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Laser Compton Scattering Gamma-Ray Experiments for Supernova Neutrino Process
https://repo.qst.go.jp/records/54772
https://repo.qst.go.jp/records/5477245af703b-3a8a-4113-95a0-fa30015adc71
Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2017-07-04 | |||||
タイトル | ||||||
タイトル | Laser Compton Scattering Gamma-Ray Experiments for Supernova Neutrino Process | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
Hayakawa, Takehito
× Hayakawa, Takehito× Miyamoto, Shuji× Mochizuki, Takayasu× Horikawa, Ken× Amano, Sho× Li, Dazhi× Imazaki, Kazuo× Izawa, Yasukazu× Ogata, Kazuyuki× 早川 岳人 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The neutrino-nucleus interactions are important for understanding nucleosyntheses by neutrino-induced reactions as well as supernova explosion mechanisms. The M1 strength in atomic nuclei is important for estimation of neutrino-nucleus interactions. We have proposed a method using (γ, n) reactions with linear polarized gamma-ray beam generated by laser Compton scattering (LCS) to measure the M1 strength and verified a theoretical prediction. We have discussed experimental technique using the next generation of LCS beams. | |||||
書誌情報 |
Plasma and Fusion Research 巻 11, p. 3406066-1-3406066-5, 発行日 2016-07 |
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出版者 | ||||||
出版者 | The Japan Society of Plasma Science and Nuclear Fusion Research | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1880-6821 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1585/pfr.11.3406066 | |||||
関連サイト | ||||||
識別子タイプ | URI | |||||
関連識別子 | http://www.jspf.or.jp/PFR/PFR_articles/pfr2016/pfr2016_11-3406066.html | |||||
関連名称 | http://www.jspf.or.jp/PFR/PFR_articles/pfr2016/pfr2016_11-3406066.html |