On Massive Neutron Cores

Details On Massive Neutron Cores On Massive Neutron Cores

Feb 1939

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1939phrv...55..374o&link_type=abstract

Physical Review, vol. 55, Issue 4, pp. 374-381

Physics

766

Scientific paper

It has been suggested that, when the pressure within stellar matter becomes high enough, a new phase consisting of neutrons will be formed. In this paper we study the gravitational equilibrium of masses of neutrons, using the equation of state for a cold Fermi gas, and general relativity. For masses under 13solar only one equilibrium solution exists, which is approximately described by the nonrelativistic Fermi equation of state and Newtonian gravitational theory. For masses 13solar

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