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NSR database version of April 27, 2024.

Search: Author = M.T.Rabban

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2000BB04      Phys.Rev. C62, 055804 (2000)

D.W.Bardayan, J.C.Blackmon, C.R.Brune, A.E.Champagne, A.A.Chen, J.M.Cox, T.Davinson, V.Y.Hansper, M.A.Hofstee, B.A.Johnson, R.L.Kozub, Z.Ma, P.D.Parker, D.E.Pierce, M.T.Rabban, A.C.Shotter, M.S.Smith, K.B.Swartz, D.W.Visser, P.J.Woods

The Astrophysically Important 3⁺ State in ¹⁸Ne and the ¹⁷F(p, γ)¹⁸Ne Stellar Rate

NUCLEAR REACTIONS ¹H(¹⁷F, ¹⁷F), (¹⁷F, p), E=9-12 MeV; measured recoil proton spectra, angular distributions, (proton)(fluorine)-coin. ¹⁸Ne; deduced resonance J, π. ¹⁷F(p, γ), E not given; calculated astrophysical reaction rates. ¹H(¹⁷O, ¹⁷O), E=10.1, 12.2 MeV; measured proton angular distributions. Silicon detector array.

doi: 10.1103/PhysRevC.62.055804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0759.

1999BA49      Phys.Rev.Lett. 83, 45 (1999)

D.W.Bardayan, J.C.Blackmon, C.R.Brune, A.E.Champagne, A.A.Chen, J.M.Cox, T.Davinson, V.Y.Hansper, M.A.Hofstee, B.A.Johnson, R.L.Kozub, Z.Ma, P.D.Parker, D.E.Pierce, M.T.Rabban, A.C.Shotter, M.S.Smith, K.B.Swartz, D.W.Visser, P.J.Woods

Observation of the Astrophysically Important 3⁺ State in ¹⁸Ne via Elastic Scattering of a Radioactive ¹⁷F Beam from ¹H

NUCLEAR REACTIONS ¹H(¹⁷F, ¹⁷F), E ≈ 10-12 MeV; measured proton yields, (proton)(fluorine)-coin. ¹⁸Ne deduced resonance energy, width. ¹⁷F(p, γ), E not given; calculated resonance contribution to proton capture rate. Astrophysical implications discussed.

doi: 10.1103/PhysRevLett.83.45
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0184.