Neutrino Burst from Supernovae and the Implications for Neutrino Oscillation Parameters

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概要

• 論文の詳細を見る

• It was shown that neutrinos have finite masses and convert each other from the solar and atmospheric neutrino observations. The time profile and energy spectrum of neutrino burst from supernovae should be greatly modified by this effect. We review how this conversion happens in a supernova mantle and how the burst will be detected by SK (Super-Kamiokande) and SNO (Sudbury Neutrino Observatory). We show that implications for neutrino parameters (mass hierarchy and the mixing angle between mass eigenstate ν_1,ν_3), are obtained if a supernova appears at Galactic Center. We also discuss effects of neutrino oscillation on the supernova relic neutrino observations.

• 理論物理学刊行会の論文
• 2003-10-15

著者

• SATO Katsuhiko

  Department of Physics, Kyoto University

• Ando Shin'ichiro

  Department Of Physics School Of Science University Of Tokyo

• TAKAHASHI Keitaro

  Department of Physics, School of Science, University of Tokyo

• Takahashi Kazuyoshi

  Yukawa Institute For Theoretical Physics Kyoto University

• Takahashi K

  Tohoku Gakuin Univ. Sendai Jpn

• Takahashi Keitaro

  Department Of Orthodontics School Of Dentistry At Tokyo Nippon Dental University

• Takahashi Keitaro

  Department Of Physics University Of Tokyo

• Sato Katsuhiko

  Department Of Cardiovascular Medicine Hokkaido University School Of Medicine

• Takahashi K

  Department Of Energy & Safety Engineering Yokohama National University

• TAKAHASHI Koichi

  Department of Liberal Arts, Tohoku Gakuin University

• TAKAHASHI Koichi

  Physics Department, Faculty of Science Tohoku University

• TAKAHASHI Koichi

  College of Liberal Arts, Tohoku Gakuin University

• Koi SATO

  Department of Physics, Nagoya University

• SATO Katsuhiko

  Research Center for the Early Universe (RESCEU), School of Science, University of Tokyo:Departrment of Physics, Scool of Science, University of Tokyo

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