NSR Query Results


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NSR database version of April 27, 2024.

Search: Author = B.M.Oginni

Found 4 matches.

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2013CE04      Phys.Rev. C 88, 065806 (2013)

J.M.Cesaratto, A.E.Champagne, M.Q.Buckner, T.B.Clegg, S.Daigle, C.Howard, C.Iliadis, R.Longland, J.R.Newton, B.M.Oginni

Measurement of the Erc.m.=138 keV resonance in the 23Na(p, γ)24Mg reaction and the abundance of sodium in AGB stars

NUCLEAR REACTIONS 23Na(p, γ)24Mg, E<500 keV; measured Eγ, Iγ, on resonance γγ-coin spectra using ECRIS ion source at LENA-TUNL accelerator facility; deduced upper limit on the strength of the 138-keV proton resonance, probability density of the final 23Na abundance, (p, α)/(p, γ) reaction rate ratio, correlations between the final abundance of 23Na in AGB stars and the rate-variation factor. 23Na(p, α)20Ne, E at T9=0.010-10.0; deduced reaction rates for 138-keV resonance. Performed one-zone post-processing nucleosynthesis calculations.

doi: 10.1103/PhysRevC.88.065806
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2076.


2011OG02      Phys.Rev. C 83, 025802 (2011)

B.M.Oginni, C.Iliadis, A.E.Champagne

Theoretical evaluation of the reaction rates for 26Al(n, p)26Mg and 26Al(n, α)23Na

NUCLEAR REACTIONS 26Al(n, p)26Mg, E=0.01-10 MeV; 26Al(n, α)23Na, E=0.01-10 MeV; evaluated σ, fractional contribution to total σ, astrophysical reaction rates using EMPIRE, TALYS, and NON-SMOKER codes. Effects of different level density models and optical model potentials.

doi: 10.1103/PhysRevC.83.025802
Citations: PlumX Metrics


2009OG06      Phys.Rev. C 80, 034305 (2009)

B.M.Oginni, S.M.Grimes, A.V.Voinov, A.S.Adekola, C.R.Brune, D.E.Carter, Z.Heinen, D.Jacobs, T.N.Massey, J.E.O'Donnell, A.Schiller

Test of level density models from reactions of 6Li on 58Fe and 7Li on 57Fe

NUCLEAR REACTIONS 58Fe(6Li, X), E=15 MeV; 57Fe(7Li, X), E=15 MeV; measured particle spectra, σ, angular distributions; deduced optical model parameters. 60Co, 63Ni; deduced level densities. Comparison with Hauser-Feshbach model calculations.

doi: 10.1103/PhysRevC.80.034305
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1749.


2009VO02      Phys.Rev. C 79, 031301 (2009)

A.V.Voinov, B.M.Oginni, S.M.Grimes, C.R.Brune, M.Guttormsen, A.C.Larsen, T.N.Massey, A.Schiller, S.Siem

Nuclear excitations at constant temperature

NUCLEAR REACTIONS 55Mn(6Li, X), (7Li, X), E=15 MeV; 59Co(d, p), (d, α), E=7.5 MeV; measured neutron and proton evaporation spectra, α spectra, σ. Hauser-Feshbach analysis. Comparison with predictions of constant temperature, Fermi-gas, and Hartree-Fock-BCS models.

doi: 10.1103/PhysRevC.79.031301
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1685.


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