Physics – Nuclear Physics – Nuclear Theory
Scientific paper
2010-03-19
Phys.Rev.C81:055805,2010
Physics
Nuclear Physics
Nuclear Theory
7 pages, 6 figures, version to appear in Phys. Rev. C
Scientific paper
10.1103/PhysRevC.81.055805
Using the momentum-dependent MDI effective interaction for nucleons, we have studied the transition density and pressure at the boundary between the inner crust and liquid core of hot neutron stars. We find that their values are larger in neutrino-trapped neutron stars than in neutrino-free neutron stars. Furthermore, both are found to decrease with increasing temperature of a neutron star as well as increasing slope parameter of the nuclear symmetry energy, except that the transition pressure in neutrino-trapped neutron stars for the case of small symmetry energy slope parameter first increases and then decreases with increasing temperature. We have also studied the effect of the nuclear symmetry energy on the critical temperature above which the inner crust in a hot neutron star disappears and found that with increasing value of the symmetry energy slope parameter, the critical temperature decreases slightly in neutrino-trapped neutron stars but first decreases and then increases in neutrino-free neutron stars.
Chen Lie-Wen
Ko Che Ming
Li Bao-An
Xu Jun
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