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NSR database version of April 25, 2024.

Search: Author = A.Meadowcroft

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2006JE03      Phys.Rev. C 73, 065802 (2006)

D.G.Jenkins, A.Meadowcroft, C.J.Lister, M.P.Carpenter, P.Chowdhury, N.J.Hammond, R.V.F.Janssens, T.L.Khoo, T.Lauritsen, D.Seweryniak, T.Davinson, P.J.Woods, A.Jokinen, H.Penttila, G.Martinez-Pinedo, J.Jose

Reevaluation of the ³⁰P(p, γ)³¹S astrophysical reaction rate from a study of the T = 1/2 mirror nuclei, ³¹S and ³¹P

NUCLEAR REACTIONS ¹²C(²⁰Ne, p), (²⁰Ne, n), E=32 MeV; measured Eγ, Iγ, γγ-, (recoil)γ-coin. ³¹S, ³¹P deduced high-spin levels, J, π. ³¹P(p, γ), E=low; deduced proton widths and resonance strengths, astrophysical reaction rates. Gammasphere array, fragment mass analyzer.

doi: 10.1103/PhysRevC.73.065802
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