179 research outputs found
Superluminal pions in a hadronic fluid
We study the propagation of pions at finite temperature and finite chemical
potential in the framework of the linear sigma model with 2 quark flavors and
colors. The velocity of massless pions in general differs from that of
light. One-loop calculations show that in the chiral symmetry broken phase
pions, under certain conditions, propagate faster than light.Comment: 8 pages, 3 figures included. Considerably revised, discussions
expanded, one figure added, typos corrected, results unchanged. To be
published in Phys. Rev.
General-Relativistic Thomas-Fermi model
A system of self-gravitating massive fermions is studied in the framework of
the general-relativistic Thomas-Fermi model. We study the properties of the
free energy functional and its relation to Einstein's field equations. A
self-gravitating fermion gas we then describe by a set of Thomas-Fermi type
self-consistency equations.Comment: 7 pages, LaTex, to appear in Gen. Rel. Gra
Is there a Supermassive Black Hole at the Center of the Milky Way?
This review outlines the observations that now provide an overwhelming
scientific case that the center of our Milky Way Galaxy harbors a supermassive
black hole. Observations at infrared wavelength trace stars that orbit about a
common focal position and require a central mass (M) of 4 million solar masses
within a radius of 100 Astronomical Units. Orbital speeds have been observed to
exceed 5,000 km/s. At the focal position there is an extremely compact radio
source (Sgr A*), whose apparent size is near the Schwarzschild radius
(2GM/c^2). This radio source is motionless at the ~1 km/s level at the
dynamical center of the Galaxy. The mass density required by these observations
is now approaching the ultimate limit of a supermassive black hole within the
last stable orbit for matter near the event horizon.Comment: Invited review submitted to International Journal of Modern Physics
D; 23 pages; 10 figure
Ghost Condensate Busting
Applying the Thomas-Fermi approximation to renormalizable field theories, we
construct ghost condensation models that are free of the instabilities
associated with violations of the null-energy condition.Comment: 9 pages, minor corrections, a reference added, the discussion on
consistency of the Thomas-Fermi approximation expanded, to appear in JCA
Generalized Chaplygin Gas Model: Dark Energy - Dark Matter Unification and CMBR Constraints
The generalized Chaplygin gas (GCG) model allows for an unified description
of the recent accelerated expansion of the Universe and the evolution of energy
density perturbations. This dark energy - dark matter unification is achieved
through an exotic background fluid whose equation of state is given by , where is a positive constant and .
Stringent constraints on the model parameters can be obtained from recent WMAP
and BOOMERanG bounds on the locations of the first few peaks and troughs of the
Cosmic Microwave Background Radiation (CMBR) power spectrum as well as SNe Ia
data.Comment: 9 pages, 2 figures; essay selected for an honorable mention by the
Gravity Research Foundation, 200
Chiral-symmetry restoration in the linear sigma model at nonzero temperature and baryon density
We study the chiral phase transition in the linear sigma model with 2 quark
flavors and colors. One-loop calculations predict a first-order phase
transition at both and . We also discuss the phase diagram
and make a comparison with a thermal parametrization of existing heavy-ion
experimental data.Comment: 12 pages, 6 ps-figures, LaTe
Quenched QCD at finite density
Simulations of quenched at relatively small but {\it nonzero} chemical
potential on lattices indicate that the nucleon
screening mass decreases linearly as increases predicting a critical
chemical potential of one third the nucleon mass, , by extrapolation.
The meson spectrum does not change as increases over the same range, from
zero to . Past studies of quenched lattice QCD have suggested that
there is phase transition at . We provide alternative
explanations for these results, and find a number of technical reasons why
standard lattice simulation techniques suffer from greatly enhanced
fluctuations and finite size effects for ranging from to
. We find evidence for such problems in our simulations, and suggest
that they can be surmounted by improved measurement techniques.Comment: 23 pages, Revte
Comment on "Quantum Scattering of Heavy Particles from a 10 K Cu(111) Surface"
In the original paper Althoff et al. (see ibid., vol.79, p.4429 (1997))
reported a study of scattering of thermal Ne, Ar, and Kr atoms from a Cu(111)
surface in which they assessed the corresponding Debye-Waller factor (DWF) as a
function of the particle mass m in a wide range of substrate temperature T. The
experiments were interpreted by the semiclassical DWF theory in which the
projectile moves on the classical recoilless trajectory and the surface
vibrations are quantized. Siber and Gumhalter claim that the experiments
described by Althoff et al. were carried out in the quantum scattering regime
in which the semiclassical scalings of Althoff et al. do not hold and the
semiclassical DWE significantly deviates from the exact quantum one both in the
low and high T limits. Hence, it is claimed, the quantum scattering data of
Althoff et al. cannot be reliably interpreted by the semiclassical theory.Comment: 1 page (2 figures) - comment in Phys. Rev. Let
Transition from a quark-gluon plasma in the presence of a sharp front
The effect of a sharp front separating the quark-gluon plasma phase from the
hadronic phase is investigated. Energy-momentum conservation and baryon number
conservation constrain the possible temperature jump across the front. If one
assumes that the temperature in the hadronic phase is 200 MeV , as
has been suggested by numerous results from relativistic ion collisions, one
can determine the corresponding temperature in the quark phase with the help of
continuity equations across the front. The calculations reveal that the quark
phase must be in a strongly supercooled state. The stability of this solution
with respect to minor modifications is investigated. In particular the effect
of an admixture of hadronic matter in the quark phase (e.g. in the form of
bubbles) is considered in detail. In the absence of admixture the transition
proceeds via a detonation transition and is accompanied by a substantial
super-cooling of the quark-gluon plasma phase. The detonation is accompanied by
less supercooling if a small fraction of bubbles is allowed. By increasing the
fraction of bubbles the supercooling becomes weaker and eventually the
transition proceeds via a smoother deflagration wave.Comment: 10 pages, manuscript in TeX, 9 figures available as Postscript files,
CERN-TH 6923/9
Effect of Helicobacter Pylori Eradication on Extent of Duodenal Gastric Metaplasia and Grade of Gastritis
The extent of the regression of duodenal gastric metaplasia (DGM) after the eradication
of Helicobacter pylori infection is controversial. Therefore, we decided to assess the
degree of DGM before, sex weeks and one year after H. pylori eradication. 105 consecutive
Helicobacter pylori positive patients with endoscopically proven duodenal ulcer,
with DGM and Helicobacter pylori infection were recruited for this study. The diagnosis
of Helicobacter pylori infection was based on CLO-test and histology, and DGM was assessed
on four bulb biopsies taken before, sex weeks and one year after Helicobacter
pylori eradication. Histological assessment of Helicobacter pylori associated gastritis
was performed according to the Sydney classification. Follow up study on 98 patients
before, six weeks and one year after the eradication of Helicobacter pylori showed that
the mean extent of DGM did not change significantly after eradication and did not differ
when compared with 14 patients with persisting infection. Our results show that the
inflammatory process related to Helicobacter pylori does not play the main role in the
development of DGM
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