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Upper limits on the observational effects of nuclear pasta in neutron stars
relativity – gravitational waves – dense matter – stars neutron – stars
2011/7/21
The effects of the existence of exotic nuclear shapes at the bottom of the neutron star inner crust - nuclear `pasta' - on observational phenomena are estimated by comparing the limiting cases that th...
QHD equation of state for strongly magnetized neutron stars
QHD equation strongly magnetized neutron stars
2011/7/21
We investigate the quantum hadrodynamic equation of state for neutron stars (with and without including hyperons) in the presence of strong magnetic fields.
Oscillations of hot, young neutron stars: Gravitational wave frequencies and damping times
Oscillations of hot young neutron stars
2011/7/21
We study how the frequencies and damping times of oscillations of a newly born, hot proto-neutron star depend on the physical quantities which characterize the star quasi-stationary evolution which fo...
Energy release from hadron-quark phase transition in neutron stars and the axial $w$-mode of gravitational waves
Energy release hadron-quark phase transition neutron stars axial $w$-mode of gravitational waves
2011/1/7
Describing the hyperonic and quark phases of neutron stars with an isospin- and momentum-
dependent effective interaction for the baryon octet and the MIT bag model, respectively, and using the Gibbs...
Influence of the nuclear equation of state on the hadron-quark phase transition in neutron stars
hadron-quark phase transition equation of state neutron stars
2009/8/14
We study the hadron-quark phase transition in the interior of neutron stars, and examine the influence of the nuclear equation of state on the phase transition and neutron star properties. The relativ...
Influence of Interactions on Populations for Hyperons in Neutron
Stars
neutron star matter relativistic mean field hyperon population
hyperon coupling constant
2007/8/15
2004Vol.41No.2pp.269-272DOI:
Influence of Interactions on Populations for Hyperons in Neutron
Stars
LIU Guang-Zhou,1,2 ZHAO En-Guang,2,3 LIU
Wei,1 and
SUN Bao-Xi2,4
1 ...