Short-range nucleon correlations and neutrino emission by neutron stars

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dc.creatorFrankfurt, Leonid
dc.creatorStrikman, Mark
dc.date2008-06-05
dc.date2008-08-24
dc.date.accessioned2026-07-07T11:51:26Z
dc.date.available2026-07-07T11:51:26Z
dc.descriptionWe argue that significant probability of protons with momenta above their Fermi surface leads for proton concentrations p/n > 1/8 to the enhancement of termally excited direct and modified URCA processes within a cold neutron star, and to a nonzero probability of direct URCA processes for small proton concentrations (p/n < 1/8). We evaluate high momentum tails of neutron, proton and electrons distributions within a neutron star. We expect also significantly faster neutrino cooling of hyperon stars.
dc.description7 pages, updated version to be published in Proceedings of Sixth International Conference on Perspectives in Hadronic Physics, Trieste, May 2008
dc.identifierhttps://arxiv.org/abs/0806.0997
dc.identifierhttp://arxiv.org/abs/0806.0997
dc.identifierAIPConf.Proc.1056:241-247,2008
dc.identifierdoi:10.1063/1.3013048
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203901
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleShort-range nucleon correlations and neutrino emission by neutron stars
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