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NSR database version of May 3, 2024.

Search: Author = S.M.Graff

Found 7 matches.

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1995SC02      Phys.Rev. C51, 379 (1995)

H.Schatz, S.Jaag, G.Linker, R.Steininger, F.Kappeler, P.E.Koehler, S.M.Graff, M.Wiescher

Stellar Cross Sections for ³³S(n, α)³⁰Si, ³⁶Cl(n, p)³⁶S, and ³⁶Cl(n, α)³³P and the Origin of ³⁶S

NUCLEAR REACTIONS ³³S(n, α), ³⁶Cl(n, p), (n, α), E=10-260 keV; measured < σ(E) >; deduced stellar reaction rate for ³³S(n, α), nucleosynthesis of ³⁶S. Ionization chamber.

doi: 10.1103/PhysRevC.51.379
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22749.

1994VO12      Phys.Rev. C50, 1185 (1994)

S.Vouzoukas, C.P.Browne, U.Giesen, J.Gorres, S.M.Graff, H.Herndl, C.Iliadis, L.O.Lamm, J.Meissner, J.G.Ross, K.Scheller, L.van Wormer, M.Wiescher, A.A.Rollefson

Reaction Rate for ³¹S(p, γ)³²Cl and Its Influence on the SiP Cycle in Hot Stellar Hydrogen Burning

NUCLEAR REACTIONS ³²S(³He, t), E=22.5-25 MeV; measured σ(Et), σ(θ); deduced ³¹S(p, γ) reaction rate, hot stellar hydrogen burning implications. ³²Cl deduced level, J, π, C²S, Γγ.

doi: 10.1103/PhysRevC.50.1185
Citations: PlumX Metrics

1993KO13      Phys.Rev. C47, 2107 (1993)

P.E.Koehler, S.M.Graff, H.A.O'Brien, Yu.M.Gledenov, Yu.P.Popov

³⁶Cl(n, p)³⁶S Cross Section from 25 meV to 800 keV and the Nucleosynthesis of the Rare Isotope ³⁶S

NUCLEAR REACTIONS ³⁶Cl(n, p), E=thermal-800 keV; measured σ(E); deduced astrophysical reaction rate. ³⁶S deduced resonances, Γ, γ-strength function. Other data input.

doi: 10.1103/PhysRevC.47.2107
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset13905.

1992IL01      Nucl.Phys. A539, 97 (1992)

C.Iliadis, U.Giesen, J.Gorres, M.Wiescher, S.M.Graff, R.E.Azuma, C.A.Barnes

Direct Proton Capture on ³²S

NUCLEAR REACTIONS, ICPND ³²S(p, γ), E=0.4-2 MeV; measured Eγ, Iγ, absolute γ yield vs E; deduced stellar reaction rate. ³³Cl levels deduced C²S.

doi: 10.1016/0375-9474(92)90237-E
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0795.

1992IL03      Phys.Rev. C45, 2989 (1992)

C.Iliadis, J.G.Ross, J.Gorres, M.Wiescher, S.M.Graff, R.E.Azuma

Reaction ³⁶Ar(p, γ)³⁷K in Explosive Hydrogen Burning

NUCLEAR REACTIONS, ICPND ³⁶Ar(p, γ), E=0.32-0.93 MeV; measured Eγ, Iγ, γ yield vs E; calculated thermonuclear reaction rate vs temperature. ³⁷K levels deduced branching ratios, resonance strength.

doi: 10.1103/PhysRevC.45.2989
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0108.

1991KO31      Phys.Rev. C44, 2788 (1991)

P.E.Koehler, S.M.Graff

¹⁷O(n, α)¹⁴C Cross Section from 25 meV to Approximately 1 MeV

NUCLEAR REACTIONS ¹⁷O(n, α), E=25 meV-1 MeV; measured σ(E); calculated astrophysical reaction rate. Non standard, big-bang nucleosynthesis. Enriched targets.

doi: 10.1103/PhysRevC.44.2788
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset13534.

1990LA05      Nucl.Phys. A510, 503 (1990)

L.O.Lamm, C.P.Browne, J.Gorres, S.M.Graff, M.Wiescher, A.A.Rollefson, B.A.Brown

The Level Structure of ²⁰Na and the Impact upon the Stellar Reaction Rate for ¹⁹Ne(p, γ)²⁰Ne

NUCLEAR REACTIONS, ICPND ²⁰Ne(³He, t), E=25.5 MeV; measured σ(θ). ²⁰Na deduced levels, J, π. ¹⁹Ne(p, γ), E=low; calculated stellar reaction rate.

doi: 10.1016/0375-9474(90)90063-R
Citations: PlumX Metrics