88 research outputs found
In-Medium Hadronic Interactions and the Nuclear Equation of State
Microscopic studies of nuclear matter under diverse conditions of density and
asymmetry are of great contemporary interest. Concerning terrestrial
applications, they relate to future experimental facilities that will make it
possible to study systems with extreme neutron-to-proton ratio. In this talk, I
will review recent efforts of my group aimed at exploring nuclear interactions
in the medium through the nuclear equation of state (EoS). The approach we take
is microscopic and relativistic, with the predicted EoS properties derived from
realistic nucleon-nucleon potentials. I will also discuss work in progress.
Most recently, we completed a DBHF calculation of the hyperon binding
energy in nuclear matter.Comment: Talk given at the International Symposium on Exotic States of Nuclear
Matter, Catania (Italy), June 11-15, 2007. 9 pages, 5 figure
The mean free path of protons and neutrons in isospin-asymmetric nuclear matter
We calculate the mean free path of protons and neutrons in symmetric and
asymmetric nuclear matter, based on microscopic in-medium nucleon-nucleon cross
sections. Those are obtained from calculations of the G-matrix including
relativistic "Dirac" effects. The dependence of the mean free path on energy
and isospin asymmetry is discussed. We conclude by suggesting possible ways our
microscopic predictions may be helpful in conjunction with studies of rare
isotopes.Comment: Revised, extended, 9 pages, 4 figure
Triton Binding Energy and Minimal Relativity
For relativistic three-body calculations, essentially two different
approaches are in use: field theory and relativistic direct interactions.
Results for relativistic corrections of the triton binding energy obtained from
the two approaches differ even in their sign, which is rather puzzling. In this
paper, we discuss the origin of such discrepancy. We show that the use of an
invariant two-body amplitude, as done in the field-theoretic approach,
increases the triton binding energy by about 0.30 MeV. This may explain a large
part of the discrepancy.Comment: 11 pages, LaTeX, no figure
More on nucleon-nucleon cross sections in symmetric and asymmetric matter
Following a recent work, we present numerical results for total two-nucleon
effective cross sections in isospin symmetric and asymmetric matter. The
present calculations include the additional effect of Pauli blocking of the
final states.Comment: 9 pages, no figures, 5 table
The impact of charge symmetry and charge independence breaking on the properties of neutrons and protons in isospin-asymmetric nuclear matter
We investigate the effects of charge independence and charge symmetry
breaking in neutron-rich matter. We consider neutron and proton properties in
isospin-asymmetric matter at normal densities as well as the high-density
neutron matter equation of state and the bulk properties of neutron stars. We
find charge symmetry and charge independence breaking effects to be very small.Comment: 6 pages, 8 figure
Relativistic predictions of spin observables for exclusive proton knockout reactions
Within the framework of the relativistic distorted wave impulse approximation
(DWIA), we investigate the sensitivity of complete sets of polarization
transfer observables for exclusive proton knockout from the 3s,
2d and 2d states in Pb, at an incident laboratory
kinetic energy of 202 MeV, and for coincident coplanar scattering angles
(, ), to different distorting optical potentials,
finite-range (FR) versus zero-range (ZR) approximations to the DWIA, as well as
medium-modified meson-nucleon coupling constants and meson masses. Results are
also compared to the nonrelativistic DWIA predictions based on the
Schr\"{o}dinger equation.Comment: Submitted for publication to Physicical Review C, 23 pages, 7 figure
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