1,569 research outputs found
A search for inverse magnetic catalysis in thermal quark-meson models
We explore the parameter space of the two-flavor thermal quark-meson model
and its Polyakov loop-extended version under the influence of a constant
external magnetic field . We investigate the behavior of the pseudo critical
temperature for chiral symmetry breaking taking into account the likely
dependence of two parameters on the magnetic field: the Yukawa quark-meson
coupling and the parameter of the Polyakov loop potential. Under the
constraints that magnetic catalysis is realized at zero temperature and the
chiral transition at is a crossover, we find that the quark-meson model
leads to thermal magnetic catalysis for the whole allowed parameter space, in
contrast to the present picture stemming from lattice QCD.Comment: 8 pages, 5figure
On thermal nucleation of quark matter in compact stars
The possibility of a hadron-quark phase transition in extreme astrophysical
phenomena such as the collapse of a supernova is not discarded by the modern
knowledge of the high-energy nuclear and quark-matter equations of state. Both
the density and the temperature attainable in such extreme processes are
possibly high enough to trigger a chiral phase transition. However, the time
scales involved are an important issue. Even if the physical conditions for the
phase transition are favorable (for a system in equilibrium), there may not be
enough time for the dynamical process of phase conversion to be completed. We
analyze the relevant time scales for the phase conversion via thermal
nucleation of bubbles of quark matter and compare them to the typical
astrophysical time scale, in order to verify the feasibility of the scenario of
hadron-quark phase conversion during, for example, the core-collapse of a
supernova.Comment: 6 pages, 4 figures, talk given at the International Conference
SQM2009, Buzios, Rio de Janeiro, Brazil, Sep.27-Oct.2, 200
Nucleation of quark matter in protoneutron star matter
The phase transition from hadronic to quark matter may take place already
during the early post-bounce stage of core collapse supernovae when matter is
still hot and lepton rich. If the phase transition is of first order and
exhibits a barrier, the formation of the new phase occurs via the nucleation of
droplets. We investigate the thermal nucleation of a quark phase in supernova
matter and calculate its rate for a wide range of physical parameters. We show
that the formation of the first droplet of a quark phase might be very fast and
therefore the phase transition to quark matter could play an important role in
the mechanism and dynamics of supernova explosions.Comment: v3: fits version published in Physical Review
The universal character of Zwanziger's horizon function in Euclidean Yang-Mills theories
In light of the recently established BRST invariant formulation of the
Gribov-Zwanziger theory, we show that Zwanziger's horizon function displays a
universal character. More precisely, the correlation functions of local BRST
invariant operators evaluated with the Yang-Mills action supplemented with a
BRST invariant version of the Zwanziger's horizon function and quantized in an
arbitrary class of covariant, color invariant and renormalizable gauges which
reduce to the Landau gauge when all gauge parameters are set to zero, have a
unique, gauge parameters independent result, corresponding to that of the
Landau gauge when the restriction to the Gribov region in the latter
gauge is imposed. As such, thanks to the BRST invariance, the cut-off at the
Gribov region acquires a gauge independent meaning in the class of the
physical correlators.Comment: 14 pages. v2: version accepted by Phys.Lett.
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