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Kirsebom, O S; Alcorta, M; Borge, M J G; Cubero, M; Diget, C Aa; Fraile, L M; Fulton, B R; Fynbo, H O U; Galaviz, D; Jonson, B; Madurga, M; Nilsson, T; Nyman, G; Riisager, K; Tengblad, O; Turrión, M
Physical review letters, 2012-May-18, Letnik: 108, Številka: 20Journal Article
The current evaluation of the triple-α reaction rate assumes that the α decay of the 7.65 MeV, 0+ state in 12C, commonly known as the Hoyle state, proceeds sequentially via the ground state of 8Be. This assumption is challenged by the recent identification of two direct α-decay branches with a combined branching ratio of 17(5)%. If correct, this would imply a corresponding reduction in the triple-α reaction rate with important astrophysical consequences. We have used the 11B(3He,d) reaction to populate the Hoyle state and measured the decay to three α particles in complete kinematics. We find no evidence for direct α-decay branches, and hence our data do not support a revision of the triple-α reaction rate. We obtain an upper limit of 5×10(-3) on the direct α decay of the Hoyle state at 95% C.L., which is 1 order of magnitude better than a previous upper limit.
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