Publication Date:
2012-02-10
Description:
Author(s): De-Hua Wen, W. G. Newton, and Bao-An Li Using a simple model of a neutron star with a perfectly rigid crust constructed with a set of crust and core equations of state that span the range of nuclear experimental uncertainty in the symmetry energy, we calculate the instability window for the onset of the Chandrasekhar-Friedmann-Schutz inst... [Phys. Rev. C 85, 025801] Published Thu Feb 09, 2012
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics