Neutrino luminosity of the bubble phase layer in a hot neutron star.

Details Neutrino luminosity of the bubble phase layer in a hot neutron star. Neutrino luminosity of the bubble phase layer in a hot neutron star.

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jetpl..57..265l&link_type=abstract

JETP Lett., Vol. 57, No. 5, p. 265 - 269

Physics

Scientific paper

A new mechanism of neutrino emission is suggested for a newly born neutron star cooling. Nucleons emit neutrino pairs due to collisions with bubbles which exist inside the spherical layer of stellar matter from half nuclear to nuclear density. During the earliest stages of the nascent neutron star cooling the νμν¯μ pair luminosity of this rather thin spherical layer is on the order of 1053erg/s.

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