Effect of bulk constants on the binding energy of neutron matter and beta stability of a neutron star

Details Effect of bulk constants on the binding energy of neutron matter and beta stability of a neutron star Effect of bulk constants on the binding energy of neutron matter and beta stability of a neutron star

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvc..53..505r&link_type=abstract

Physical Review C (Nuclear Physics), Volume 53, Issue 1, January 1996, pp.505-507

Physics

Nuclear Physics

1

Binding Energies And Masses, Nuclear Forces, Nuclear Matter, Neutron Stars

Scientific paper

We have studied pure neutron matter using a derivative scalar coupling (DSC) model and different nonlinear models. It is found that small bound energy of pure neutron matter at equilibrium density is due to the high value of effective nucleon mass m*n in this model. Other nonlinear models having large m*n(ρ0) also yield bound neutron matter. It is also shown that the role of symmetry energy is very significant in the study of neutron matter and the beta stability of neutron matter.

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