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NSR database version of April 11, 2024.

Search: Author = L.R.Buchmann

Found 4 matches.

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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
Citations: PlumX Metrics


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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