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Antikaon condensation in neutron star matter with strong magnetic fields
quark-meson coupling model antikaon condensation magnetic fields
2009/8/17
We study the influence of strong magnetic fields on antikaon condensation in neutron star matter using the quark-meson coupling (QMC) model. The QMC model describes a nuclear many-body system as nonov...
Influence of Model Parameters on Hadron-Quark Phase
Transition in Neutron Star Matter
phase transition equation of state mass-radius relation third family
2007/8/15
2006Vol.45No.3pp.505-510DOI:
Influence of Model Parameters on Hadron-Quark Phase
Transition in Neutron Star Matter
BAO Tmurbagan,1,2 LIU Guang-Zhou,1 and ZHU Ming-Feng1
...
Three-Body Force Effects on EOS of Asymmetric Nuclear Matter
and Proton Fraction in Neutron Star Matter
three-body force asymmetric nuclear matter isospin
2007/8/15
2003Vol.39No.4pp.439-446DOI:
Three-Body Force Effects on EOS of Asymmetric Nuclear Matter
and Proton Fraction in Neutron Star Matter
ZUO Wei,1 A. Lejeune,2 U. Lombardo,3 and J.F.
...
Neutron Star Matter Including Delta Isobars
neutron star matter relativistic mean field equation of state
pion condensation
2007/8/15
2004Vol.42No.1pp.99-102DOI:
Neutron Star Matter Including Delta Isobars
LIU Guang-Zhou,1,2 LIU
Wei,1 and ZHAO
En-Guang2
1 Center for Theoretical Physics and Departmen...
Effect of Mesons f0(975) and $\phi(1020)$ and Variety of $U_\Xi^{(N)}$ on Properties of Neutron Star Matter
neutron star equation of state
2007/8/15
2004Vol.41No.3pp.441-446DOI:
Effect of Mesons f0(975) and $\phi(1020)$ and Variety of $U_\Xi^{(N)}$ on Properties of Neutron Star Matter
TAN Yu-Hong,1 SUN Bao-Xi,2 LI Lei,3 and...