Collective excitations in nucleonic matter and the problem of cooling of neutron stars

Details Collective excitations in nucleonic matter and the problem of cooling of neutron stars Collective excitations in nucleonic matter and the problem of cooling of neutron stars

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phlb..184..119s&link_type=abstract

Physics Letters B, Volume 184, Issue 2-3, p. 119-124.

Physics

18

Scientific paper

The problem of cooling of neutron stars is solved with inclusion of the collective effects in a dense nucleonic medium. The resulting neutrino emissivity exceeds that found previously. The neutrino opacity of the neutron stars is calculated. From the obtained results it is possible to explain the Einstein Observatory data assuming the presence of neutron stars in supernovae remnants.

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