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Nucleon effective masses within the Brueckner-Hartree-Fock theory: Impact on stellar neutrino emission

We calculate the effective masses of neutrons and protons in dense nuclear matter within the microscopic Brueckner-Hartree-Fock many-body theory and study the impact on the neutrino emissivity processes of neutron stars. We compare results based on different nucleon-nucleon potentials and nuclear three-body forces. Useful parametrizations of the numerical results are given. We find substantial in-medium suppression of the emissivities, strongly dependent on the interactions.

preprint2014arXivOpen access
M. BaldoG. F. BurgioH. -J. SchulzeG. Taranto
nucl-thastro-ph.SR
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Open access4 authors2 topics
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M. BaldoG. F. BurgioH. -J. SchulzeG. Taranto

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