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Leinson, L.B.; Pérez Cañellas, Armando | |||
Aquest document és un/a article, creat/da en: 2006 | |||
Este documento está disponible también en : 10.1016/j.physietb.2006.05.036 |
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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. | |||
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