Neutrinos from Presupernova Stars

Takashi Yoshida; Koh Takahashi; Hideyuki Umeda; Koji Ishidoshiro

doi:10.1007/978-3-030-13876-9_26

Neutrinos from Presupernova Stars

Takashi Yoshida, Koh Takahashi, Hideyuki Umeda, Koji Ishidoshiro

Research Center for Neutrino Science (RCNS)

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

Neutrinos from a presupernova star will be observed by current and future neutrino detectors if a nearby supernova at a few hundred parsec from the earth occurs. The events of neutrinos produced through pair-neutrino process are expected to be a few to hundreds depending on stellar mass, neutrino mass hierarchy, and detectors. The neutrino events can be applied to an alarm of the supernova. The supernova alarm will be sent before a few to more than ten hours before the supernova explosion by KamLAND. If hundreds neutrino events are observed by JUNO, the time variation of the burning processes in the central core of the presupernova star can be analyzed from the neutrino events.

Original language	English
Title of host publication	Nuclei in the Cosmos XV
Editors	Alba Formicola, Matthias Junker, Lucio Gialanella, Gianluca Imbriani
Publisher	Springer Science and Business Media, LLC
Pages	157-161
Number of pages	5
ISBN (Print)	9783030138752
DOIs	https://doi.org/10.1007/978-3-030-13876-9_26
Publication status	Published - 2019
Event	15th International Symposium on Nuclei in the Cosmos, NIC 2018 - L'Aquila, Italy Duration: 2018 Jun 24 → 2018 Jun 29

Publication series

Name	Springer Proceedings in Physics
Volume	219
ISSN (Print)	0930-8989
ISSN (Electronic)	1867-4941

Conference

Conference	15th International Symposium on Nuclei in the Cosmos, NIC 2018
Country/Territory	Italy
City	L'Aquila
Period	18/6/24 → 18/6/29

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10.1007/978-3-030-13876-9_26

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title = "Neutrinos from Presupernova Stars",

abstract = "Neutrinos from a presupernova star will be observed by current and future neutrino detectors if a nearby supernova at a few hundred parsec from the earth occurs. The events of neutrinos produced through pair-neutrino process are expected to be a few to hundreds depending on stellar mass, neutrino mass hierarchy, and detectors. The neutrino events can be applied to an alarm of the supernova. The supernova alarm will be sent before a few to more than ten hours before the supernova explosion by KamLAND. If hundreds neutrino events are observed by JUNO, the time variation of the burning processes in the central core of the presupernova star can be analyzed from the neutrino events.",

author = "Takashi Yoshida and Koh Takahashi and Hideyuki Umeda and Koji Ishidoshiro",

note = "Publisher Copyright: {\textcopyright} 2019, Springer Nature Switzerland AG.; 15th International Symposium on Nuclei in the Cosmos, NIC 2018 ; Conference date: 24-06-2018 Through 29-06-2018",

year = "2019",

doi = "10.1007/978-3-030-13876-9_26",

language = "English",

isbn = "9783030138752",

series = "Springer Proceedings in Physics",

publisher = "Springer Science and Business Media, LLC",

pages = "157--161",

editor = "Alba Formicola and Matthias Junker and Lucio Gialanella and Gianluca Imbriani",

booktitle = "Nuclei in the Cosmos XV",

}

Yoshida, T, Takahashi, K, Umeda, H & Ishidoshiro, K 2019, Neutrinos from Presupernova Stars. in A Formicola, M Junker, L Gialanella & G Imbriani (eds), Nuclei in the Cosmos XV. Springer Proceedings in Physics, vol. 219, Springer Science and Business Media, LLC, pp. 157-161, 15th International Symposium on Nuclei in the Cosmos, NIC 2018, L'Aquila, Italy, 18/6/24. https://doi.org/10.1007/978-3-030-13876-9_26

Neutrinos from Presupernova Stars. / Yoshida, Takashi; Takahashi, Koh; Umeda, Hideyuki et al.
Nuclei in the Cosmos XV. ed. / Alba Formicola; Matthias Junker; Lucio Gialanella; Gianluca Imbriani. Springer Science and Business Media, LLC, 2019. p. 157-161 (Springer Proceedings in Physics; Vol. 219).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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T1 - Neutrinos from Presupernova Stars

AU - Yoshida, Takashi

AU - Takahashi, Koh

AU - Umeda, Hideyuki

AU - Ishidoshiro, Koji

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N2 - Neutrinos from a presupernova star will be observed by current and future neutrino detectors if a nearby supernova at a few hundred parsec from the earth occurs. The events of neutrinos produced through pair-neutrino process are expected to be a few to hundreds depending on stellar mass, neutrino mass hierarchy, and detectors. The neutrino events can be applied to an alarm of the supernova. The supernova alarm will be sent before a few to more than ten hours before the supernova explosion by KamLAND. If hundreds neutrino events are observed by JUNO, the time variation of the burning processes in the central core of the presupernova star can be analyzed from the neutrino events.

AB - Neutrinos from a presupernova star will be observed by current and future neutrino detectors if a nearby supernova at a few hundred parsec from the earth occurs. The events of neutrinos produced through pair-neutrino process are expected to be a few to hundreds depending on stellar mass, neutrino mass hierarchy, and detectors. The neutrino events can be applied to an alarm of the supernova. The supernova alarm will be sent before a few to more than ten hours before the supernova explosion by KamLAND. If hundreds neutrino events are observed by JUNO, the time variation of the burning processes in the central core of the presupernova star can be analyzed from the neutrino events.

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ER -

Neutrinos from Presupernova Stars

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