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- W1988799230 abstract "We suggest that the period of the submillisecond optical pulsar in SN1987A is related to the pulsation period of the neutron star. A recent analysis of the arrival times of the neutrinos from the supernovae provides significant evidence of pulsed emission with a period equivalent to that of the pulsar. At first sight, an old theoretical model seems to account satisfactorily for this intriguing discovery: a cold, strongly pulsating neutron star created in the implosion of the core of the supernova would produce a pulsed emission of neutrinos of the observed energies; most of the neutrinos would be emitted during the first few seconds, as observed. However, there is a flaw in this theoretical model: the temperature of a cold, strongly pulsating neutron star should rapidly rise." @default.
- W1988799230 created "2016-06-24" @default.
- W1988799230 creator A5084943283 @default.
- W1988799230 date "1990-08-01" @default.
- W1988799230 modified "2023-10-18" @default.
- W1988799230 title "A neutrino pulsar in SN1987A?" @default.
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- W1988799230 doi "https://doi.org/10.1007/bf02741564" @default.
- W1988799230 hasPublicationYear "1990" @default.
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