text stringlengths 1 2.26M | meta dict |
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\section{Introduction}
Radio emission from solar flares can be detected from millimeter to
kilometer wavelengths. Flare microwave emission can provide
important diagnostics of acceleration processes in the corona because
the radio emission is produced by energetic electrons accelerated
during the flare. The mic... | {
"timestamp": "2010-09-21T02:01:48",
"yymm": "1009",
"arxiv_id": "1009.3654",
"language": "en",
"url": "https://arxiv.org/abs/1009.3654"
} |
{
"timestamp": "2010-09-23T02:01:24",
"yymm": "1009",
"arxiv_id": "1009.4303",
"language": "en",
"url": "https://arxiv.org/abs/1009.4303"
} | |
\section{Introduction}
\label{intro}
Chiral effective field theory (EFT) as proposed in the pioneering works of
Weinberg \cite{Wei90} is a powerful tool for the derivation of nuclear forces.
In this scheme there is an underlying power counting which allows to improve calculations
systematically by going to higher o... | {
"timestamp": "2010-09-23T02:01:35",
"yymm": "1009",
"arxiv_id": "1009.4319",
"language": "en",
"url": "https://arxiv.org/abs/1009.4319"
} |
\section{Introduction}
Mathematically, the simplest models of the Universe are those which
possess a high degree of symmetry. Spacelike slices of the
Friedmann-Robertson-Walker (FRW) solutions possess the maximal six
Killing vector fields (KVFs), reducing the number of degrees of
freedom to just one, the curvature rad... | {
"timestamp": "2010-09-22T02:00:22",
"yymm": "1009",
"arxiv_id": "1009.3935",
"language": "en",
"url": "https://arxiv.org/abs/1009.3935"
} |
\section{Introduction}
In this article, we study local zeta functions for non-degenerate Laurent
polynomials (in two variables) with respect to its Newton polytope at infinity
over $p$-adic fields. By using toroidal compactifications, we show the
existence of a meromorphic continuation for these zeta functions as... | {
"timestamp": "2012-08-20T02:02:26",
"yymm": "1009",
"arxiv_id": "1009.3680",
"language": "en",
"url": "https://arxiv.org/abs/1009.3680"
} |
\section{Introduction}
\label{sec:intro}
Is there a positive constant $C$ such that every $C$-connected graph
is hamiltonian? Certainly not, as shown by the complete bipartite
graphs $K_{n,n+1}$, where $n$ is large. The situation may change,
however, if the problem is restricted to graphs not containing a
speci... | {
"timestamp": "2011-04-01T02:03:09",
"yymm": "1009",
"arxiv_id": "1009.3754",
"language": "en",
"url": "https://arxiv.org/abs/1009.3754"
} |
\section{Introduction}\label{int}
Let $X$ be a compact connected Riemann surface of genus
$g$, with $g\,\geq\, 2$. Let ${\mathcal M}_\eta(2)$ denote
the moduli space of stable vector bundles $E$ over $X$
of rank two with $\bigwedge^2 E\,=\, \eta$, where $\eta\,
\longrightarrow\, X$ is a fixed holomorphic line bundle o... | {
"timestamp": "2010-09-22T02:01:09",
"yymm": "1009",
"arxiv_id": "1009.4009",
"language": "en",
"url": "https://arxiv.org/abs/1009.4009"
} |
\section{Introduction}
X-ray observations of accreting neutron stars and black holes
necessarily probe regions close to the compact object. The long--held
promise of these observations is that aspects of the compact object
itself, and the innermost accretion flow, may be revealed. Notable
early attempts to realize t... | {
"timestamp": "2010-09-23T02:02:23",
"yymm": "1009",
"arxiv_id": "1009.4391",
"language": "en",
"url": "https://arxiv.org/abs/1009.4391"
} |
\section{Introduction}
To any locally finite subset ${\mathcal N}$ of $\bR^d$ one can associate a
partition of the plane as follows. To each point ${\mathbf v}\in {\mathcal N}$
corresponds a polygonal region $C_{\mathbf v}$, the \emph{Voronoi tile} at ${\mathbf v}$, consisting of the set of points of $\bR^d$ which are
... | {
"timestamp": "2011-08-15T02:02:50",
"yymm": "1009",
"arxiv_id": "1009.3898",
"language": "en",
"url": "https://arxiv.org/abs/1009.3898"
} |
\section{#1} \setcounter{equation}{0} }
\newcommand{\Aslash}{A \! \! \! /}
\newcommand{\Dslash}{D \! \! \! \! /}
\newcommand{\kslash}{k \! \! \! /}
\newcommand{\pslash}{p \! \! \! /}
\newcommand{\xslash}{x \! \! \! /}
\newcommand{\partialslash}{\partial \! \! \! /}
\newcommand{\half}{\mbox{\small{$\frac{1}{2}$}... | {
"timestamp": "2010-09-21T02:04:01",
"yymm": "1009",
"arxiv_id": "1009.3889",
"language": "en",
"url": "https://arxiv.org/abs/1009.3889"
} |
\section{Introduction}
An outstanding problem in stellar astrophysics concerns
the identification of physical processes responsible for the heating
of outer stellar atmospheres and the acceleration of stellar winds
(see reviews by \citealt{nara90,nara96} and \citealt{gued07}).
For the Sun and other types of star... | {
"timestamp": "2010-09-22T02:03:08",
"yymm": "1009",
"arxiv_id": "1009.4174",
"language": "en",
"url": "https://arxiv.org/abs/1009.4174"
} |
\section{Introduction}\label{sec:intro}
To tile means to cover a given part of space, without overlaps, using a small
number, often just one, of different types of objects. When we are covering the
floor of a room using identical rectangular tiles (in the ordinary sense of the
word) we put down the copies of the tiles... | {
"timestamp": "2010-09-21T02:03:11",
"yymm": "1009",
"arxiv_id": "1009.3799",
"language": "en",
"url": "https://arxiv.org/abs/1009.3799"
} |
\section{Phase in the Fourier Plane}
Only two parameters essentially determine whether a source is
detectable during an observation: its brightness at the wavelength
$\lambda$ of interest and the angular resolution necessary to separate
the source or feature from its direct environment.
The angular resolution is ultim... | {
"timestamp": "2010-09-22T02:00:21",
"yymm": "1009",
"arxiv_id": "1009.3933",
"language": "en",
"url": "https://arxiv.org/abs/1009.3933"
} |
\section{Introduction}
Throughout the history of Lie theory there has been a notion of ``local isomorphism". Indeed, the original notion of Lie groups considered by
Sophus Lie in \cite{LieEngel1888} was an essentially local one. Suppose that $G$ is an algebraic group defined over a Hausdorff topological field $k$.... | {
"timestamp": "2012-07-24T02:06:25",
"yymm": "1009",
"arxiv_id": "1009.4249",
"language": "en",
"url": "https://arxiv.org/abs/1009.4249"
} |
\section{Introduction} \label{introduction}
In the past 15 years it has been extensively studied (see for example \cite{Moffat:1994qy,Mustapha:1998jb, Tomita:1999qn, Celerier:1999hp, Iguchi:2001sq, Alnes:2005rw, Chung:2006xh, Enqvist:2006cg, Tanimoto:2007dq, Alexander:2007xx, GarciaBellido:2008nz, Clifton:2008hv, Yoo... | {
"timestamp": "2010-12-10T02:02:30",
"yymm": "1009",
"arxiv_id": "1009.4193",
"language": "en",
"url": "https://arxiv.org/abs/1009.4193"
} |
\section{Introduction}
The pseudo-differential operator (p.d.o.) $h_{\mu,a}$ have applications in the study of boundary value problems on the half line. The p.d.o. $h_{\mu,a}$ was introduced by {\cite{pp}}, and its properties were investigated using Zemanian's theory of the Hankel transformation to certain space of Ul... | {
"timestamp": "2010-09-22T02:01:45",
"yymm": "1009",
"arxiv_id": "1009.4060",
"language": "en",
"url": "https://arxiv.org/abs/1009.4060"
} |
\section{Introduction}
Strong observational evidence supports the idea that the inner Solar
system is subject to a steady flux of `new' comets which originate
from the `Oort cloud' \citep{Oort50}. The semi-major axes of these
comets are thought to evolve under the influence of external forces
such as the Galact... | {
"timestamp": "2010-09-23T02:00:12",
"yymm": "1009",
"arxiv_id": "1009.4190",
"language": "en",
"url": "https://arxiv.org/abs/1009.4190"
} |
\section{Introduction}
Solitons describe a class of fascinating
nonlinear wave propagation phenomena appearing as a result of
balance between nonlinearity and dispersion or diffraction
properties of the medium under nonlinear excitations, which leads
to undistorted propagation over extended distance \cite{Haus}. One o... | {
"timestamp": "2010-09-21T02:02:26",
"yymm": "1009",
"arxiv_id": "1009.3727",
"language": "en",
"url": "https://arxiv.org/abs/1009.3727"
} |
\section{Introduction}
Recently, \citet{Fryer2010} have presented arguments in favour of
type~Ia supernova (SN) explosions taking place within rather dense
extended C--O envelopes formed during a merging process in Double Degenerate (DD) scenario.
They obtained light curves which are very powerful in hard spectral ran... | {
"timestamp": "2010-10-06T02:03:10",
"yymm": "1009",
"arxiv_id": "1009.4353",
"language": "en",
"url": "https://arxiv.org/abs/1009.4353"
} |
\section{Introduction}
``Sparse'' classification or regression problems, which involve
an $\ell_{1}-\text{norm}$ regularization has attracted a lot of interest
in the statistics~\citep{tibshirani1996regression}, signal processing~\citep{chen2001atomic},
and machine learning communities. The $\ell_{1}$ regularization l... | {
"timestamp": "2011-05-19T02:03:55",
"yymm": "1009",
"arxiv_id": "1009.4219",
"language": "en",
"url": "https://arxiv.org/abs/1009.4219"
} |
\section*{Introduction}
Let $X$ be a smooth compact manifold with non-empty boundary $\pa X$. Assume that $\pa X$ is the total space of a smooth fibration
\begin{equation*}
\xymatrix{
Z \ar@{-}[r] & \pa X \ar[d]^{\Phi} \\
& Y
... | {
"timestamp": "2011-12-21T02:01:56",
"yymm": "1009",
"arxiv_id": "1009.4272",
"language": "en",
"url": "https://arxiv.org/abs/1009.4272"
} |
\section{Introduction}
The peculiarity of a condensate arises from its macroscopic occupation.
The order of magnitude of the typical quantum fluctuations is $\ord{\hbar^{1/2}}$
in a trivial, perturbative vacuum. When a condensate is present then the field
is supposed to display an $\hbar$-independent, $\ord{\hbar^0}$ ... | {
"timestamp": "2010-09-21T02:01:45",
"yymm": "1009",
"arxiv_id": "1009.3652",
"language": "en",
"url": "https://arxiv.org/abs/1009.3652"
} |
\section{Introduction}
An important issue in wireless random-access networks is how to deal
with the collisions caused by simultaneous packet transmissions.
Multiuser detection (MUD), first proposed by Verdu in the 1980s, is
the traditional method to solve this problem. However, this method
relies heavily on the cross... | {
"timestamp": "2010-09-22T02:01:40",
"yymm": "1009",
"arxiv_id": "1009.4046",
"language": "en",
"url": "https://arxiv.org/abs/1009.4046"
} |
\section{Introduction}
Many high energy astrophysical phenomena, including accretion flows, jet
flows, gamma-ray bursts, and pulsar winds involve relativistic flows.
In powerful extragalactic radio sources, for example, ejections from
galactic nuclei produce intrinsic beam Lorentz factors of usually more than $5$
and ... | {
"timestamp": "2010-09-21T02:02:54",
"yymm": "1009",
"arxiv_id": "1009.3774",
"language": "en",
"url": "https://arxiv.org/abs/1009.3774"
} |
\section{%
\@startsection
{section}%
{1}%
{\z@}%
{0.8cm \@plus1ex \@minus .2ex}%
{0.5cm}%
{%
\normalfont\small\bfseries
\centering
}%
}%
\def\@hangfrom@section#1#2#3{\@hangfrom{#1#2}\MakeTextUppercase{#3}}%
\def\subsection{%
\@startsection
{subsection}%
{2}%
{\z@... | {
"timestamp": "2010-09-24T02:00:15",
"yymm": "1009",
"arxiv_id": "1009.4461",
"language": "en",
"url": "https://arxiv.org/abs/1009.4461"
} |
\section{Introduction}
In physics it is sometimes useful to decompose a multi--component variable/quantity
with respect to a pair of orthogonal subspaces spanning its range. Examples relevant for
the area of application that we target here, namely QCD and its vacuum structure, include
the decomposition of a bispino... | {
"timestamp": "2011-08-05T02:03:50",
"yymm": "1009",
"arxiv_id": "1009.4451",
"language": "en",
"url": "https://arxiv.org/abs/1009.4451"
} |
\section{Introduction}\label{s:intro}
One of the main tools for studying piecewise-linear manifolds is the
notion of triangulation, or more generally, cell complexes formed by
convex cells. However, for many purposes this is too restrictive. For
example, for any explicit computation of state-sum invariants of
3-man... | {
"timestamp": "2011-11-08T02:07:59",
"yymm": "1009",
"arxiv_id": "1009.4227",
"language": "en",
"url": "https://arxiv.org/abs/1009.4227"
} |
\section{Introduction}
Entanglement is believed to be an important resource in quantum information
processing and consequently many works are devoted to its characterization
\cite{hororeview,gtreview}. This characterization becomes complicated, if more
than two particles are entangled, since then different classes ... | {
"timestamp": "2011-01-04T02:03:23",
"yymm": "1009",
"arxiv_id": "1009.3782",
"language": "en",
"url": "https://arxiv.org/abs/1009.3782"
} |
\section{The model}
To study the basic effects of internal stress generated by molecular motors on the macroscopic mechanical properties of stiff polymer networks we employ a minimalistic model, which is illustrated in Fig.~\ref{fig:network}. Filamentous networks in 2D are generated by arranging filaments spanning th... | {
"timestamp": "2010-09-21T02:03:38",
"yymm": "1009",
"arxiv_id": "1009.3848",
"language": "en",
"url": "https://arxiv.org/abs/1009.3848"
} |
\section{Introduction}
The non-messing-up property of matrices is a well-known result about sorting the entries in a matrix. It appears in work by Boerner \cite{boerner}, Gale and Karp \cite{gale-karp}, Knuth \cite{knuth}, and Winkler \cite{winkler}, and a detailed discussion of its provenance occurs in \cite{nmut}. ... | {
"timestamp": "2010-09-23T02:00:17",
"yymm": "1009",
"arxiv_id": "1009.4201",
"language": "en",
"url": "https://arxiv.org/abs/1009.4201"
} |
\section{Introduction}
Small-scale turbulence plays a crucial role in cosmic magnetism, providing the small-scale (turbulent)
MHD-dynamo and contributing a lot to the dynamics of large-scale magnetic fields.
The mean field (large-scale) dynamo equations are derived by applying the
Reynolds approach to the magne... | {
"timestamp": "2010-09-23T02:01:46",
"yymm": "1009",
"arxiv_id": "1009.4333",
"language": "en",
"url": "https://arxiv.org/abs/1009.4333"
} |
\section{Introduction}
\setcounter{equation}{0}
\vspace*{-1mm}
Sylvester~\cite{Sylvester} initiated
the study of subposets of the
partition lattice.
He proved that the M\"obius function of
the poset of set partitions
where each block has even cardinality is given
by every other Euler number, also known as the tang... | {
"timestamp": "2010-09-22T02:00:46",
"yymm": "1009",
"arxiv_id": "1009.3976",
"language": "en",
"url": "https://arxiv.org/abs/1009.3976"
} |
\chapter[Abstract]{\huge Abstract}
We employ the theoretical framework of positive operator valued measures, to study Markovian open quantum systems. In particular, we discuss how a quantum system influences its environment, or parts thereof. Using the theory of indirect measurements, we then draw conclusions about th... | {
"timestamp": "2010-09-23T02:02:00",
"yymm": "1009",
"arxiv_id": "1009.4349",
"language": "en",
"url": "https://arxiv.org/abs/1009.4349"
} |
\section{Introduction}
The physics of progressive material damage and healing under load has been studied using models that incorporate both failure thresholds and load sharing. Models of this class include slider-block models and fiber-bundle models. In both models, external loads are applied to a ``loader plate''... | {
"timestamp": "2010-09-22T02:03:00",
"yymm": "1009",
"arxiv_id": "1009.4166",
"language": "en",
"url": "https://arxiv.org/abs/1009.4166"
} |
\section{Introduction}
Let $X$ be a Banach space and
\[
\A_n:\D_n\to X,
\qquad
\D_n={\rm dom}(\A_n)\subset X,
\]
inftinitesimal generators of strongly continuous contraction semigroups $e^{t\A_n}$ on $X$. It is classical that
\begin{equation}\label{se}
e^{t\A_n}f\xrightarrow[n]{} e^{t\A_0}f,
\qquad
f\in... | {
"timestamp": "2010-09-21T02:03:22",
"yymm": "1009",
"arxiv_id": "1009.3821",
"language": "en",
"url": "https://arxiv.org/abs/1009.3821"
} |
\section{Introduction} The thermoelectric properties of
nanomaterials have attracted a great deal of interest in the last
few years due to the potential applications in power generation
and refrigeration \cite{Dresselhaus}. There is increasing evidence
that the thermoelectric performance of nanostructured materials
can... | {
"timestamp": "2010-09-23T02:00:25",
"yymm": "1009",
"arxiv_id": "1009.4215",
"language": "en",
"url": "https://arxiv.org/abs/1009.4215"
} |
\section{Introduction}
In D Euclidean dimensions, at $N=\infty$ $SU(N)$ pure YM simplifies~\cite{thooftN}, but this has not yet been turned
into a quantitative tool. We are trying to improve on this situation.
Let ${\cal O}$ be an observable characterized by one single scale $l$
in 4D.
For $l\Lambda_N\ll 1$, ... | {
"timestamp": "2010-09-21T02:04:11",
"yymm": "1009",
"arxiv_id": "1009.3915",
"language": "en",
"url": "https://arxiv.org/abs/1009.3915"
} |
\section{Introduction}
\hspace{15pt} Since some decades ago just after the discovery of asymptotic freedom of QCD
\cite{asymp-freedom} the possibility of the existence of a new state of matter in
high energy physics is under consideration, namely, a color deconfined phase
of quarks and gluons, the so-called quark-g... | {
"timestamp": "2010-09-21T02:01:12",
"yymm": "1009",
"arxiv_id": "1009.3596",
"language": "en",
"url": "https://arxiv.org/abs/1009.3596"
} |
\section{Partial permutations and the Ivanov-Kerov algebra}
Since our argument is essentially inspired by the construction of \cite{IK99}, let us recall it briefly. A \textbf{partial permutation} of order $n$ is a pair $(\sigma,S)$ where $S$ is a subset of $\lle 1,n\rre$, and $\sigma$ is a permutation in $\sym(S)$. Alt... | {
"timestamp": "2010-09-23T02:01:12",
"yymm": "1009",
"arxiv_id": "1009.4285",
"language": "en",
"url": "https://arxiv.org/abs/1009.4285"
} |
\section{Geometric Huffman Coding}
\label{sec:ghc}
For a PMF $\boldsymbol{p}$ and a vector $\boldsymbol{x}$ with non-negative entries, the KL-distance is given by
\begin{align}
\kl(\boldsymbol{p}\Vert\boldsymbol{x})=\sum_i p_i\log \frac{p_i}{x_i}.\label{eq:wKL}
\end{align}
Note that $\kl(\boldsymbol{p}\Vert\boldsymbol... | {
"timestamp": "2011-01-04T02:02:23",
"yymm": "1009",
"arxiv_id": "1009.3751",
"language": "en",
"url": "https://arxiv.org/abs/1009.3751"
} |
\section{Introduction}
In our current picture of the Universe, structure evolves hierarchically from an initial density field that is very nearly homogenous. Tiny perturbations in this field seed the growth of overdensities, which then accrete more matter through gravitational collapse. As matter is pulled into these... | {
"timestamp": "2010-09-23T02:00:13",
"yymm": "1009",
"arxiv_id": "1009.4191",
"language": "en",
"url": "https://arxiv.org/abs/1009.4191"
} |
\section{Introduction and main results.}This paper stems from a question raised by Moshe Marcus and Laurent V\'{e}ron several years ago and its answer \cite{anc4} (see the appendix in \cite{VYA} and the comments after Theorem \ref{charac} below). Another independent -- and recent -- question of Moshe Marcus has also... | {
"timestamp": "2012-03-09T02:01:59",
"yymm": "1009",
"arxiv_id": "1009.4084",
"language": "en",
"url": "https://arxiv.org/abs/1009.4084"
} |
\section{Introduction}
A manifestly covariant gauge-invariant cosmological perturbation
theory for \textsc{flrw} universes based on the Theory of General
Relativity combined with Thermodynamics and a realistic equation of
state for the pressure $p=p(n,\varepsilon)$ has been developed in a
foregoing article~\cite{2010a... | {
"timestamp": "2010-09-21T02:04:17",
"yymm": "1009",
"arxiv_id": "1009.3920",
"language": "en",
"url": "https://arxiv.org/abs/1009.3920"
} |
\section{Introduction}
Let $C$ be a curve in $\mathbb{P}^3_k$, being $k$ an algebraically closed field. Let $\Gamma$ be the generic plane section of $C$. In this paper we study the problem of finding bounds on the degree of $C$ in such a way that, if $\Gamma$ is contained in a plane curve of degree $s$, then $C$ is co... | {
"timestamp": "2010-09-22T02:01:21",
"yymm": "1009",
"arxiv_id": "1009.4017",
"language": "en",
"url": "https://arxiv.org/abs/1009.4017"
} |
\section{Introduction}
The resolution and interpretability of transmission electron microscopy (TEM) images have been hampered for decades by the strong aberrations of magnetic electron lenses. In particular the spherical aberration has been the dominant resolution-limiting aberration. The most severe consequence of sp... | {
"timestamp": "2010-09-22T02:01:36",
"yymm": "1009",
"arxiv_id": "1009.4038",
"language": "en",
"url": "https://arxiv.org/abs/1009.4038"
} |
\section{Introduction}
We start with the formal definition of $k$-step nilmanifolds.
\begin{definition} Let $L$ be a $k$-nilpotent Lie group. This means that the $k$-fold iterated commutator $$[\dots[[L,L],L],L\dots]$$ is trivial. Let $\Gamma$ be a co-compact subgroup in $L$. The left coset space $N=L/\Gamma$ is a co... | {
"timestamp": "2012-06-12T02:03:54",
"yymm": "1009",
"arxiv_id": "1009.3825",
"language": "en",
"url": "https://arxiv.org/abs/1009.3825"
} |
\section{Introduction}
Within the framework of a global approach to quantum theory
\cite{dewi03}, the path integrals of ordinary
quantum mechanics \cite{feyn48} and
the functional integrals of quantum field theory remain a tool of
fundamental importance and well suited for a Lagrangian, and hence
fully relativistic,... | {
"timestamp": "2010-09-22T02:01:41",
"yymm": "1009",
"arxiv_id": "1009.4050",
"language": "en",
"url": "https://arxiv.org/abs/1009.4050"
} |
\section{Introduction}
The relationship between the Einstein field equations and the
first law of black hole thermodynamics was first presented by
Jacobson \cite{jac}. Padmanabhan \cite {a6} made the key
development by establishing a general formalism for understanding
the thermodynamics of horizons in spherical... | {
"timestamp": "2010-09-21T02:02:42",
"yymm": "1009",
"arxiv_id": "1009.3749",
"language": "en",
"url": "https://arxiv.org/abs/1009.3749"
} |
\section*{Introduction}
It is well-known that every Del Pezzo surface of degree~5 over a field $k$
(not necessarily algebraically closed) has a proper parametrization
with coefficients in $k$ (see \cite{Swinnerton:72,Sheperd-Barron:92}).
In this paper, we give a simple algorithm for constructing such a parametrization... | {
"timestamp": "2011-05-18T02:01:52",
"yymm": "1009",
"arxiv_id": "1009.4044",
"language": "en",
"url": "https://arxiv.org/abs/1009.4044"
} |
\section{#1}}
\def\alpha} \def\b {\beta} \def\g {\gamma {\alpha} \def\b {\beta} \def\g {\gamma}
\def\Gamma} \def\d {\delta} \def\D {\Delta {\Gamma} \def\d {\delta} \def\D {\Delta}
\def\epsilon} \def\ve {\varepsilon} \def\k {\kappa {\epsilon} ... | {
"timestamp": "2011-10-26T02:03:27",
"yymm": "1009",
"arxiv_id": "1009.4428",
"language": "en",
"url": "https://arxiv.org/abs/1009.4428"
} |
\section{Introduction}
The application of elastic waves of suitable power and frequency (in
particular ultrasounds) to a liquid with gas dispersed in it gives
rise to the phenomenon known as acoustic cavitation~\cite{cg,bren}.
The main physical effects occurring in a cavitated liquid can be
accounted for in term... | {
"timestamp": "2010-09-22T02:02:33",
"yymm": "1009",
"arxiv_id": "1009.4127",
"language": "en",
"url": "https://arxiv.org/abs/1009.4127"
} |
\section{Introduction}
Synoptic surveys are increasingly important probes of the sky at all wavelengths.
These surveys provide the opportunity to simultaneously probe the static and
variable components of the Universe through multiple observations of the sky.
Complete static catalogs such as that of the NRAO VLA Sk... | {
"timestamp": "2010-09-28T02:02:50",
"yymm": "1009",
"arxiv_id": "1009.4443",
"language": "en",
"url": "https://arxiv.org/abs/1009.4443"
} |
\section{Introduction}
The deconfinement phase transition in dense matter, a manifestation
of asymptotic freedom of quantum chromodynamics (QCD), may lead
to stable quark matter cores in massive compact stars. The deconfined
(``liberated'') quarks occupy continuum of scattering states, which in
the low-temperatu... | {
"timestamp": "2010-09-21T02:03:24",
"yymm": "1009",
"arxiv_id": "1009.3826",
"language": "en",
"url": "https://arxiv.org/abs/1009.3826"
} |
\section{The Problem of Drug Delivery
\label{The Problem of Drug Delivery}}
We could cure cancer
if we knew how to deliver a drug
intact to the cytosol
of every cancer cell,
sparing healthy cells.
The circulatory system can deliver
a drug to every cell in the body,
and certain chemical tricks
protect drugs from
... | {
"timestamp": "2010-09-21T02:01:17",
"yymm": "1009",
"arxiv_id": "1009.3606",
"language": "en",
"url": "https://arxiv.org/abs/1009.3606"
} |
\section{Introduction}
\label{sec:intro}
The discovery of planets beyond the confines of our Solar system has
presented many surprises and continues to challenge our understanding
of planet formation and their subsequent evolution. This is
particularly true in the case of hot-Jupiters, whose short orbital
periods of a... | {
"timestamp": "2011-02-22T02:04:01",
"yymm": "1009",
"arxiv_id": "1009.4132",
"language": "en",
"url": "https://arxiv.org/abs/1009.4132"
} |
\section{Introduction}\label{sec1}
Consider the one-dimensional non-linear Schr\"odinger
equation (NLS) with periodically varying dispersion
coefficient
\begin{equation}\label{eq:periodic-NLS}
i u_t + d(t) u_{xx} + |u|^2 u = 0.
\end{equation}
It describes the amplitude of a signal
transmitted via amplitude modula... | {
"timestamp": "2010-09-21T02:02:15",
"yymm": "1009",
"arxiv_id": "1009.3707",
"language": "en",
"url": "https://arxiv.org/abs/1009.3707"
} |
\section{Introduction}
The temperature anisotropy and polarization state of the CMB constitute a
unique window on the physical state of the universe in the era of
recombination ($z\approx 1100$), $\sim 400,000$ years after the big bang.
Measurements with the COBE and WMAP satellites, along with a host
ground-based... | {
"timestamp": "2010-09-22T02:02:21",
"yymm": "1009",
"arxiv_id": "1009.4110",
"language": "en",
"url": "https://arxiv.org/abs/1009.4110"
} |
\section{introduction}
The wealth of data produced by the Relativistic Heavy-Ion Collider (RHIC)
has lead to new insights about the nature of the quark-gluon plasma (QGP),
in particular in the strongly coupled regime just above the chiral phase
transition (see Refs.~\cite{Muller:2006ee,Shuryak:2008eq,BraunMunzinger... | {
"timestamp": "2010-09-21T02:02:48",
"yymm": "1009",
"arxiv_id": "1009.3762",
"language": "en",
"url": "https://arxiv.org/abs/1009.3762"
} |
\section{Introduction}
\subsection{Main results}
In his book \cite{Sha74}, Shafarevich splits the classification of universal covers of projective manifolds into two types. The type I corresponds to manifolds having a finite fundamental group and their universal covers still belong to the class of projective manifold... | {
"timestamp": "2010-09-21T02:02:33",
"yymm": "1009",
"arxiv_id": "1009.3739",
"language": "en",
"url": "https://arxiv.org/abs/1009.3739"
} |
\section{Introduction}
Galaxies have long been known to follow well-ordered sequences in many properties
\citep[see][for a review]{R&H}. In the simplest classification scheme,
galaxies divide into spirals and ellipticals. In more complex schemes, these classes are partitioned into additional
sub-classes. Irrespect... | {
"timestamp": "2010-09-23T02:01:28",
"yymm": "1009",
"arxiv_id": "1009.4309",
"language": "en",
"url": "https://arxiv.org/abs/1009.4309"
} |
\section{Introduction}
\label{introduction}
I begin with simple derivations of some results from \cite{1}. Let $g$ be the element $1+x+x^{4}+x^{9}+\cdots$ of $A=\ensuremath{\mathbb{Z}}/2 [[x]]$. Write $\frac{1}{g}$ as $\sum b_{i}x^{i}$ with the $b_{i}$ in $\ensuremath{\mathbb{Z}}/2$, and let $B$ consist of all $n$ wit... | {
"timestamp": "2010-09-22T02:00:53",
"yymm": "1009",
"arxiv_id": "1009.3985",
"language": "en",
"url": "https://arxiv.org/abs/1009.3985"
} |
\section{Summary}
We (\cite{Bro07}, \cite{BLMM08}, \cite{Lee02}, \cite{Mor07}, \cite{Mor08}) model binaries in which the primary star (BH progenitor) evolves as a single star until its core begins He burning. When He burning begins in the core the stellar radius expands a further $10$ to $15\%$ relative to the red ... | {
"timestamp": "2010-09-23T02:01:47",
"yymm": "1009",
"arxiv_id": "1009.4334",
"language": "en",
"url": "https://arxiv.org/abs/1009.4334"
} |
\section{Introduction}\label{sec:introduction}
As we are moving on from desktop computers to a pervasive computing
intelligence interwoven in the ``fabric of everyday life'', our
environment is about to become enriched with more and more smart
assistance systems.
Through this transformation, it becomes feasibl... | {
"timestamp": "2010-09-23T02:00:57",
"yymm": "1009",
"arxiv_id": "1009.4259",
"language": "en",
"url": "https://arxiv.org/abs/1009.4259"
} |
\section{Introduction} \label{sec:intro}
When referring to a ``network'', one typically visualizes it as a distributed system where nodes correspond to agents or processors.
These nodes can only interact locally and therefore, since they all lack of global information, new algorithmic and complexity notions arise.
In... | {
"timestamp": "2010-10-06T02:03:19",
"yymm": "1009",
"arxiv_id": "1009.4447",
"language": "en",
"url": "https://arxiv.org/abs/1009.4447"
} |
\section{Introduction}
Cosmology has definitely entered a phase of precision measurements:
Cosmic Microwave Background (CMB) anisotropies \citep{WMAP7}, Large
Scale Structure (LSS) observations \citep{LSS} and the
magni\-tu\-de-redshift distribution of Supernov\ae{} Ia \citep{SNIa}
to name the most prominent, have rad... | {
"timestamp": "2010-09-23T02:01:42",
"yymm": "1009",
"arxiv_id": "1009.4327",
"language": "en",
"url": "https://arxiv.org/abs/1009.4327"
} |
\section{Non Lipschitz drifts}\label{nonlip}
The interest for such mean field limits with locally but non globally Lipschitz drifts has been renewed by kinetic models, in which the interaction may become larger for larger relative velocities.
For instance, for space homogeneous models such as~\eqref{edpMKV} with... | {
"timestamp": "2010-09-21T02:03:44",
"yymm": "1009",
"arxiv_id": "1009.3855",
"language": "en",
"url": "https://arxiv.org/abs/1009.3855"
} |
\section{Introduction}
\label{sec:intro}
The Dynamical Mean-Field Theory (DMFT) maps lattice models
for electrons with a Hubbard-type interaction
onto effective single-impurity models;
for a review, see Ref.~[\onlinecite{dmftreviews}].
The parameters of the impurity model must be determined in such a way
that the s... | {
"timestamp": "2010-09-22T02:02:16",
"yymm": "1009",
"arxiv_id": "1009.4100",
"language": "en",
"url": "https://arxiv.org/abs/1009.4100"
} |
\section{Introduction}
\label{intro}
Prolog and Logtalk \cite{pmoura03,lgtuserman2390} meta-predicates are predicates with one or more arguments that are either goals or closures\footnote{In Prolog and Logtalk, a closure is defined as a callable term used to construct a goal by appending one or more additional argumen... | {
"timestamp": "2010-09-21T02:02:54",
"yymm": "1009",
"arxiv_id": "1009.3773",
"language": "en",
"url": "https://arxiv.org/abs/1009.3773"
} |
\section{}
\end{document}
| {
"timestamp": "2011-02-03T02:00:54",
"yymm": "1009",
"arxiv_id": "1009.4001",
"language": "fa",
"url": "https://arxiv.org/abs/1009.4001"
} |
\section{Introduction}
Problems dealing with the persistence of motion of tracer particles -- that
is, the tendency to continue or not in the same direction at a scattering
event -- are encountered in many areas of physics; see e.g.\
\cite{Haus:1987p513} and references therein. We are specifically interested
in the e... | {
"timestamp": "2010-09-21T02:04:19",
"yymm": "1009",
"arxiv_id": "1009.3922",
"language": "en",
"url": "https://arxiv.org/abs/1009.3922"
} |
\section{Introduction}
\label{sec:intro}
Clusters of galaxies are receiving an increasing interest in astronomical studies in the last decade for a variety of reasons. They are the largest gravitationally bound objects in the universe and provide ideal organized laboratories for the cosmic evolution of baryons, in the ... | {
"timestamp": "2010-09-22T02:00:19",
"yymm": "1009",
"arxiv_id": "1009.3930",
"language": "en",
"url": "https://arxiv.org/abs/1009.3930"
} |
\section{Introduction}
Communication complexity is one of the most basic models in computational complexity,
with wide-ranging applications in computer science~\cite{kushilevitznisan-book}.
The typical question asked in this model is the following. Two remote players, call them Alice and Bob,
are each given an input a... | {
"timestamp": "2010-09-21T02:01:37",
"yymm": "1009",
"arxiv_id": "1009.3640",
"language": "en",
"url": "https://arxiv.org/abs/1009.3640"
} |
\section{Globally Operator Monotone Functions}
\label{secg}
\begin{definition}
Let $E$ be an open set in $\mathbb R^d$, and $f$ be a real-valued
$C^1$ function on
$E$.
Say $f$ is globally operator monotone on $E$ if, whenever
$S$ and $T$
are $d$-tuples of commuting bounded self-adjoint operators on a Hilbert space
w... | {
"timestamp": "2012-03-15T01:04:21",
"yymm": "1009",
"arxiv_id": "1009.3921",
"language": "en",
"url": "https://arxiv.org/abs/1009.3921"
} |
\section{Introduction}
Fix a prime number $p$.
The aim of this paper is to define a complete moduli stack of
degree-$p$ covers $Y \to \cX$, with $Y$ a stable curve which is a
$\cG$-torsor over $\cX$, for a suitable group scheme
$\cG/\cX$. The curve $\cX$ is a twisted curve in the sense of
\cite{A-V,AOV2} but in gener... | {
"timestamp": "2010-09-23T02:00:52",
"yymm": "1009",
"arxiv_id": "1009.4126",
"language": "en",
"url": "https://arxiv.org/abs/1009.4126"
} |
\section{Introduction}
In our recent paper \cite{OP}, inspired by the classification of conic-connected manifolds given in \cite{IR}, we started the study of \emph{rationally cubic connected} manifolds (RCC-manifolds, for short), i.e. smooth complex projective polarized varieties $(X,H)$ of dimension $ n \ge 2$ which... | {
"timestamp": "2010-09-21T02:03:18",
"yymm": "1009",
"arxiv_id": "1009.3811",
"language": "en",
"url": "https://arxiv.org/abs/1009.3811"
} |
\section{Introduction}\label{introduction}
Consider the three-node chain network in Fig. \ref{fig:figure1}. Nodes $S_1$ and $S_2$ are the source nodes which are going to communicate with each other. In particular, we consider two real numbers $r_1$ and $r_2$, which $S_1$ and $S_2$ are going to exchange, respectively... | {
"timestamp": "2010-09-21T02:03:10",
"yymm": "1009",
"arxiv_id": "1009.3797",
"language": "en",
"url": "https://arxiv.org/abs/1009.3797"
} |
\section{Cell-Penetrating Peptides
\label{Cell-Penetrating Peptides}}
Polyarginine, TAT~\citep{Loewenstein1988,Pabo1988},
Penetratin, and other short, positively
charged peptides can penetrate
the plasma membranes of live cells
and can tow along with them cargos
that greatly exceed the 600 Da restriction barrier.
They... | {
"timestamp": "2010-09-21T02:01:17",
"yymm": "1009",
"arxiv_id": "1009.3607",
"language": "en",
"url": "https://arxiv.org/abs/1009.3607"
} |
\section{Introduction}
This paper is concerned with Aczel's predicative constructive set theory {\bf CZF} and with related systems for predicative algebraic set theory; it also studies extensions of {\bf CZF}, for example by the axiom of countable choice.
We are particularly interested in certain statements about Can... | {
"timestamp": "2011-11-17T02:02:05",
"yymm": "1009",
"arxiv_id": "1009.3553",
"language": "en",
"url": "https://arxiv.org/abs/1009.3553"
} |
\section{Introduction}
\label{sec:intro}
The existence of an intricate network of filaments in the large scale distribution of matter is now considered an established fact. Its was first observed by \citet{lapparent86} \citep[see also {\it e.g. }][]{2Df} and latter theorized \citep[see {\it e.g. }][]{pogo96,bond96}: u... | {
"timestamp": "2010-09-22T02:01:17",
"yymm": "1009",
"arxiv_id": "1009.4015",
"language": "en",
"url": "https://arxiv.org/abs/1009.4015"
} |
\section{Friedmann equations in the $f(T)$ theory}
In the framework of $f(T)$-gravity, the Friedmann equations in the
flat spatial Friedmann-Robertson-Walker (FRW) universe are given by
\cite{Karami1,Ferraro,bengochea,yerzhanov,linder,WufT,Bamba}
\begin{equation}
\frac{3}{k^2}H^2=\rho+\rho_T,\label{fT11}
\end... | {
"timestamp": "2010-09-21T02:01:09",
"yymm": "1009",
"arxiv_id": "1009.3587",
"language": "en",
"url": "https://arxiv.org/abs/1009.3587"
} |
\section{}
| {
"timestamp": "2010-09-22T02:00:58",
"yymm": "1009",
"arxiv_id": "1009.3990",
"language": "en",
"url": "https://arxiv.org/abs/1009.3990"
} |
\section{Introduction}
Plasma is a ubiquitous form of matter in the universe, nearly always
found to be magnetized and turbulent. In a wide variety of space and
astrophysical plasmas, the dissipation of turbulent fluctuations makes
a significant contribution to the thermodynamic heating of the plasma,
requiring an un... | {
"timestamp": "2010-09-23T02:00:23",
"yymm": "1009",
"arxiv_id": "1009.4212",
"language": "en",
"url": "https://arxiv.org/abs/1009.4212"
} |
\section{Introduction}
\label{sec:intro}
In this paper we study embeddings of complex projective curves
into (smooth) Calabi-Yau complete intersection ($CICY$) threefolds. Such embeddings,
and Calabi-Yau threefolds in general, have in the past decades been
objects of extended interest in both algebraic geometry and... | {
"timestamp": "2010-09-23T02:02:34",
"yymm": "1009",
"arxiv_id": "1009.4419",
"language": "en",
"url": "https://arxiv.org/abs/1009.4419"
} |
\section{Introduction}
\label{cha:int}
Many firms these days,
forced by increasing international competition and
an unstable economy,
are opting to
specialize rather than generalize as a way of maintaining their competitiveness.
Consequently,
they cannot rely solely on themselves, but must
cooperate by comb... | {
"timestamp": "2010-09-22T02:01:13",
"yymm": "1009",
"arxiv_id": "1009.4013",
"language": "en",
"url": "https://arxiv.org/abs/1009.4013"
} |
\section{Introduction}
Ever since the discovery of the so-called $D_{sJ}$ in 2003 by BaBar\cite{BB03} and
CLEO,\cite{CLEO03} which are now identified as $D_s(2317)$ and $D_s(2460)$ with $j_q^P
=(1/2)^+$ and $(3/2)^+$, respectively, the particles are discovered in the vicinity of
this energy or above one after ano... | {
"timestamp": "2010-09-21T02:03:43",
"yymm": "1009",
"arxiv_id": "1009.3853",
"language": "en",
"url": "https://arxiv.org/abs/1009.3853"
} |
\section{Introduction}
The Kepler satellite delivers light curves of unique accuracy and time coverage,
providing unprecedented data for the asteroseismic analysis. The identification of
non-radial pulsation modes and the asteroseismic modeling, on the other hand,
require a classification of the observed stars in te... | {
"timestamp": "2010-09-23T02:01:34",
"yymm": "1009",
"arxiv_id": "1009.4316",
"language": "en",
"url": "https://arxiv.org/abs/1009.4316"
} |
\section{Introduction and main results}\label{intro}
Recently, there has been much progress in describing the complexity
of various relations between subspaces of a given separable Banach space.
The reader is referred to \cite{FG, FLRo, FRo} for the known results on
the relations of isomorphism, biembeddability, and m... | {
"timestamp": "2010-09-21T02:01:10",
"yymm": "1009",
"arxiv_id": "1009.3591",
"language": "en",
"url": "https://arxiv.org/abs/1009.3591"
} |
\section{Introduction}
Strong evidences from the current cosmological observations such as supernovae type Ia (SNeIa)\cite{A.G. Riess}, cosmic microwave background (CMB)\cite{D. N. Spergel et al.} and large scale structure (LSS)\cite{M. Tegmark et al.} converge upon the fact that the universe is spatially flat and the... | {
"timestamp": "2010-09-21T02:02:55",
"yymm": "1009",
"arxiv_id": "1009.3776",
"language": "en",
"url": "https://arxiv.org/abs/1009.3776"
} |
\section{Introduction}
According to the computationalist theory of the mind, conscious experiences are identified with computational states of algorithms \cite{compt,compb}. This view is the logical conclusion one arrives at if one assumes that physics applies to everything, including us. One can then still question ... | {
"timestamp": "2010-09-24T02:00:21",
"yymm": "1009",
"arxiv_id": "1009.4472",
"language": "en",
"url": "https://arxiv.org/abs/1009.4472"
} |
\section{Introduction}\label{sec0}
\indent
In a classic paper \cite{B}, Beurling posed and answered two fundamental questions for the unilateral shift operator on Hilbert space and its adjoint. The first problem was the characterization of the cyclic vectors for the forward shift operator, while the second one conce... | {
"timestamp": "2010-09-23T02:02:38",
"yymm": "1009",
"arxiv_id": "1009.4427",
"language": "en",
"url": "https://arxiv.org/abs/1009.4427"
} |
\section{Introduction}
A random $\mathbb{R}^d$-valued vector $X$ has a regularly varying distribution with
characteristic exponent $\alpha>0$ if there exists a finite measure $\sigma$ in
the unit sphere $S^{d-1}=\left\{x~\left|~\|x\|=1, x\in\mathbb{R}^d\right.\right\}$ such that
$\forall B\in\mathcal{B}(S^{d-1})$ with ... | {
"timestamp": "2010-09-22T02:01:54",
"yymm": "1009",
"arxiv_id": "1009.4070",
"language": "en",
"url": "https://arxiv.org/abs/1009.4070"
} |
\section{Introduction}
\label{sec1}
Antiferromagnetically interacting Heisenberg spins on geometrically frustrated lattices
have attracted much attention of physicists during last years.\cite{lhuillier,mikeska,richter_lnp}
A rapidly developing direction in this area
is the study of the properties of such models in the... | {
"timestamp": "2010-09-21T02:03:25",
"yymm": "1009",
"arxiv_id": "1009.3828",
"language": "en",
"url": "https://arxiv.org/abs/1009.3828"
} |
\section{Introduction}
Let us begin with a few words regarding the title. A couple of days after I gave this talk in Valencia, Blas {\it et al} submitted the following paper to the arXiv: {\it Models of non-relativistic quantum gravity: the good, the bad and the healthy} \cite{gbh}. At the time I did not know whether t... | {
"timestamp": "2010-09-22T02:01:56",
"yymm": "1009",
"arxiv_id": "1009.4074",
"language": "en",
"url": "https://arxiv.org/abs/1009.4074"
} |
\section{Introduction}
The last decade has seen an explosive growth in wireless network services and consequently an increasing demand of high data rates on wireless networks.
Multiple-input-multiple-output (MIMO)~\cite{MIMO:Foschini:98:limits,MIMO:Teletar99:CapacityOfMultiAntennaGaus} communication has generated a lo... | {
"timestamp": "2010-09-22T02:02:07",
"yymm": "1009",
"arxiv_id": "1009.4091",
"language": "en",
"url": "https://arxiv.org/abs/1009.4091"
} |
\section{Introduction} \label{Sect:Intro}
Boosting is a powerful learning technique
for improving the accuracy of any given classification algorithm.
It has been attracting much research interest in the machine learning
and pattern recognition community.
Since Viola and Jones applied boosting to ... | {
"timestamp": "2010-09-21T02:02:13",
"yymm": "1009",
"arxiv_id": "1009.3702",
"language": "en",
"url": "https://arxiv.org/abs/1009.3702"
} |
\section{Introduction}
Recently much attention has been given to the effects of currents that arise from the axial anomaly in QCD. Such currents arise in the presence of a magnetic field when there is an imbalance in the number of right- and left-handed fermions. The most well known of these are the charge separation ... | {
"timestamp": "2011-07-05T02:05:18",
"yymm": "1009",
"arxiv_id": "1009.4230",
"language": "en",
"url": "https://arxiv.org/abs/1009.4230"
} |
\section{Introduction}\label{sec: intro}
Finding (sufficiently) sparse solutions of underdetermined
systems of linear equations has been studied extensively in recent
years~\cite{ChenDS99,CandRT06,DonoH01,DonoE03,EladB02,Fuch04,GribL06,GribN03,LiCA03,Trop04,ZibuP01}.
The problem has a growing range of applications ... | {
"timestamp": "2010-09-21T02:04:01",
"yymm": "1009",
"arxiv_id": "1009.3890",
"language": "en",
"url": "https://arxiv.org/abs/1009.3890"
} |
\section{Introduction}
The early developments in Ramsey theory focused mainly on partition
regularity of systems of linear equations. A system $\mathcal{L}$ of
linear homogeneous equations with coefficients in a ring $R$ is called
\emph{$r$-regular} over $R$ if, for every $r$-coloring of the nonzero
elements of $R$, t... | {
"timestamp": "2010-09-23T02:00:40",
"yymm": "1009",
"arxiv_id": "1009.4234",
"language": "en",
"url": "https://arxiv.org/abs/1009.4234"
} |
\section{Introduction}
The aim of this paper is to describe a small number of types of groups, which
have the property that every finitely generated soluble group that is not
virtually abelian has a subgroup of one of these types.
In Section~\ref{twogenmetasec}, we shall define a class of 2-generator
abelian-by-cycli... | {
"timestamp": "2011-03-28T02:01:31",
"yymm": "1009",
"arxiv_id": "1009.4149",
"language": "en",
"url": "https://arxiv.org/abs/1009.4149"
} |
\section{Introduction}
$\lambda$-rings were first introduced in an algebraic-geometry
setting by Grothendieck in 1958, then later used in group theory by
Atiyah and Tall. In 1962 Adams introduced the operations $\Psi^{i}$ to study vector fields of spheres. These operations give us another type of ring, the $\Psi$-rings... | {
"timestamp": "2010-09-23T02:02:06",
"yymm": "1009",
"arxiv_id": "1009.4360",
"language": "en",
"url": "https://arxiv.org/abs/1009.4360"
} |
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