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Pre-SN neutrino emissions from ONe cores in the progenitors of CCSNe

Published online by Cambridge University Press:  28 July 2017

Chinami Kato ,
S. Yamada ,
H. Nagakura ,
S. Furusawa ,
K. Takahashi ,
H. Umeda ,
T. Yoshida  and
K. Ishidoshiro
Chinami Kato
Affiliation:
School of Advanced Science and Engineering, Waseda University, Japan
S. Yamada
Affiliation:
School of Advanced Science and Engineering, Waseda University, Japan Advanced Research Institute for Science and Engineering, Waseda University, Japan
H. Nagakura
Affiliation:
TAPIR, Walter Burke Institute for Theoretical Physics, California Institute of Technology, USA
S. Furusawa
Affiliation:
Frankfurt Institute for Advanced Studies, J.W. Goethe University, Germany
K. Takahashi
Affiliation:
Department of Astronomy, The University of Tokyo, Japan
H. Umeda
Affiliation:
Department of Astronomy, The University of Tokyo, Japan
T. Yoshida
Affiliation:
Department of Astronomy, The University of Tokyo, Japan
K. Ishidoshiro
Affiliation:
Research Center for Neutrino Science, Tohoku University, Japan
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Abstract

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In order to investigate the distinguishability about the progenitors of FeCCSNe and ECSNe, we calculate the luminosities and spectra of their pre-SN neutrinos and estimate the number of events at neutrino detectors.

Keywords

Supernovae:generalneutrinos
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 411
Copyright
Copyright © International Astronomical Union 2017 

References

Kato, C., Yamada, S., Nagakura, H., Furusawa, S., Takahashi, K., Umeda, H., Yoshida, T., & Ishidoshiro, K., 2017, in preparationGoogle Scholar
Takahashi, K., Yoshida, T., & Umeda, H., 2013, ApJ, 771, 28 Google Scholar
Nagakura, H., Sumiyoshi, K., & Yamada, S., 2014, ApJS, 214, 16 CrossRefGoogle Scholar