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Three-dimensional calculation of inhomogeneous structure in low-density nuclear matter
low-density nuclear matter inhomogeneous structure
2011/7/20
In low-density nuclear matter which is relevant to the crust region of neutron stars and collapsing stage of supernovae, non-uniform structures called "nuclear pasta" are expected.
Flavor unification, dark matter, proton decay and other observable predictions with low-scale $S_4$ symmetry
Flavor symmetries Grand unification Proton decay Intermediate symmetry
2011/1/10
We show how gauge coupling unification is successfully implemented through non- supersym-
metric GU ×Gf (GU = SU(5), SO(10); Gf = S4 , SO(3)f , SU(3)f ) at the grand unification
scale MU > 1015 GeV ...
Study of various charged ρ-meson masses in asymmetric nuclear matter
asymmetric nuclear matter ρ-meson effective mass Dirac sea
2009/9/17
We study the effective masses of ρ-mesons for different charged states in asymmetric nuclear matter (ANM) using the Quantum Hadrodynamics II model. The closed form analytical results are presented for...
Properties of Cold and Hot Polarized Nuclear Matter with Realistic Nucleon Nucleon Interaction
nuclear-matter Hartree-Fock equation of state
2010/4/13
The Thomas-Fermi (TF) model is used to calculate the equation of state ofthermal polarized nuclear-matter (NM) within a nonrelativistic Hartree-Fock (HF) scheme. The potential employed is a new realis...