%0 Journal Article
%T Hardon-Quark Hybrid Stars Constructed by the Nonlinear <em>¦Ò</em>-<em>¦Ø</em>-<em>¦Ñ</em> Mean-Field Model and MIT-Bag Model
%A Schun T. Uechi
%A Hiroshi Uechi
%J Open Access Library Journal
%V 2
%N 11
%P 1-16
%@ 2333-9721
%D 2015
%I Open Access Library
%R 10.4236/oalib.1102012
%X Density-dependent relations among saturation properties of symmetric
nuclear matter and hyperonic matter, properties of hadron-(strange) quark
hybrid stars are discussed by applying the conserving nonlinear <i>s</i>-<i>w</i>-<i>r</i> hadronic
mean-field theory. Nonlinear interactions that will be renormalized as
effective coupling constants, effective masses and sources of meson equations
of motion are constructed self-consistently by maintaining thermodynamic
consistency to the mean- field
approximation. The coupling constants expected from the hadronic mean-field
model and SU (6) quark model for the vector coupling constants are compared;
the coupling constants exhibit different density-dependent results for effective
masses and binding energies of hyperons, properties of hadron and hadron-quark
stars. The nonlinear <i>s</i>-<i>w</i>-<i>r</i> hadronic
mean-field approximation with or without vacuum fluctuation corrections and
strange quark matter defined by MIT-bag model are employed to examine
properties of hadron-(strange) quark hybrid stars. The hadron- (strange) quark hybrid
stars become more stable at high densities compared to pure hadronic and pure
strange quark stars.
%K Nonlinear <i>¦Ò</i>-<i>¦Ø</i>-<i>¦Ñ</i> Mean-Field
%K Hyperon Onset Densities
%K Hyperon Coupling Ratios
%K Hadron-Quark Hybrid Stars
%U http://www.oalib.com/paper/3151190