52,424 research outputs found
Neutrino-nucleon scattering rate in proto neutron star matter
We present a calculation of the neutrino-nucleon scattering cross section
which takes into account the nuclear correlations in the relativistic random
phase approximation. Our approach is based on a quantum hadrodynamics model
with exchange of , , , and mesons. In view
of applications to neutrino transport in the final stages of supernova
explosion and protoneutron star cooling, we study the evolution of the neutrino
mean free path as a function of density, proton-neutron asymmetry and
temperature. Special attention was paid to the issues of renormalization of the
Dirac sea, residual interactions in the tensor channel and meson mixing. It is
found that RPA corrections, with respect to the mean field approximation,
amount to only 10% to 15% at high density.Comment: 20 pages, 9 figures, subm. to EPJ
Relativistic approach to positronium levels in a strong magnetic field
We have investigated the bound states of an electron and positron in
superstrong magnetic fields typical for neutron stars. The complete
relativistic problem of positronium in a strong magnetic field has not been
succesfully solved up to now. In particular, we have studied the positronium
when it moves relativistically across the magnetic field. A number of problems
which deal with the pulsar magnetosphere, as well as the evolution of
protoneutron stars, could be considered as a field for application
Bar pattern speed evolution over the last 7 Gyr
The tumbling pattern of a bar is the main parameter characterising its
dynamics. From numerical simulations, its evolution since bar formation is
tightly linked to the dark halo in which the bar is formed through dynamical
friction and angular momentum exchange. Observational measurements of the bar
pattern speed with redshift can restrict models of galaxy formation and bar
evolution. We aim to determine, for the first time, the bar pattern speed
evolution with redshift based on morphological measurements. We have selected a
sample of 44 low inclination ringed galaxies from the SDSS and COSMOS surveys
covering the redshift range 0 <z< 0.8 to investigate the evolution of the bar
pattern speed. We have derived morphological ratios between the deprojected
outer ring radius (R_{ring}) and the bar size (R_{bar}). This quantity is
related to the parameter {\cal R}=R_{CR}/R_{bar} used for classifiying bars in
slow and fast rotators, and allow us to investigate possible differences with
redshift. We obtain a similar distribution of at all redshifts. We do not
find any systematic effect that could be forcing this result. The results
obtained here are compatible with both, the bulk of the bar population (~70%)
being fast-rotators and no evolution of the pattern speed with redshift. We
argue that if bars are long-lasting structures, the results presented here
imply that there has not been a substantial angular momentum exchange between
the bar and halo, as predicted by numerical simulations. In consequence, this
might imply that the discs of these high surface-brightness galaxies are
maximal.Comment: Accepted for publication in A&
Quantum computational tensor network on string-net condensate
The string-net condensate is a new class of materials which exhibits the
quantum topological order. In order to answer the important question, "how
useful is the string-net condensate in quantum information processing?", we
consider the most basic example of the string-net condensate, namely the
gauge string-net condensate on the two-dimensional hexagonal lattice, and show
that the universal measurement-based quantum computation (in the sense of the
quantum computational webs) is possible on it by using the framework of the
quantum computational tensor network. This result implies that even the most
basic example of the string-net condensate is equipped with the correlation
space that has the capacity for the universal quantum computation.Comment: 5 pages, 4 figure
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