Neutron star accretion in dense environments.

Details Neutron star accretion in dense environments. Neutron star accretion in dense environments.

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phr...256...95c&link_type=abstract

Physics Reports, Vol. 256, No. 1 - 3, p. 95 - 108

Physics

3

Neutron Stars: Accretion, Neutron Stars: Supernovae, Neutron Stars: Neutrinos

Scientific paper

For a neutron star in a dense environment, the gravitational energy of accreting matter can be lost to neutrinos. One such environment surrounds a newly formed neutron star in a supernova; for the conditions in SN 1987A, ⪉0.1 Msun may have fallen back onto the central neutron star on a timescale of hours after the explosion. The mass accretion rate subsequently drops more rapidly than t-1, but steady accretion solutions with an extended shocked envelope around the neutron star and neutrino emission close to the surface are possible.

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