Abstract
We have learned a great deal from the neutrino observations[l,2] of the stellar collapse SN1987A in the LMC. In particular we have a much better idea about the time structure, energy spectrum and neutrino content of a stellar collapse neutrino burst. These factors can be taken into account in the design of future experiments.
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References
R.M. Bionta, et al, Phys. Rev. Lett. 58, 1494 (1987)
C.B. Bratton, et al., Phys. Rev. D37, 3361 (1988).
K. Hirata, et al, Phys. Rev. Lett. 58, 1490 (1987)
K. Hirata, et al, Phys. Rev. Lett. D37, 3361 (1988)
T.D. Lee and C.N. Yang, Phys. Rev. 126, 2239 (1962)
S. Bonetti, et al, Nuov. Cim. 38, 38 (1977)
C. Llewellyn-Smith, Phys. Rep. 3C, 261 (1972).
S.A. Bludman and P.J. Schinder, Ap. J. 326, 265 (1988)
I. Goldman et al., Phys, Rev. Lett. 60 1789 (1988)
J.M. LoSecco, Phys. Rev. D39, 1013, (1989).
H.-T. Janka, this conference.
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LoSecco, J. (1991). Implications of SN 1987A Neutrino Observations for Future Detections. In: Woosley, S.E. (eds) Supernovae. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2988-9_61
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DOI: https://doi.org/10.1007/978-1-4612-2988-9_61
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