Articles
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08/25/1997--
08/25/1997
QCD Sum Rules and the Pi(1300) Resonance
Global fits to the shape of the first QCD Laplace sum rule exhibiting
sensitivity to pion-resonance [$\Pi (1300)$] parameters are performed, leading
to predictions for the pion-resonance mass and decay constant. Two scenarios
are considered which differ only in their treatment of the dimension-six quark
condensate $< O_6>$. The first scenario assumes an effective scale for $< O_6>$
from other sum-rule applications which is assumed to be independent of the
physical value of the quark mass, while the second scenario requires
self-consistency between the value of $< O_6>$ and the current algebra
constraint $2m< \bar q q>=-f_\pi^2m_\pi^2$. Predictions of the pion-resonance
mass $M_\pi$ and decay constant $F_\pi$ are obtained in these two scenarios. A
byproduct of this analysis is a prediction of the renormalization-group
invariant quark mass $(\hat m_u+\hat m_d)/2$.
T. G. Steele
J. C. Breckenridge
M. Benmerrouche
V. Elias
A. H. Fariborz
04/29/2003--
04/29/2003
Strangeness Saturation: Dependence on System-Size, Centrality and Energy
The dependence of the strangeness saturation factor on the system size,
centrality and energy is studied in relativistic heavy-ion collisions.
B. Kampfer
J. Cleymans
P. Steinberg
S. Wheaton
04/15/2005--
04/15/2005
Direct Photon Measurement at RHIC-PHENIX
Results on direct photon measurements from the PHENIX experiment at RHIC are
presented. The direct photon yields for $p_T>$6 GeV/$c$ as a function of
centrality in Au-Au collisions at $\sqrt{s_{NN}}$=200 GeV are found to be
consistent with NLO pQCD calculation scaled by the number of binary collisions.
The results suggest that the photons observed are emitted from the initial
stage of hard scattering. Comparisons with several theoretical calculations are
also presented.
T. Sakaguchi
04/13/2009--
12/23/2008
Kerr/CFT correspondence and five-dimensional BMPV black holes
We apply a recently proposed Kerr/CFT correspondence to extremal
supersymmetric five-dimensional charged spinning black holes, constructed by
Breckenridge, Myers, Peet and Vafa. By computing the central charge of the dual
CFT and Frolov-Thorne temperature, Cardy's formula succeeds in reproducing
Bekenstein-Hawking area law.
Hiroshi Isono
Ta-Sheng Tai
Wen-Yu Wen
05/20/2005--
05/20/2005
High transverse momentum identified particle spectra in 200 GeV collisions from STAR
Significant baryon over meson enhancement was measured at RHIC in the
intermediate transverse momentum range of $p_T=2-4$ GeV/$c$ ("baryon-meson
puzzle"). With STAR detector we were able to extend particle identification
towards higher transverse momentum offering further insights into the particle
production mechanisms at intermediate to high $p_T$. In this paper we present
results on charged pion, proton and anti-proton spectra and ratios at
intermediate to high $p_T$ exploiting the relativistic rise of the specific
ionization energy loss measured in the STAR Time Projection Chamber. These
measurements provide valuable information about the production mechanisms of
particles at intermediate $p_T$ in relativistic heavy ion collisions, e.g.
coalescence/recombination versus jet fragmentation.
Olga Barannikova
04/25/2005--
04/25/2005
Triaxiality, chirality and gamma-softness
Current work explores the impact of gamma-softness on partner bands built on
the h11/2h11/2 proton-particle-neutron-hole configurations in triaxial odd-odd
nuclei. The results of calculations conducted using a core-particle-hole
coupling are presented. The model Hamiltonian includes the collective core, the
single-particle valence nucleons, and separable quadrupole-quadrupole
interactions. The Kerman-Klein method was applied to find eigenstates, which
provided a convenient way for exploring core effects. Calculations were made
for triaxial cores with various gamma-softness using the General Collective
Model keeping the expectation value for the triaxiality parameter fixed at
<gamma>=30 deg. The degeneracy in the proton-neutron h11/2h11/2 bands results
from the calculations for the gamma-rigid core but is lifted for the
gamma-unstable core.
K. Starosta
M. A. Caprio
T. Koike
R. Kruecken
C. Vaman
03/07/2000--
03/07/2000
A flexible framework for defeasible logics
Logics for knowledge representation suffer from over-specialization: while
each logic may provide an ideal representation formalism for some problems, it
is less than optimal for others. A solution to this problem is to choose from
several logics and, when necessary, combine the representations. In general,
such an approach results in a very difficult problem of combination. However,
if we can choose the logics from a uniform framework then the problem of
combining them is greatly simplified. In this paper, we develop such a
framework for defeasible logics. It supports all defeasible logics that satisfy
a strong negation principle. We use logic meta-programs as the basis for the
framework.
G. Antoniou
D. Billigton
G. Governatori
M. J. Maher
04/23/2003--
04/23/2003
Do Ordinary Nuclei Contain Exotic States of Matter?
The strongly repulsive core of the short-range nucleon-nucleon interaction
leads to the existence of high-momentum nucleons in nuclei. Inclusive electron
scattering can be used to probe these high-momentum nucleons and study the
nature of the corresponding short-range correlations in nuclei. With recent
data from Jefferson Lab we have begun to map out the strength of two-nucleon
correlations in nuclei, while upcoming experiments should allow us to isolate
the presence of multi-nucleon correlations. In addition to their importance in
describing nuclear structure, these configurations of correlated nucleons
represent high density 'droplets' of hadronic matter. As the density of
hadronic matter increases there should be a weakening of quark confinement,
similar to the onset of deconfinement expected at extremely high temperatures.
While there have been hints of non-hadronic structure in nuclei, future
measurements will allow us to directly probe the quark distributions of high
density configurations in nuclei. A modified quark structure in these closely
packed nucleons would provide a clear signature of exotic components to the
structure of nuclei.
J. Arrington
05/23/2005--
05/23/2005
Isospin Asymmetry in Nuclei, Neutron Stars, and Heavy-Ion Collisions
The roles of isospin asymmetry in nuclei and neutron stars are investigated
using a range of potential and field-theoretical models of nucleonic matter.
The parameters of these models are fixed by fitting the properties of
homogeneous bulk matter and closed-shell nuclei. We discuss and unravel the
causes of correlations among the neutron skin thickness in heavy nuclei, the
pressure of beta-equilibrated matter at a density of 0.1 fm$^{-3}$, and the
radii of moderate mass neutron stars. The influence of symmetry energy on
observables in heavy-ion collisions is summarized.
Andrew W. Steiner
Madappa Prakash
James M. Lattimer
Paul J. Ellis
08/20/1999--
06/14/1999
Supersymmetric Rotating Black Holes and Causality Violation
The geodesics of the rotating extreme black hole in five spacetime dimensions
found by Breckenridge, Myers, Peet and Vafa are Liouville integrable and may be
integrated by additively separating the Hamilton-Jacobi equation. This allows
us to obtain the St\"ackel-Killing tensor. We use these facts to give the
maximal analytic extension of the spacetime and discuss some aspects of its
causal structure. In particular, we exhibit a `repulson'-like behaviour
occuring when there are naked closed timelike curves. In this case we find that
the spacetime is geodesically complete (with respect to causal geodesics) and
free of singularities. When a partial Cauchy surface exists, we show, by
solving the Klein-Gordon equation, that the absorption cross-section for
massless waves at small frequencies is given by the area of the hole. At high
frequencies a dependence on the angular quantum numbers of the wave develops.
We comment on some aspects of `inertial time travel' and argue that such time
machines cannot be constructed by spinning up a black hole with no naked closed
timelike curves.
G. W. Gibbons
C. A. R. Herdeiro
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