Neutron stars and the coherent nuclear interaction.

Details Neutron stars and the coherent nuclear interaction. Neutron stars and the coherent nuclear interaction.

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ijmpd...4..531d&link_type=abstract

International Journal of Modern Physics D, Vol. 4, No. 4, p. 531 - 548

Physics

1

Neutron Stars: Masses, Neutron Stars: Densities, Neutron Stars: Nuclear Reactions

Scientific paper

In the framework of a novel approach to the dynamics of nuclei and large collections of nucleons, which fully exploits the coherent interaction among π's, nucleons and Δ's, the authors derive a new equation of state for neutronic matter. By introducing it in the Tolman-Oppenheimer-Volkof equations they derive the masses and radii of neutron stars as a function of the central density. The authors obtain a maximum mass Mmax ≅ 2.7 Msun and a minimum period of rotation Tmin = 0.8 msec.

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