C-12+C-12 fusion S*-factor from a full-microscopic nuclear model

Taniguchi, Yasutaka; Kimura, Masaaki

Physics Letters B, 2022, 823, 136790

Permalink : https://hdl.handle.net/2115/84532

このアイテムのアクセス数:463件（2026-02-12 16:45 集計）

ファイル	フォーマット	サイズ	閲覧回数	説明
https://doi.org/10.1016/j.physletb.2021.136790

アクセス権	metadata only access
URI	https://hdl.handle.net/2115/84532
タイトル	C-12+C-12 fusion S*-factor from a full-microscopic nuclear model
著者	著者名 Taniguchi, Yasutaka
著者	e-Rad_Researcher 50402813 著者名 Kimura, Masaaki
言語	英語
キーワード	C-12+C-12 fusion
	Astrophysical S-factor
	Microscopic nuclear model
発行日	2022
出版者	Elsevier
収録物名	Physics Letters B
巻(号)	823
ページ	136790
抄録	The C-12 + C-12 fusion reaction plays a vital role in the explosive phenomena of the universe. The resonances in the Gamow window rule its reaction rate and products. Hence, the determination of the resonance parameters by nuclear models is indispensable as the direct measurement is not feasible. Here, for the first time, we report the resonances in the C-12 + C-12 fusion reaction described by a full-microscopic nuclear model. The model plausibly reproduces the measured low-energy astrophysical S-factors and predicts the resonances in the Gamow window. Contradictory to the hindrance model, we conclude that there is no low-energy suppression of the S-factor. (C) 2021 The Authors. Published by Elsevier B.V.
資源タイプ	学術雑誌論文
出版タイプ	Version of Record
PISSN	0370-2693
関連情報 (isIdenticalTo)	出版社版DOI https://doi.org/10.1016/j.physletb.2021.136790