Neutrino mass and mixing constrained from the LMC supernova burst

J. Arafune; M. Fukugita; T. Yanagida; M. Yoshimura

doi:10.1016/0370-2693(87)90220-6

Neutrino mass and mixing constrained from the LMC supernova burst

J. Arafune, M. Fukugita, T. Yanagida, M. Yoshimura

Research output: Contribution to journal › Article › peer-review

28 Citations (Scopus)

Abstract

Observation of the prompt neutronization burst by Kamiokande II is shown to constrain the mixing parameter sin²θ{symbol} of a 10-100 eV mass range neutrino less than 10^-7, implying that the neutrino is unlikely to provide the critical mass of the universe except in a special case of a neutrino decoupled from other lighter neutrinos. Model dependent bounds on neutrino masses are also given for a class of neutrino mixing models.

Original language	English
Pages (from-to)	477-481
Number of pages	5
Journal	Physics Letters B
Volume	194
Issue number	4
DOIs	https://doi.org/10.1016/0370-2693(87)90220-6
Publication status	Published - Aug 20 1987
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/0370-2693(87)90220-6

Cite this

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title = "Neutrino mass and mixing constrained from the LMC supernova burst",

abstract = "Observation of the prompt neutronization burst by Kamiokande II is shown to constrain the mixing parameter sin2θ{symbol} of a 10-100 eV mass range neutrino less than 10-7, implying that the neutrino is unlikely to provide the critical mass of the universe except in a special case of a neutrino decoupled from other lighter neutrinos. Model dependent bounds on neutrino masses are also given for a class of neutrino mixing models.",

author = "J. Arafune and M. Fukugita and T. Yanagida and M. Yoshimura",

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T1 - Neutrino mass and mixing constrained from the LMC supernova burst

AU - Arafune, J.

AU - Fukugita, M.

AU - Yanagida, T.

AU - Yoshimura, M.

PY - 1987/8/20

Y1 - 1987/8/20

N2 - Observation of the prompt neutronization burst by Kamiokande II is shown to constrain the mixing parameter sin2θ{symbol} of a 10-100 eV mass range neutrino less than 10-7, implying that the neutrino is unlikely to provide the critical mass of the universe except in a special case of a neutrino decoupled from other lighter neutrinos. Model dependent bounds on neutrino masses are also given for a class of neutrino mixing models.

AB - Observation of the prompt neutronization burst by Kamiokande II is shown to constrain the mixing parameter sin2θ{symbol} of a 10-100 eV mass range neutrino less than 10-7, implying that the neutrino is unlikely to provide the critical mass of the universe except in a special case of a neutrino decoupled from other lighter neutrinos. Model dependent bounds on neutrino masses are also given for a class of neutrino mixing models.

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Neutrino mass and mixing constrained from the LMC supernova burst

Abstract

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