1,501 research outputs found
Momentum-resolved study of an array of 1D strongly phase-fluctuating Bose gases
We investigate the coherence properties of an array of one-dimensional Bose
gases with short-scale phase fluctuations. The momentum distribution is
measured using Bragg spectroscopy and an effective coherence length of the
whole ensemble is defined. In addition, we propose and demonstrate that
time-of-flight absorption imaging can be used as a simple probe to directly
measure the coherence-length of 1D gases in the regime where phase-fluctuations
are strong. This method is suitable for future studies such as investigating
the effect of disorder on the phase coherence.Comment: 4 pages, 4 figure
Cosmic shear surveys
Gravitational weak shear produced by large-scale structures of the universe
induces a correlated ellipticity distribution of distant galaxies. The
amplitude and evolution with angular scale of the signal depend on cosmological
models and can be inverted in order to constrain the power spectrum and the
cosmological parameters. We present our recent analysis of 50 uncorrelated VLT
fields and the very first constrains on () and the nature of
primordial fluctuations based on the join analysis of present-day cosmic shear
surveys.Comment: Latex, 7 pages. To appear in the ESO Proceedings ``Deep Fields'',
Garching Oct 9-12, 200
Mass-detection of a matter concentration projected near the cluster Abell 1942: Dark clump or high-redshift cluster?
A weak-lensing analysis of wide-field - and -band images centered on
the cluster Abell 1942 has uncovered a mass concentration arcminutes
South of the cluster center. A statistical analysis shows that the detections
are highly significant. No strong concentration of bright galaxies is seen at
the position of the mass concentration, though a slight galaxy number
overdensity and a weak extended X-ray source are present about 1' away from its
center.
From the spatial dependence of the tangential alignment around the center of
the mass concentration, we inferred a lower bound on the mass inside a sphere
of radius \ts Mpc of , much higher
than crude mass estimates based on X-ray data. No firm conclusion can be
inferred about the nature of the clump. If it were a high-redshift cluster, the
weak X-ray flux would indicate that it had an untypically low X-ray luminosity
for its mass; if the X-ray emission were physically unrelated to the mass
concentration, this conclusion would be even stronger.
The search for massive halos by weak lensing enables us for the first time to
select halos based on their mass properties only and to detect new types of
objects, e.g., dark halos. The mass concentration in the field of A1942 may be
the first example of such a halo.Comment: Sumitted to A&A Main Journal. 15 pages, 11 figures. 75 Kb gzipped tar
file. Figures with images not included, but available on ftp.iap.fr
/pub/from_users/mellier/A1942: a1942darkclump.ps.gz (2.1 Mb
Detection of correlated galaxy ellipticities on CFHT data: first evidence for gravitational lensing by large-scale structures
We report the detection of a significant (5.5 sigma) excess of correlations
between galaxy ellipticities at scales ranging from 0.5 to 3.5 arc-minutes.
This detection of a gravitational lensing signal by large-scale structure was
made using a composite high quality imaging survey of 6300 arcmin^2 obtained at
the Canada France Hawaii Telescope (CFHT) with the UH8K and CFH12K panoramic
CCD cameras. The amplitude of the excess correlation is 2.2\pm 0.2 % at 1
arcmin scale, in agreement with theoretical predictions of the lensing effect
induced by large-scale structure.We provide a quantitative analysis of
systematics which could contribute to the signal and show that the net effect
is small and can be corrected for. We show that the measured ellipticity
correlations behave as expected for a gravitational shear signal. The
relatively small size of our survey precludes tight constraints on cosmological
models. However the data are in favor of cluster normalized cosmological
models, and marginally reject Cold Dark Matter models with (Omega=0.3,
sigma_8<0.6) or (Omega=1, sigma_8=1). The detection of cosmic shear
demonstrates the technical feasibility of using weak lensing surveys to measure
dark matter clustering and the potential for cosmological parameter
measurements, in particular with upcoming wide field CCD cameras.Comment: 19 pages. 19 Figures. Revised version accepted in A&
Evolutionary advantages of adaptive rewarding
Our wellbeing depends as much on our personal success, as it does on the
success of our society. The realization of this fact makes cooperation a very
much needed trait. Experiments have shown that rewards can elevate our
readiness to cooperate, but since giving a reward inevitably entails paying a
cost for it, the emergence and stability of such behavior remain elusive. Here
we show that allowing for the act of rewarding to self-organize in dependence
on the success of cooperation creates several evolutionary advantages that
instill new ways through which collaborative efforts are promoted. Ranging from
indirect territorial battle to the spontaneous emergence and destruction of
coexistence, phase diagrams and the underlying spatial patterns reveal
fascinatingly reach social dynamics that explains why this costly behavior has
evolved and persevered. Comparisons with adaptive punishment, however, uncover
an Achilles heel of adaptive rewarding that is due to over-aggression, which in
turn hinders optimal utilization of network reciprocity. This may explain why,
despite of its success, rewarding is not as firmly weaved into our societal
organization as punishment.Comment: 14 pages, 8 figures; accepted for publication in New Journal of
Physic
Fractional Statistics in Three Dimensions: Compact Maxwell-Higgs System
We show that a (3+1)-dimensional system composed of an open magnetic vortex
and an electrical point charge exhibits the phenomenon of Fermi-Bose
transmutation. In order to provide the physical realization of this system we
focus on the lattice compact scalar electrodynamics whose topological
excitations are open Nielsen-Olesen strings with magnetic monopoles attached at
their ends.Comment: 8 page
Exploring correlated 1D Bose gases from the superfluid to the Mott-insulator state by inelastic light scattering
We report the Bragg spectroscopy of interacting one-dimensional Bose gases
loaded in optical lattices across the superfluid to Mott-insulator phase
transition. Elementary excitations are created with a non-zero momentum and the
response of the correlated 1D gases is in the linear regime. The complexity of
the strongly correlated quantum phases is directly displayed in the spectra
which exhibit novel features. This work paves the way for a precise
characterization of the state of correlated atomic phases in optical lattices.Comment: 5 pages, 4 figure
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