns into assets with ... | {
"timestamp": "2017-12-15T02:02:00",
"yymm": "1712",
"arxiv_id": "1712.05031",
"language": "en",
"url": "https://arxiv.org/abs/1712.05031"
} |
\section{Introduction}
\label{section_1}
\IEEEPARstart{D}{eep} Learning (DL) algorithm, which is materialized by Deep Neural Networks (DNNs) for learning meaningful representations~\cite{bengio2013representation}, is a very hot research area during recent years~\cite{krizhevsky2012imagenet,farabet2013learning,tompson... | {
"timestamp": "2018-02-27T02:03:40",
"yymm": "1712",
"arxiv_id": "1712.05043",
"language": "en",
"url": "https://arxiv.org/abs/1712.05043"
} |
\section{Introduction}
There are growing evidences for the co-evolution between the central supermassive black holes
and their host galaxies \citep{Kormendy:13}, including the strong correlation between the mass
of the black hole and the luminosity, stellar velocity dispersion, or the stellar mass in the
galaxy sphero... | {
"timestamp": "2018-03-22T01:07:50",
"yymm": "1712",
"arxiv_id": "1712.04964",
"language": "en",
"url": "https://arxiv.org/abs/1712.04964"
} |
\section{Introduction}}
At the core of image based 3D reconstruction systems~\cite{Agarwal_11,Heinly_CVPR15}, one fundamental task is to establish reliable point correspondences across multiple images of the reconstructed scene, which are captured from different viewpoints, positions, and usually at different time. Pop... | {
"timestamp": "2017-12-15T02:08:58",
"yymm": "1712",
"arxiv_id": "1712.05271",
"language": "en",
"url": "https://arxiv.org/abs/1712.05271"
} |
\section{Introduction}
\label{perugia_mini4:sec:1}
For the numerical approximation of the Helmholtz problem,
it has been shown that, by using
non-polynomial basis functions, it is possible
to reduce the pollution effect in finite element approximations.
One special class of such methods are Trefftz finite element met... | {
"timestamp": "2018-08-17T02:07:03",
"yymm": "1712",
"arxiv_id": "1712.05174",
"language": "en",
"url": "https://arxiv.org/abs/1712.05174"
} |
\section{Introduction}
The widely used Jensen's inequality for convex functions, attributed to Danish
mathematician Johan Jensen, dates back to 1906\cite{jensen1906fonctions}.
The literature contains numerous bounds on the Jensen gap, defined as $\J{f} = \E{f\left(X\right)}-f\left(\E{X}\right)$, where $X$ is a rando... | {
"timestamp": "2018-11-06T02:44:31",
"yymm": "1712",
"arxiv_id": "1712.05267",
"language": "en",
"url": "https://arxiv.org/abs/1712.05267"
} |
\section{Introduction}
A small value (several tens keV) of the spreading width of the Isobaric Analog Resonances (IARs), $\Gamma^{\downarrow}_{A}$, is the impressive manifestation of the approximate isospin-symmetry conservation in medium-heavy mass nuclei. The spreading width of an arbitrary giant resonance (including... | {
"timestamp": "2017-12-15T02:05:48",
"yymm": "1712",
"arxiv_id": "1712.05146",
"language": "en",
"url": "https://arxiv.org/abs/1712.05146"
} |
\section{Introduction}
\label{sec:intro}
One of the outstanding problems of statistical physics is the nature of
the ordered phase of spin glasses. While this problem is primarily of
interest to researchers in statistical and condensed matter physics,
spin-offs from its study have found their way into different fields... | {
"timestamp": "2018-03-08T02:10:23",
"yymm": "1712",
"arxiv_id": "1712.04971",
"language": "en",
"url": "https://arxiv.org/abs/1712.04971"
} |
\section{Group reconstruction Methods}
\label{appendix:method}
It is known that the identification of the groups in redshift space is hampered by several difficulties. Of particular concern are redshift-space distortions such as the elongation of groups along the line of sight due to the peculiar velocities of the gro... | {
"timestamp": "2018-03-30T02:06:29",
"yymm": "1712",
"arxiv_id": "1712.05318",
"language": "en",
"url": "https://arxiv.org/abs/1712.05318"
} |
\section{Introduction}
Blazars---active galaxies with relativistically beamed non-thermal broad-band emission---belong to the brightest gamma-ray sources in the sky. Their emission is notoriously variable, and their gamma-ray variability has been measured on time scales ranging from years to minutes (see \cite{mad16} ... | {
"timestamp": "2017-12-15T02:00:49",
"yymm": "1712",
"arxiv_id": "1712.04984",
"language": "en",
"url": "https://arxiv.org/abs/1712.04984"
} |
\section{Introduction}
\label{sec:intro}
The most widely used measure of correlation
is the product-moment correlation coefficient.
Its definition is quite simple. Consider a paired
sample, that is $\{(x_1,y_1),\ldots,(x_n,y_n)\}$\;
where the two numerical variables are the
column vectors
$X_n = (x_1,\ldots... | {
"timestamp": "2019-10-22T02:18:11",
"yymm": "1712",
"arxiv_id": "1712.05151",
"language": "en",
"url": "https://arxiv.org/abs/1712.05151"
} |
\section{Acknowledgement}
The author thanks Nikesh Koirala, Nuh Gedik and Liang Fu for useful discussions and the MIT for hospitality during the visit where this work was initiated.
\renewcommand{\theequation}{A-\arabic{equation}}
\renewcommand{\thesection}{S\arabic{section}}
\renewcommand{\thetable}{S\arabic{table}}... | {
"timestamp": "2018-06-12T02:10:41",
"yymm": "1712",
"arxiv_id": "1712.05140",
"language": "en",
"url": "https://arxiv.org/abs/1712.05140"
} |
\section{Introduction}
In the context of this report, Chern-Simons gravities (CSG) and gravitational Chern-Simons (GCS) densities are distinct
but not unrelated objects. They both result from the definition of Chern-Simons (CS) densities of the non-Abelian (nA) Yang-Mills (YM) fields.
The CSG consist of some superpo... | {
"timestamp": "2018-01-03T02:10:09",
"yymm": "1712",
"arxiv_id": "1712.05190",
"language": "en",
"url": "https://arxiv.org/abs/1712.05190"
} |
\section*{abstract}
Exciton diffusion length plays a vital role in the function of opto-electronic devices. Oftentimes, the domain occupied by an organic semiconductor is subject to surface measurement error. In many experiments, photoluminescence over the domain is measured and used as the observation data to estimate... | {
"timestamp": "2017-12-15T02:04:46",
"yymm": "1712",
"arxiv_id": "1712.05126",
"language": "en",
"url": "https://arxiv.org/abs/1712.05126"
} |
\section{Mapping to the extended Ising model and Exact solutions}
We start from the extended quantum Ising model with longer-range interactions in a transverse
field, with the Hamiltonian
\begin{equation}
H=\sum_{n=1}^{N_f}\sum_{j=1}^L\left(\frac{{J}_n^x}{2}\sigma_j^x\sigma_{j+n}^x\!+\frac{{J}_n^y}{2}\sigma_j^y\sigma_... | {
"timestamp": "2018-04-04T02:10:54",
"yymm": "1712",
"arxiv_id": "1712.05286",
"language": "en",
"url": "https://arxiv.org/abs/1712.05286"
} |
\section{The pentagon-wheel cocycle}
\hangindent=-6.5cm\hangafter=-3%
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\begin{picture}(0,0)(-32,2.5)
\put(65,0){$\boldsymbol{\gamma}_5 = {}$}
\put(85,0){
{\unitlength=0.3mm
\begin{picture}(55,53)(5,-5
\put(27.5,8.5){\circle*{3}}
\put(0,29.5){\circle*{3}}
\put(-27.5,8.5){\circle*{3}}
\put(-17.5,-23.75){\... | {
"timestamp": "2017-12-15T02:08:50",
"yymm": "1712",
"arxiv_id": "1712.05259",
"language": "en",
"url": "https://arxiv.org/abs/1712.05259"
} |
\section{Introduction}
\label{section1}
In this paper we consider the Arratia flow $\{x(u,\cdot),\; u\in\mbR\}$, which is an ordered family of standard Brownian motions starting from every point of the real line such that for any $u,v\in\mbR$ the joint quadratic variation of $x(u,\cdot)$ and $x(v,\cdot)$ is given... | {
"timestamp": "2017-12-15T02:03:53",
"yymm": "1712",
"arxiv_id": "1712.05098",
"language": "en",
"url": "https://arxiv.org/abs/1712.05098"
} |
\section{Introduction}
Topological Data Analysis (TDA)~\cite{carlsson,eh}, which clarifies the geometric features
of data from the viewpoint of topology, is developed rapidly in this century
both in theory and application. In TDA, persistent homology and its persistence
diagram (PD) \cite{elz,zc} are
important tool fo... | {
"timestamp": "2017-12-15T02:04:01",
"yymm": "1712",
"arxiv_id": "1712.05103",
"language": "en",
"url": "https://arxiv.org/abs/1712.05103"
} |
\section{Introduction}
\label{sec:intro}
The \emph{worst-case execution time (WCET)}
problem~\cite{WilhelmEtAl:2008,PuschnerBurns:2000} is an important
research area within the context of real-time systems. There exist
many tools and techniques for static WCET
analyis~\cite{GustafssonEtAl:2006,ColinPuaut:2000,Ferdinan... | {
"timestamp": "2017-12-15T02:08:52",
"yymm": "1712",
"arxiv_id": "1712.05264",
"language": "en",
"url": "https://arxiv.org/abs/1712.05264"
} |
\section{Introduction}\label{sec:1}
A standard option (also called plain vanilla) is a financial contract which gives the owner of the contract the right, but not the obligation, to buy or sell a specified asset to a prespecified price (strike price) at a prespecified time (maturity). The specified asset (underlying a... | {
"timestamp": "2017-12-15T02:08:44",
"yymm": "1712",
"arxiv_id": "1712.05254",
"language": "en",
"url": "https://arxiv.org/abs/1712.05254"
} |
\section{Density-Functional Theory calculations}
\label{dft}
In order to compute binding energies of CO$_2$~gas molecules, we optimize mmen-M$_2$(dobpdc) MOFs without CO$_2$~molecules (E$_{\rm{mmen-MOF}}$),
CO$_2$ in the gas phase (E$_{\rm{CO}_2}$) within a $15\AA \times 15 \AA \times 15 \AA$ cubic supercell, and
mm... | {
"timestamp": "2017-12-15T02:02:49",
"yymm": "1712",
"arxiv_id": "1712.05061",
"language": "en",
"url": "https://arxiv.org/abs/1712.05061"
} |
\section{Definitions}
\section{Introduction and preliminaries}
We will use standard set-theoretic notation following e.g. \cite{Jech}.
For a set $X$, $P(X)$ denotes the power set of $X$ and $|X|$ denotes the cardinality of $X$.
If $\kappa$ is a cardinal number then we denote:
\begin{itemize}
\item $[X]^\kappa \hspac... | {
"timestamp": "2017-12-15T02:07:29",
"yymm": "1712",
"arxiv_id": "1712.05212",
"language": "en",
"url": "https://arxiv.org/abs/1712.05212"
} |
\section{INTRODUCTION}
\IEEEPARstart{T}{o} handle soft materials, such as clothes while performing a complex task, a robot is required to not only conduct multiple subtasks properly but also to adapt to the deformation and displacement of the materials.
These subjects are very important from the scientific and prac... | {
"timestamp": "2018-07-06T02:06:56",
"yymm": "1712",
"arxiv_id": "1712.05109",
"language": "en",
"url": "https://arxiv.org/abs/1712.05109"
} |
\section{Background}
There has been extensive research on hand gesture recognition
system. \cite{Pavlovic_survey}, \cite{Mitra_survey}, \cite{Rautaray_survey} provide
execellent surveys on vision-based gesture recognition systems.
Convolutional neural networks (CNN) such as in
\cite{Molchanov_2015_CVPR_Workshops} and... | {
"timestamp": "2017-12-15T02:00:28",
"yymm": "1712",
"arxiv_id": "1712.04961",
"language": "en",
"url": "https://arxiv.org/abs/1712.04961"
} |
\section{Introduction}\label{sec:intro}
Statistical process control (SPC) applies statistical methods to the monitoring and control of a process in order to detect abnormal variations of the process. One of the most popular SPC tools is the control chart, which plots a statistic that measures a feature of the proces... | {
"timestamp": "2017-12-15T02:03:08",
"yymm": "1712",
"arxiv_id": "1712.05072",
"language": "en",
"url": "https://arxiv.org/abs/1712.05072"
} |
\section{Introduction}
In the financial literature, models based on L\'evy (or $\alpha$-stable) distributions~\cite{Zolotarev86} play a prominent role, because such distributions possess heavy tails and thus allow extreme but realistic events, such as sudden jumps of market prices,
that Gaussian models fail to describ... | {
"timestamp": "2018-10-16T02:19:41",
"yymm": "1712",
"arxiv_id": "1712.04990",
"language": "en",
"url": "https://arxiv.org/abs/1712.04990"
} |
\section{Introduction}
Modern life is influenced by an immense variety of motors in all forms and sizes, driven by energy sources ranging from heat, as in a combustion engine, through chemical energy in biological motors to electrical energy in electric motors. As the miniaturization of modern devices moves towards e... | {
"timestamp": "2017-12-15T02:00:20",
"yymm": "1712",
"arxiv_id": "1712.04952",
"language": "en",
"url": "https://arxiv.org/abs/1712.04952"
} |
\section{Introduction}
Transition metal dichalcogenides (TMDs) present a promising class of nanomaterials with a direct band gap, efficient electron-light coupling, and strong Coulomb interaction
\cite{THeinz, He2014, splendiani2010emerging, arora2015excitonic,gunnar_nano}.
The latter gives rise to a variety of tightl... | {
"timestamp": "2017-12-15T02:07:37",
"yymm": "1712",
"arxiv_id": "1712.05219",
"language": "en",
"url": "https://arxiv.org/abs/1712.05219"
} |
\section{Introduction}
\label{intro}
Under CPT symmetry time-reversal-invariance violating but parity conserving
(TVPC) forces are considered as a possible source of CP-invariance violation, which is
required to account for the matter-antimatter asymmetry in the universe \cite{sakharov}.
In contrast to ef... | {
"timestamp": "2017-12-15T02:06:48",
"yymm": "1712",
"arxiv_id": "1712.05184",
"language": "en",
"url": "https://arxiv.org/abs/1712.05184"
} |
\section{Introduction}
Early-type dwarf galaxies (dEs) play a key role in understanding galaxy cluster evolution. dEs\footnote[16]{The term dE has traditionally been used to refer to dwarf elliptical galaxies, whereas we loosely use the term here to include dwarf ellipticals and dwarf lenticulars (dS0).}, the low
lumin... | {
"timestamp": "2017-12-19T02:14:11",
"yymm": "1712",
"arxiv_id": "1712.04953",
"language": "en",
"url": "https://arxiv.org/abs/1712.04953"
} |
\section{Background}
\subsection{Paired Comparison Experiments and the Bradley-Terry Model}
A paired comparison experiment is a set of binary comparisons between
pairs out of a set of $t$ objects. The Bradley-Terry model
\citep{Zermelo1929,BRADLEY01121952} assigns to each object $i$
($i=1,\ldots t$) a strength param... | {
"timestamp": "2017-12-15T02:09:47",
"yymm": "1712",
"arxiv_id": "1712.05311",
"language": "en",
"url": "https://arxiv.org/abs/1712.05311"
} |
\section{Introduction}
In recent years and after the standardization of coherent optical transmission systems, phase modulation formats have been widely investigated \cite{Karlsson2009,Kojima2017}. Different studies concluded that designing high-dimensional modulation formats can increase the product of reach and capac... | {
"timestamp": "2017-12-15T02:05:28",
"yymm": "1712",
"arxiv_id": "1712.05141",
"language": "en",
"url": "https://arxiv.org/abs/1712.05141"
} |
\section{Introduction}
\label{Sec-1:introduction}
The matrix elements of the energy-momentum tensor (EMT) \cite{Pagels}
provide most basic information: the mass and spin of a particle.
They also define the $D$-term \cite{Polyakov:1999gs},
a property not known experimentally for any particle.
The most direct way to ... | {
"timestamp": "2017-12-15T02:09:52",
"yymm": "1712",
"arxiv_id": "1712.05317",
"language": "en",
"url": "https://arxiv.org/abs/1712.05317"
} |
\section{Introduction}
An \emph{intersection graph} of geometric objects has one vertex per object and an edge between every pair of vertices corresponding to intersecting objects.
Intersection graphs for many different families of geometric objects have been studied due to their practical applications and rich struct... | {
"timestamp": "2018-03-01T02:11:53",
"yymm": "1712",
"arxiv_id": "1712.05010",
"language": "en",
"url": "https://arxiv.org/abs/1712.05010"
} |
\section{Introduction}
Automatic music generation using neural networks has attracted much attention.
There are two classes of music generation approaches, symbolic music generation~\cite{hadjeres2016deepbach}\cite{magenta2016}\cite{yang2017midinet} and audio music generation~\cite{oord2016wavenet}\cite{mehri2016sampl... | {
"timestamp": "2018-09-06T02:05:57",
"yymm": "1712",
"arxiv_id": "1712.05274",
"language": "en",
"url": "https://arxiv.org/abs/1712.05274"
} |
\section{Introduction}
Maritime transportation has significant benefits in terms of cost and
capability for carrying a higher number of cargos. Indeed, sea trade
statistics indicate that 90\% of global trade is performed by maritime
transportation. This has led to new investments in container terminals
and a variety o... | {
"timestamp": "2017-12-15T02:09:42",
"yymm": "1712",
"arxiv_id": "1712.05302",
"language": "en",
"url": "https://arxiv.org/abs/1712.05302"
} |
\section{Introduction}
Following the discovery of a Higgs boson with a mass of 125 GeV \cite{atlas,cms}, henceforth
labeled by $H$, with characteristics similar to those of the predicted state
of the Standard Model (SM), experiments at the LHC have effectively begun to
probe Electro-Weak Symmetry Breaking (EWSB) dynam... | {
"timestamp": "2017-12-25T02:09:03",
"yymm": "1712",
"arxiv_id": "1712.05332",
"language": "en",
"url": "https://arxiv.org/abs/1712.05332"
} |
\section{Introduction}
The nitrogen-vacancy (NV) center in diamond is currently one of the most studied and anticipated platforms for high spatial-resolution sensing of magnetic fields \cite{Balasubramanian2008,Rondin2014,Schirhagl2014}, electric fields \cite{Dolde2011} and temperature \cite{Kucsko2013,Neumann2013} at ... | {
"timestamp": "2017-12-15T02:06:16",
"yymm": "1712",
"arxiv_id": "1712.05161",
"language": "en",
"url": "https://arxiv.org/abs/1712.05161"
} |
\section{INTRODUCTION}
\label{sec:intro}
The kinetic Sunyaev--Zel'dovich (kSZ) effect \citep{kSZ1980} is a powerful
probe of the physics of the epoch of reionisation (EoR), as it is sensitive
to patchiness of ionised bubbles \citep[see][and references
therein]{Park2013}. Measurements of the power spectrum of the kSZ,
h... | {
"timestamp": "2017-12-15T02:09:44",
"yymm": "1712",
"arxiv_id": "1712.05305",
"language": "en",
"url": "https://arxiv.org/abs/1712.05305"
} |
\section{Introduction}
In the past four decades, the semilinear wave equations in the following form
\begin{equation*}
\Box \varphi = Q(\partial \varphi, \partial \varphi),
\end{equation*}
have been studied intensively and have found many deep applications in geometry and physics. We assume that the field $\varphi(t,x)... | {
"timestamp": "2017-12-15T02:03:14",
"yymm": "1712",
"arxiv_id": "1712.05076",
"language": "en",
"url": "https://arxiv.org/abs/1712.05076"
} |
\section{Introduction}
Many $C^*$-algebras can be modeled as groupoid $C^*$-algebras (see e.g. \cite{Renault}), which allows the use of the additional structural information to answer general questions in the theory of $C^*$-algebras. For example, J. L. Tu showed in \cite{Tu} that groupoids which satisfy the Haageru... | {
"timestamp": "2018-03-14T01:02:12",
"yymm": "1712",
"arxiv_id": "1712.05237",
"language": "en",
"url": "https://arxiv.org/abs/1712.05237"
} |
\section{\label{sec:introduction} Introduction}
The dawn of the multi-messenger astronomy has been one of the most great achievements in the scientific community in the last decade. Combining neutrino observations with measurements of cosmic rays, electromagnetic radiation and gravitational wave will be crucial to so... | {
"timestamp": "2017-12-15T02:00:46",
"yymm": "1712",
"arxiv_id": "1712.04979",
"language": "en",
"url": "https://arxiv.org/abs/1712.04979"
} |
\section{Introduction}
\label{sIntro}
The present paper concerns the relationship between sum-and-distance systems
and sum systems, and their general structure, including a construction method
for all such systems. Roughly speaking, a sum-and-distance system consists of
several component sets of natural numbers such th... | {
"timestamp": "2017-12-15T02:07:03",
"yymm": "1712",
"arxiv_id": "1712.05195",
"language": "en",
"url": "https://arxiv.org/abs/1712.05195"
} |
\section{Introduction}
Given a convex polygon $P$ with $n$ edges, the \emph{minimum all-flush $k$-gon problem} asks for the minimum (with respect to area throughout this paper) $k$-gon
whose edges are all flushed with edges of $P$ (i.e. each edge must contain an edge of $P$ as a subregion).
In other words, it asks f... | {
"timestamp": "2018-07-17T02:11:17",
"yymm": "1712",
"arxiv_id": "1712.05081",
"language": "en",
"url": "https://arxiv.org/abs/1712.05081"
} |
\subsubsection{\@startsection{subsubsection
{3
{\z@
{0ex plus 0.1ex minus 0.1ex
{0ex
{\normalfont\normalsize\itshape}
\makeatother
\usepackage[T1]{fontenc... | {
"timestamp": "2017-12-15T02:00:46",
"yymm": "1712",
"arxiv_id": "1712.04980",
"language": "en",
"url": "https://arxiv.org/abs/1712.04980"
} |
\section*{$T_5$ and $K_{2,4}$ are SPN}
We begin by recalling some known results about the matrices
\[S(\btheta)=\left(\begin {array}{ccccc} 1&-\cos({\theta_1})&\cos({\theta_1+\theta_2})&\cos({\theta_4+\theta_5})&-\cos({\theta_5})\\
\noalign{\medskip}-\cos({\theta_1})&1&-\cos({\theta_2})&\cos({\theta_2+\theta_3})&\co... | {
"timestamp": "2017-12-15T02:04:30",
"yymm": "1712",
"arxiv_id": "1712.05115",
"language": "en",
"url": "https://arxiv.org/abs/1712.05115"
} |
\section{Introduction}
\label{sec:intro}
Unwanted quasiparticle excitations can degrade the performance of superconducting devices. For example, they can be a limiting factor for superconducting detectors used in astronomy~\cite{Day}, and a source of errors in superconductor-based charge pumps used for metrology~\cite... | {
"timestamp": "2017-12-25T02:05:48",
"yymm": "1712",
"arxiv_id": "1712.05235",
"language": "en",
"url": "https://arxiv.org/abs/1712.05235"
} |
\section{Introduction}
\IEEEPARstart{D}{ecoherence} in superconducting qubits can be caused by dielectric loss generated on many surfaces in and around the environment of the qubit. For example, contamination layers and native oxides present on semiconductor and metallization surfaces will exhibit participation based... | {
"timestamp": "2018-06-19T02:13:42",
"yymm": "1712",
"arxiv_id": "1712.05079",
"language": "en",
"url": "https://arxiv.org/abs/1712.05079"
} |
\section{Introduction and motivation}
The purpose of this paper is to study general relativistic effects of space-time curvature on fermionic spins, via an analog
gravity black hole setup in the context of superfluid $\text{He}^3$-A. In particular, we will focus on such relativistic effects on
fermionic quasiparticle... | {
"timestamp": "2017-12-20T02:08:20",
"yymm": "1712",
"arxiv_id": "1712.05230",
"language": "en",
"url": "https://arxiv.org/abs/1712.05230"
} |
\section{Introduction}
Effective interactions between nano-/macromolecular bodies in aqueous solutions can broadly be decomposed into two equally important contributions: The static or equilibrium forces, and the dynamic forces, arising when the system is driven out of equilibrium, such as when the bodies are in relat... | {
"timestamp": "2018-07-03T02:04:09",
"yymm": "1712",
"arxiv_id": "1712.05051",
"language": "en",
"url": "https://arxiv.org/abs/1712.05051"
} |
\section{Introduction}
The neutrino-plasma coupling in magnetized media is a relevant issue in diverse situations, as near the core of proto-neutron stars, where it is a source of the free energy behind the stalled supernova shock \cite{Bludman}--\cite{Bethe2}.
Neutrino-driven wakefields and neutrino effective charge... | {
"timestamp": "2017-12-15T02:10:24",
"yymm": "1712",
"arxiv_id": "1712.05328",
"language": "en",
"url": "https://arxiv.org/abs/1712.05328"
} |
\section*{Abstract}
We seek models for the genotype evolution of agricultural animals,
animals involved in primary production processes. Classical models
for genotype evolution have tended to be very simple in order that
analytic methods may be employed in their study. Unfortunately
these models fail to describe p... | {
"timestamp": "2017-12-15T02:06:40",
"yymm": "1712",
"arxiv_id": "1712.05177",
"language": "en",
"url": "https://arxiv.org/abs/1712.05177"
} |
\section{Introduction}
\label{Introduction}
SrRuO$_3$ (SRO) is a ferromagnetic metal oxide with a Curie temperature $T_c$ of 160 K \cite{j1}. It is often used as a gate electrode due to its high conductivity and ease of epitaxial growth \cite{j2}. SRO has attracted considerable attention because of its intriguing elec... | {
"timestamp": "2017-12-15T02:05:25",
"yymm": "1712",
"arxiv_id": "1712.05137",
"language": "en",
"url": "https://arxiv.org/abs/1712.05137"
} |
\section{Introduction}\label{sec1}
Gamma-ray bursts (GRBs) are traditionally classified in short GRBs, with a total duration $\lesssim 2$~s, and long GRBs, lasting $\gtrsim 2$~s \citep{1981Ap&SS..80....3M,Dezalay1992,Klebesadel1992,Kouveliotou1993,Tavani1998}. Large majority of long bursts is spatially correlated wi... | {
"timestamp": "2018-11-06T02:22:30",
"yymm": "1712",
"arxiv_id": "1712.05001",
"language": "en",
"url": "https://arxiv.org/abs/1712.05001"
} |
\section{Introduction}
Autonomous robot navigation has a broad spectrum of applications, ranging from search and rescue to transportation. Typical approaches to introduce autonomy rely on heuristics or require a predefined set of manually specified rules. Alternative solutions based on machine learning generally requir... | {
"timestamp": "2017-12-15T02:03:28",
"yymm": "1712",
"arxiv_id": "1712.05084",
"language": "en",
"url": "https://arxiv.org/abs/1712.05084"
} |
\section{Introduction}
Association rule mining (ARM) has emerged as a powerful and specialized tool to identify patterns in large datasets. It can be used in applications or business operations where instances of some spatio-temporal occurrence is represented in tabular format across a set of common attributes. An ARM... | {
"timestamp": "2017-12-15T02:06:59",
"yymm": "1712",
"arxiv_id": "1712.05193",
"language": "en",
"url": "https://arxiv.org/abs/1712.05193"
} |
\section{Experimental Setup}
Our qubit is encoded in the $^2\mathrm{S}_{1/2}$ hyperfine ground states of a single laser-cooled ${}^{171}{\textrm{Yb}}^{+}$ ion confined in a linear Paul trap, with the computational basis states defined as $\ket{0} \equiv \ket{\textrm{F}=0, \textrm{m}_\textrm{F} = 0}$ and $\ket{1} \eq... | {
"timestamp": "2017-12-15T02:00:22",
"yymm": "1712",
"arxiv_id": "1712.04954",
"language": "en",
"url": "https://arxiv.org/abs/1712.04954"
} |
\section{Ehrenfest equations of motion}
Denoting by ${\bf n}_i(\Omega)$ the $i$-th principal axis of the rotor so that ${\bf n}_k(\Omega) \cdot \mathrm{I}(\Omega) {\bf n}_j(\Omega) = I_k \delta_{kj}$, the components of the angular momentum operator in the body fixed frame are given by $\widetilde{\op{J}}_k = {\bf n}_k... | {
"timestamp": "2018-07-27T02:07:44",
"yymm": "1712",
"arxiv_id": "1712.05163",
"language": "en",
"url": "https://arxiv.org/abs/1712.05163"
} |
\section{Introduction}
The Magellanic Clouds have significantly advanced our understanding on galaxy evolution. Owing to their proximity, individual stars can be observed, providing important information about the spatially resolved star formation, and the origin and properties of their stellar populations.
The Small... | {
"timestamp": "2017-12-15T02:00:42",
"yymm": "1712",
"arxiv_id": "1712.04974",
"language": "en",
"url": "https://arxiv.org/abs/1712.04974"
} |
\section{Methods}
\textbf{Experimental procedure.} To perform our experiments we prepare a Bose-Einstein condensate of $\approx\num{80e3}$ $^{87}\mathrm{Rb}$ atoms, spin polarized in the $\ket{5\mathrm{S}_{1/2}, F=2, m_F=2}$ state, in a crossed optical dipole trap with trapping frequencies $\omega_{x,y,z} = 2\pi\times(... | {
"timestamp": "2017-12-15T02:08:52",
"yymm": "1712",
"arxiv_id": "1712.05263",
"language": "en",
"url": "https://arxiv.org/abs/1712.05263"
} |
\section{Introduction}
Flavor-changing neutral current (FCNC) processes are sensitive probes for new physics beyond the Standard Model (SM), since in the SM there are no FCNC processes at the tree level, and they are suppressed further by the Glashow-Iliopoulos-Maiani (GIM) mechanism. One of the FCNC observables, the ... | {
"timestamp": "2018-04-04T02:09:13",
"yymm": "1712",
"arxiv_id": "1712.04959",
"language": "en",
"url": "https://arxiv.org/abs/1712.04959"
} |
\section{Introduction}
\label{sec_1}
In this work we deal with categorical (ordinal) variables collected in a contingency table and we propose a model able to capture different kind of independence relationships involving ordinal variables. Different models have been proposed in the literature with the aim of describi... | {
"timestamp": "2017-12-25T02:07:49",
"yymm": "1712",
"arxiv_id": "1712.05229",
"language": "en",
"url": "https://arxiv.org/abs/1712.05229"
} |
\section{Introduction}
In recent years there has been a great interest in the construction of discrete dynamical systems with given properties (see for example \cite{bib:eich93,bib:EHHW98,bib:HBM17,bib:ost10,bib:OPS10,bib:OS10degree,bib:OS10length}) both for applications (see for example \cite{bib:BW05,bib:chou95,bib:... | {
"timestamp": "2018-09-12T02:02:12",
"yymm": "1712",
"arxiv_id": "1712.05258",
"language": "en",
"url": "https://arxiv.org/abs/1712.05258"
} |
\section{Introduction}
The enhancement seen in atomic hyperfine structure experiments for electric quadrupole (E2) moments \cite{sc35} over predictions for a configuration formed by only one or a few single particle orbitals has triggered intensive research on its consequences for nuclear structure: Besides the pressur... | {
"timestamp": "2017-12-15T02:01:08",
"yymm": "1712",
"arxiv_id": "1712.04999",
"language": "en",
"url": "https://arxiv.org/abs/1712.04999"
} |
\section{Introduction}\label{sec:intro}
The connections that have been uncovered between gravity and thermodynamics -- with the fundamental intervention of quantum effects -- have been widely regarded as clues leading to a long-sought theory of quantum gravity. In the work \cite{ACQUAVIVA2017317} we propose a new pi... | {
"timestamp": "2017-12-15T02:09:04",
"yymm": "1712",
"arxiv_id": "1712.05275",
"language": "en",
"url": "https://arxiv.org/abs/1712.05275"
} |
\section{Introduction}
An unbiased line survey is an effective method in understanding chemical compositions as well as excitation conditions in the ISM. So far, many line survey observations toward characteristic sources in our Galaxy have been carried out using radio telescopes. For example, line surveys toward mass... | {
"timestamp": "2017-12-15T02:03:04",
"yymm": "1712",
"arxiv_id": "1712.05070",
"language": "en",
"url": "https://arxiv.org/abs/1712.05070"
} |
\section{Introduction}
In \cite{Luo}, we proved the following theorem:
\begin{thm}[\cite{Luo}]
Let $L:\Sigma\to \mathbb{S}^5$ be a contact stationary Legendrian surface. Then we have
\begin{eqnarray*}
\int_L\rho^2(3-\frac{3}{2}S+2H^2)d\mu\leq0,
\end{eqnarray*}
where $\rho^2:=S-2H^2$. In particular, if
\beg... | {
"timestamp": "2019-11-26T02:22:36",
"yymm": "1712",
"arxiv_id": "1712.05100",
"language": "en",
"url": "https://arxiv.org/abs/1712.05100"
} |
\section{Introduction}
Nuclear fusion reactors need to be heated to very high temperature to overcome the Coulomb repulsion between nuclei to fuse.
\cite{McCracken}. (Mathematically it is manifested in the exponential energy
dependent factor in the cross section of fusion reactions [see $\left( \re
{sigma}\right)... | {
"timestamp": "2018-01-16T02:12:28",
"yymm": "1712",
"arxiv_id": "1712.05270",
"language": "en",
"url": "https://arxiv.org/abs/1712.05270"
} |
\section{Introduction}
\IEEEPARstart{T}{his} demo file is intended to serve as a ``starter file''
for IEEE journal papers produced under \LaTeX\ using
IEEEtran.cls version 1.8b and later.
I wish you the best of success.
\hfill mds
\hfill August 26, 2015
\subsection{Subsection Heading Here}
Subsection text here.
\... | {
"timestamp": "2017-12-15T02:07:13",
"yymm": "1712",
"arxiv_id": "1712.05200",
"language": "en",
"url": "https://arxiv.org/abs/1712.05200"
} |
\section{INTRODUCTION}
Dark matter (DM) has been discovered through its
gravitational interaction with usual matter. DM particles have been
and are still searched in various processes at the high energy colliders.
For a recent review with many references see \cite{rev1}.\\
Many (hundreds of) models have been propose... | {
"timestamp": "2017-12-15T02:10:54",
"yymm": "1712",
"arxiv_id": "1712.05352",
"language": "en",
"url": "https://arxiv.org/abs/1712.05352"
} |
\section{Characteristic kernels on spaces with additional structure}\label{sec:structure}
In this section, we apply the developed theory to translation-invariant or isotropic kernels on compact Abelian groups or
spheres, respectively.
\input{compact-groups}
\subsection{Spheres}\label{sec:Sd}
In this ... | {
"timestamp": "2017-12-15T02:09:13",
"yymm": "1712",
"arxiv_id": "1712.05279",
"language": "en",
"url": "https://arxiv.org/abs/1712.05279"
} |
\section{Introduction}
Precise segmentation of infant brain MRI into white matter (WM), gray matter (GM) and cerebrospinal fluid (CSF) is essential to study early brain development. Throughout this period, the postnatal human brain shows its most dynamic phase of development, with a rapid growth of tissues and the for... | {
"timestamp": "2017-12-20T02:10:30",
"yymm": "1712",
"arxiv_id": "1712.05319",
"language": "en",
"url": "https://arxiv.org/abs/1712.05319"
} |
\section{Introduction}
The key notion of this paper, the \emph{comparison} originates in the theory of \mbox{$C^*$-al}geb\-ras, but the most important for us ``dynamical'' version concerns group actions on compact spaces. In this setup it was defined by J.~Cuntz (see \cite{Cu}) and further investigated by M.~R\o rdam i... | {
"timestamp": "2017-12-15T02:05:02",
"yymm": "1712",
"arxiv_id": "1712.05129",
"language": "en",
"url": "https://arxiv.org/abs/1712.05129"
} |
\section{Introduction}
\dropcap{C}ell motility is an integral part of biological processes such as morphogenesis \cite{Friedl2004}, wound healing \cite{Bindschadler2007} , and cancer invasion \cite{Kraning-Rush2013}. But what are the rules that govern how cells move? Cell migration involves a multitude of organelles a... | {
"timestamp": "2017-12-15T02:02:25",
"yymm": "1712",
"arxiv_id": "1712.05049",
"language": "en",
"url": "https://arxiv.org/abs/1712.05049"
} |
\section{Introduction}
As much as one would welcome the production of a light charged Higgs boson from top-quark decay at the LHC, as
the event rate would be plentiful, it must be recognised by now that the likelihood of this being a design of Nature is becoming slimmer and slimmer. This is because extensive searches ... | {
"timestamp": "2017-12-15T02:01:49",
"yymm": "1712",
"arxiv_id": "1712.05018",
"language": "en",
"url": "https://arxiv.org/abs/1712.05018"
} |
\section{Introduction}
Quasars are among the most luminous objects in the observable universe associated with rapidly accreting supermassive black holes. We classify AGN depending on how the AGN is viewed – whether the detected radiation allows us to „see” the nucleus directly (Type-1 AGNs); or the radiation is partia... | {
"timestamp": "2017-12-15T02:06:36",
"yymm": "1712",
"arxiv_id": "1712.05176",
"language": "en",
"url": "https://arxiv.org/abs/1712.05176"
} |
\section{Introduction}
After the discovery of the Higgs boson particle at LHC in 2012~\cite{Htn,Htn1},
many improved measurements confirmed the consistence of its quantum numbers and couplings
with the Standard Model (SM) predictions, including the loop-induced coupling
$h\gamma\gamma$~\cite{Khachatryan:2016vau,HiggsE... | {
"timestamp": "2018-11-06T02:22:09",
"yymm": "1712",
"arxiv_id": "1712.05234",
"language": "en",
"url": "https://arxiv.org/abs/1712.05234"
} |
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