A possible explanation of the second neutrino burst from SN 1987a

Details A possible explanation of the second neutrino burst from SN 1987a A possible explanation of the second neutrino burst from SN 1987a

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.138..421v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 138, no. 2, Nov. 1987, p. 421-424. Research supported by the Akademie der

Astronomy and Astrophysics

Astrophysics

5

Bursts, Magellanic Clouds, Neutrinos, Neutron Stars, Stellar Evolution, Supernova 1987A, Density Distribution, Stellar Models

Scientific paper

It is argued that the neutrino bursts registered on February 23.316 UT,
1987 signalized the transition of a newborn neutron star into a
superdense state. The neutron star is assumed to have been formed
approximately five hours before at February 23.12 UT in the supernova SN
1987a in the Large Magellanic Cloud.

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