January 2012
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26 Reads
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2 Citations
International Journal of Modern Physics D
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, we derive a new equation of state for neutronic matter. By introducing it in the Tolman-Oppenheimer-Volkof equations we derive the masses and radii of neutron stars as a function of the central density. We obtain a maximum mass M max ≃2.7 M ʘ and a minimum period of rotation T min =0.8 msec.