Neutron star models and nuclear forces

Details Neutron star models and nuclear forces Neutron star models and nuclear forces

Feb 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971zphy..246...60h&link_type=abstract

Zeitschrift für Physik, Volume 246, Issue 1, pp.60-70

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Scientific paper

Equations of state of cold neutron matter are calculated by the method of unitary transformations for a hard-core and a soft-core potential. Equilibrium configurations are constructed in the Newtonian and the general relativistic theory of gravitation. It is found that Newtonian treatment to a certain extent gives very good results. On the other hand neutron star models are strongly affected by the nuclear forces used in the equation of state.

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