95,571 research outputs found
Superfluid Transition in a Chiron Gas
Low temperature measurements of the magnetic susceptibility of LSCO suggest
that the superconducting transition is associated with the disappearance of a
vortex liquid. In this note we wish to draw attention to the fact that
spin-orbit-like interactions in a poorly conducting layered material can lead
to a new type of quantum ground state with spin polarized soliton-like charge
carriers as the important quantum degree of freedom. In 2-dimensions these
solitons are vortex-like, while in 3-dimensional systems they are
monopole-like. In either case there is a natural mechanism for the pairing of
spin up and spin down solitons, and we find that at low temperatures there is a
cross-over transition as a function of carrier density between a state where
the solitons are free and a condensate state where the spin up and spin down
solitons in neighboring layers are paired.Comment: 10 pages, 1 figur
How to Host a Data Competition: Statistical Advice for Design and Analysis of a Data Competition
Data competitions rely on real-time leaderboards to rank competitor entries
and stimulate algorithm improvement. While such competitions have become quite
popular and prevalent, particularly in supervised learning formats, their
implementations by the host are highly variable. Without careful planning, a
supervised learning competition is vulnerable to overfitting, where the winning
solutions are so closely tuned to the particular set of provided data that they
cannot generalize to the underlying problem of interest to the host. This paper
outlines some important considerations for strategically designing relevant and
informative data sets to maximize the learning outcome from hosting a
competition based on our experience. It also describes a post-competition
analysis that enables robust and efficient assessment of the strengths and
weaknesses of solutions from different competitors, as well as greater
understanding of the regions of the input space that are well-solved. The
post-competition analysis, which complements the leaderboard, uses exploratory
data analysis and generalized linear models (GLMs). The GLMs not only expand
the range of results we can explore, they also provide more detailed analysis
of individual sub-questions including similarities and differences between
algorithms across different types of scenarios, universally easy or hard
regions of the input space, and different learning objectives. When coupled
with a strategically planned data generation approach, the methods provide
richer and more informative summaries to enhance the interpretation of results
beyond just the rankings on the leaderboard. The methods are illustrated with a
recently completed competition to evaluate algorithms capable of detecting,
identifying, and locating radioactive materials in an urban environment.Comment: 36 page
A Deep Relevance Matching Model for Ad-hoc Retrieval
In recent years, deep neural networks have led to exciting breakthroughs in
speech recognition, computer vision, and natural language processing (NLP)
tasks. However, there have been few positive results of deep models on ad-hoc
retrieval tasks. This is partially due to the fact that many important
characteristics of the ad-hoc retrieval task have not been well addressed in
deep models yet. Typically, the ad-hoc retrieval task is formalized as a
matching problem between two pieces of text in existing work using deep models,
and treated equivalent to many NLP tasks such as paraphrase identification,
question answering and automatic conversation. However, we argue that the
ad-hoc retrieval task is mainly about relevance matching while most NLP
matching tasks concern semantic matching, and there are some fundamental
differences between these two matching tasks. Successful relevance matching
requires proper handling of the exact matching signals, query term importance,
and diverse matching requirements. In this paper, we propose a novel deep
relevance matching model (DRMM) for ad-hoc retrieval. Specifically, our model
employs a joint deep architecture at the query term level for relevance
matching. By using matching histogram mapping, a feed forward matching network,
and a term gating network, we can effectively deal with the three relevance
matching factors mentioned above. Experimental results on two representative
benchmark collections show that our model can significantly outperform some
well-known retrieval models as well as state-of-the-art deep matching models.Comment: CIKM 2016, long pape
Adaptive Optics Observations of the Galactic Center Young Stars
Adaptive Optics observations have dramatically improved the quality and
versatility of high angular resolution measurements of the center of our
Galaxy. In this paper, we quantify the quality of our Adaptive Optics
observations and report on the astrometric precision for the young stellar
population that appears to reside in a stellar disk structure in the central
parsec. We show that with our improved astrometry and a 16 year baseline,
including 10 years of speckle and 6 years of laser guide star AO imaging, we
reliably detect accelerations in the plane of the sky as small as 70
microarcsec/yr/yr (~2.5 km/s/yr) and out to a projected radius from the
supermassive black hole of 1.5" (~0.06 pc). With an increase in sensitivity to
accelerations by a factor of ~6 over our previous efforts, we are able to
directly probe the kinematic structure of the young stellar disk, which appears
to have an inner radius of 0.8". We find that candidate disk members are on
eccentric orbits, with a mean eccentricity of = 0.30 +/- 0.07. Such
eccentricities cannot be explained by the relaxation of a circular disk with a
normal initial mass function, which suggests the existence of a top-heavy IMF
or formation in an initially eccentric disk.Comment: 7 pages, 4 figures, SPIE Astronomical Telescopes and Instrumentation
201
The dust morphology of the elliptical Galaxy M86 with SPIRE
We present Herschel-SPIRE observations at 250–500 μm of the giant elliptical galaxy M 86 and examine the distribution of the resolved cold dust emission and its relation with other galactic tracers. The SPIRE images reveal three dust components: emission from the central region; a dust lane extending north-south; and a bright emission feature 10 kpc to the south-east. We estimate that ~10^6 M_☉ of dust is spatially coincident with atomic and ionized hydrogen, originating from stripped material from the nearby spiral NGC 4438 due to recent tidal interactions with M 86. The gas-to-dust ratio of the cold gas component ranges from ~20–80. We discuss the different heating mechanisms for the dust features
Proximity and anomalous field-effect characteristics in double-wall carbon nanotubes
Proximity effect on field-effect characteristic (FEC) in double-wall carbon
nanotubes (DWCNTs) is investigated. In a semiconductor-metal (S-M) DWCNT, the
penetration of electron wavefunctions in the metallic shell to the
semiconducting shell turns the original semiconducting tube into a metal with a
non-zero local density of states at the Fermi level. By using a two-band
tight-binding model on a ladder of two legs, it is demonstrated that anomalous
FEC observed in so-called S-M type DWCNTs can be fully understood by the
proximity effect of metallic phases.Comment: 4 pages, 4 figure
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