2018/07/31 by P. S. Shternin, M. Baldo, P. Haensel · 1 citation
Physics and Astronomy · #astro-ph.HE #nucl-th
paper · pdf · doi:10.1016/j.physletb.2018.09.035
published as Physics Letters B 786, 28-34 (2018) · 8 pages, 3 figures; accepted for publication in PLB. In v.2 misprint in eq.(9) corrected and discussion of cooling curves expanded
arxiv created 2018/09/18 · arxiv updated 2018/09/25
We calculate modified Urca neutrino emission rates in the dense nuclear matter in neutron star cores. We find that these rates are strongly enhanced in the beta-stable matter in regions of the core close to the direct Urca process threshold. This enhancement can be tracked to the use of the in-medium nucleon spectrum in the virtual nucleon propagator. We describe the in-medium nucleon scattering in the non-relativistic Bruckner-Hartree-Fock framework taking into account two-body as well as the effective three-body forces, although the proposed enhancement does not rely on a particular way of the nucleon interaction treatment. Finally we suggest a simple approximate expression for the emissivity of the n-branch of the modified Urca process that can be used in the neutron stars cooling simulations with any nucleon equation of state of dense matter.