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Properties of a proto-neutron star with smeared trapped neutrinos

Authors
Ryu, C. Y.Maruyama, TomoyukiKajino, ToshitakaCheoun, Myung-Ki
Issue Date
26-Jan-2011
Publisher
AMER PHYSICAL SOC
Citation
PHYSICAL REVIEW C, v.83, no.1
Journal Title
PHYSICAL REVIEW C
Volume
83
Number
1
URI
http://scholarworks.bwise.kr/ssu/handle/2018.sw.ssu/13735
DOI
10.1103/PhysRevC.83.018802
ISSN
0556-2813
Abstract
We investigate the structure of a proto-neutron star with trapped neutrinos by using quantum hadrodynamics. Ratios of the trapped neutrinos and corresponding leptons to the baryons are usually assumed to be constant. But relevant reactions associated with the beta equilibrium could be sensitive to the given density and temperature. By adopting a phenomenological lepton density that is smeared near the surface, we calculate and discuss populations of baryons and leptons, equations of state, and the mass-radius relation of a proto-neutron star in an isentropic process.
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