NSR Query Results


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NSR database version of April 11, 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


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