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

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Abstract

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

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Authors and Affiliations

  1. Institute for Physics and Engineering, Moscow, USSR

    D. N. Voskresensky & A. V. Senatorov

  2. Central Institute for Nuclear Research Rossendorf, Dresden, GDR

    B. Kaempfer

  3. Central Institute for Astrophysics, Potsdam, GDR

    H. J. Haubold

Authors
  1. D. N. Voskresensky
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  2. A. V. Senatorov
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  3. B. Kaempfer
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  4. H. J. Haubold
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Voskresensky, D.N., Senatorov, A.V., Kaempfer, B. et al. A possible explanation of the second neutrino burst from SN 1987A. Astrophys Space Sci 138, 421–424 (1987). https://doi.org/10.1007/BF00637864

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  • DOI: https://doi.org/10.1007/BF00637864

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