Summary
The energy release of the proto-neutron star by the diffusion of the neutrinos and the majoron-like particles is discussed. It is shown that the majoron neutrino coupling is constrained from the observed neutrino flux from SN 1987A. A possible way of extending the constraint is also briefly discussed.
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Presented at the Second Italian-Korean Meeting on Relativistic Astrophysics held at the University of Rome and in Limone Piemonte in July 1989.
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Kim, J. The diffusion of weakly interacting particles from the proto-neutron star. Nuovo Cim B 105, 835–844 (1990). https://doi.org/10.1007/BF02741551
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DOI: https://doi.org/10.1007/BF02741551