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Review Article
Open Access
Theoretical Prediction of Presupernova Neutrinos and Their Detection
- C. Kato1, K. Ishidoshiro2, and T. Yoshida3
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View Affiliations Hide AffiliationsAffiliations: 1Department of Aerospace Engineering, Tohoku University, Sendai 980-8579, Japan; email: [email protected] 2Research Center for Neutrino Science, Tohoku University, Sendai 980-8578, Japan; email: [email protected] 3Department of Astronomy, Graduate School of Science, University of Tokyo, Tokyo 113-0033, Japan; email: [email protected]
- Vol. 70:121-145 (Volume publication date October 2020) https://doi.org/10.1146/annurev-nucl-040620-021320
- First published as a Review in Advance on June 02, 2020
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Copyright © 2020 by Annual Reviews.This work is licensed under a Creative Commons Attribution 4.0 International License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. See credit lines of images or other third party material in this article for license information.
Abstract
More than 30 years have passed since the successful detection of supernova (SN) neutrinos from SN 1987A. In the last few decades, remarkable progress has been made in neutrino detection techniques, through which it may be possible to detect neutrinos from a new source, presupernova (pre-SN) neutrinos. They are emitted from a massive star prior to core bounce. Because neutrinos escape from the core freely, they carry information about the stellar physics directly. Pre-SN neutrinos may play an important role in verifying our understanding of stellar evolution for massive stars. Observation of pre-SN neutrinos, moreover, may serve as an alarm regarding an SN explosion a few days in advance if the progenitor is located in our vicinity, enabling us to observe the next galactic SN. In this review, we summarize the current status of pre-SN neutrino studies from both the theoretical and observational points of view.
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