Vector current conservation and neutrino emission from singlet-paired baryons in neutron stars
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Vector current conservation and neutrino emission from singlet-paired baryons in neutron stars

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Vector current conservation and neutrino emission from singlet-paired baryons in neutron stars

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dc.contributor.author Leinson, L.B.
dc.contributor.author Pérez Cañellas, Armando
dc.date.accessioned 2014-02-18T12:03:27Z
dc.date.available 2014-02-18T12:03:27Z
dc.date.issued 2006
dc.identifier.uri http://dx.doi.org/10.1016/j.physietb.2006.05.036
dc.identifier.uri http://hdl.handle.net/10550/33036
dc.description.abstract Neutrino emission caused by singlet Cooper pairing of baryons in neutron stars is recalculated by accurately taking into account for conservation of the vector weak currents. The neutrino emissivity via the vector weak currents is found to be several orders of magnitude smaller than that obtained before by different authors. This makes unimportant the neutrino radiation from singlet pairing of protons or hyperons.
dc.relation.ispartof Physics Letters B, 2006, vol. 638, num. 2-3, p. 114-118
dc.rights.uri info:eu-repo/semantics/openAccess
dc.source Leinson, L.B. Pérez Cañellas, Armando 2006 Vector current conservation and neutrino emission from singlet-paired baryons in neutron stars Physics Letters B 638 2-3 114 118
dc.subject Partícules (Física nuclear)
dc.title Vector current conservation and neutrino emission from singlet-paired baryons in neutron stars
dc.type info:eu-repo/semantics/article
dc.date.updated 2014-02-18T12:03:27Z
dc.identifier.doi http://dx.doi.org/10.1016/j.physietb.2006.05.036
dc.identifier.idgrec 041265

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