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NSR database version of April 25, 2024.

Search: Author = L.R.Buchmann

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2006BU32      Nucl.Phys. A777, 254 (2006)

L.R.Buchmann, C.A.Barnes

Nuclear reactions in stellar helium burning and later hydrostatic burning stages

NUCLEAR REACTIONS ¹²C(α, α), E=2.5-8.3 MeV; analyzed σ, phase-shifts. ¹²C(α, γ), E=0.25-3.39, 6.5-8.5 MeV; analyzed σ, astrophysical S-factor, E1, E2 contributions and capture to ¹⁶O 6.9 MeV state. R-matrix analysis. Implications to stellar reaction rates discussed.

NUCLEAR STRUCTURE ¹²C, ¹⁶O; analyzed energy levels, spin, π. Implications to stellar reaction rates discussed.

RADIOACTIVITY ¹⁶N(β^-α); analyzed Eα, Iα.

doi: 10.1016/j.nuclphysa.2005.01.005
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2005JU03      Nucl.Phys. B(Proc.Supp.) S138, 112 (2005)

A.R.Junghans, E.C.Mohrmann, K.A.Snover, T.D.Steiger, E.G.Adelberger, J.M.Casandjian, H.E.Swanson, L.R.Buchmann, A.Laird, S.Park, A.Y.Zyuzin

The new Seattle-TRIUMF ⁷Be(p, γ)⁸B S-factor determination

NUCLEAR REACTIONS ⁷Be(p, γ), E(cm)=116-2460 MeV; measured σ; deduced astrophysical S-factors. Comparison with previous results.

doi: 10.1016/j.nuclphysbps.2004.11.028
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2004JU08      Nucl.Phys. A746, 210c (2004)

A.R.Junghans, E.C.Mohrmann, K.A.Snover, T.D.Steiger, E.G.Adelberger, J.M.Casandjian, H.E.Swanson, L.R.Buchmann, A.M.Laird, S.Park, A.Y.Zyuzin

New determination of the ⁷Be(p, γ)⁸B S-factor

NUCLEAR REACTIONS ⁷Be(p, γ), E(cm)=116-2460 MeV; measured σ; deduced astrophysical S-factors. Comparison with previous results.

doi: 10.1016/j.nuclphysa.2004.09.035
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1004.

1994KU06      Z.Phys. A348, 59 (1994)

S.Kubono, C.C.Yun, R.N.Boyd, L.R.Buchmann, Y.Fuchi, M.Hosaka, N.Ikeda, C.L.Jiang, I.Katayama, H.Kawashima, H.Miyatake, T.Niizeki, T.Nomura, A.Odahara, M.Ohura, H.Ohnuma, H.Orihara, C.Rolfs, T.Shimoda, Y.Tajima, M.H.Tanaka, H.Toyokawa

High Resolution Study of ²⁴Mg(p, d)²³Mg for the Ne-E Problem

NUCLEAR REACTIONS ²⁴Mg(p, d), E=34-945 MeV; measured deuteron spectra, σ(θ); deduced ²²Na(p, γ) reaction rate, astrophysics related Ne-E problem implications. ²³Mg deduced level, possible J, π.

doi: 10.1007/BF01291654
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