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Prog. Theor. Phys. Vol. 80 No. 5 (1988) pp. 861-867

[ Full Text PDF : FREE ACCESS (421K) ]

Phase Transitions in the Newly-Born Neutron Star and Neutrino Emissions from SN1987A

Mariko Takahara and Katsuhiko Sato*

Department of Physics, Tokyo Institute of Technology, Tokyo 152
*Department of Physics, University of Tokyo, Tokyo 113

(Received July 4, 1988)

Abstract:

We investigated the possibility that the last three events detected by Kamiokande-II can be explained by the phase transitions occurred in the neutron stars just born. We found that, if the equation of state of neutron stars is stiff enough, the last three neutrino events can be explained by the enhanced neutrino emission from the neutron star reheated by phase transitions.


URL : http://ptp.ipap.jp/link?PTP/80/861/
DOI : 10.1143/PTP.80.861

[ Full Text PDF : FREE ACCESS (421K) ] Citation:

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Citing Article(s) :

  1. Progress of Theoretical Physics Vol. 83 No. 3 (1990) pp. 499-521 :
    Static and Dynamical Properties of Neutron Stars with Combined π0-πc Condensation
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  2. Progress of Theoretical Physics Vol. 86 No. 1 (1991) pp. 57-71 :
    Phase Transition of Hot Neutron Matter to π0-Condensed State
    Mariko Takahara, Tatsuyuki Takatsuka and Katsuhiko Sato
  3. Progress of Theoretical Physics Vol. 92 No. 4 (1994) pp. 779-802 :
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  4. Progress of Theoretical Physics Supplement No. 186 (2010) pp. 87-92 :
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  5. Progress of Theoretical Physics Supplement No. 186 (2010) pp. 93-98 :
    Can a Supernova Bang Twice?
    Jürgen Schaffner-Bielich, Tobias Fischer, Matthias Hempel, Matthias Liebendörfer, Giuseppe Pagliara and Irina Sagert

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