A simple model for neutrino cooling of the Large Magellanic Cloud supernova

Details A simple model for neutrino cooling of the Large Magellanic Cloud supernova A simple model for neutrino cooling of the Large Magellanic Cloud supernova

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sci...237.1471s&link_type=abstract

Science (ISSN 0036-8075), vol. 237, Sept. 18, 1987, p. 1471-1473.

Physics

23

Cooling, Magellanic Clouds, Neutrinos, Stellar Models, Supernovae, Antineutrinos, Black Body Radiation, Hot Stars, Neutron Stars

Scientific paper

A simplified analytical model of a cooling hot neutron star is presented which describes the neutrinos detected from the recent supernova in the LMC. The model accounts for all of the observational data and provides an estimate of the radius of the hot neutron star. While the supernova has confirmed the general picture of core collapse, it has not provided sufficient data to discriminate between equations of state or to validate specific detailed models.

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