Neutron Star in Relativistic Mean-field Approximation
- Received Date:1900-01-01
- Accepted Date:1900-01-01
- Available Online:2000-07-15
Abstract:The equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different couplings of the hyperons.The properties of neutron stars are studied by solving the Oppenheimer-Vollkoff equation.It shows that these properties change distinctly as different couplings of hyperons are concemed.

Abstract
HTML
Reference
Related
PDF










DownLoad: