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A New measurement of the astrophysical $$^8$$Li(d,t)$$^7$$Li reaction

Hashimoto, Takashi; Ishiyama, Hironobu*; Watanabe, Yutaka*; Hirayama, Yoshikazu*; Imai, Nobuaki*; Miyatake, Hiroari; Jeong, S.-C.*; Tanaka, Masahiko*; Yoshikawa, Nobuharu*; Nomura, Toru*; Mitsuoka, Shinichi; Nishio, Katsuhisa   ; Sato, Tetsuya   ; Osa, Akihiko  ; Ichikawa, Shinichi; Matsuda, Makoto  ; Ikezoe, Hiroshi; Das, S. K.*; Mizoi, Yutaka*; Fukuda, Tomokazu*; Sato, Akihiko*; Shimoda, Tadashi; Otsuki, Kaori*; Kajino, Toshitaka*

The excitation function of the $$^8$$Li(d,t)$$^7$$Li reaction was directly measured using $$^8$$Li beams at E$$_{mathrm{cm}}$$ = 0.3, 0.4, 0.5, 0.7, 0.8, 1.0, 1.1, and 1.2 MeV with CD$$_2$$ targets. The beam energies covered the Gamow peaks for 1$$sim$$3$$times$$10$$^9$$ K. Large cross sections were observed at around E$$_{mathrm{cm}}$$ = 0.8 MeV, implying a resonance state located at 22.4 MeV in $$^{10}$$Be. The present astrophysical reaction rate is higher in one order magnitude than the presently adopted rate at around 1$$times$$10$$^9$$ K.

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Category:Astronomy & Astrophysics

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