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NSR database version of April 27, 2024.

Search: Author = D.S.Burke

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2018CH08      Phys.Rev. C 97, 025802 (2018)

G.Christian, G.Lotay, C.Ruiz, C.Akers, D.S.Burke, W.N.Catford, A.A.Chen, D.Connolly, B.Davids, J.Fallis, U.Hager, D.Hutcheon, A.Mahl, A.Rojas, X.Sun

Direct measurement of astrophysically important resonances in ³⁸K(p, γ) ³⁹Ca

NUCLEAR REACTIONS ¹H(³⁸K, γ)³⁹Ca, E=15.58, 20.56, 27.17 MeV, [³⁸K secondary beam produced at ISAC-I, TRIUMF facility by impinging 500 MeV protons on a high-power TiC production target]; measured recoils using DRAGON spectrometer, prompt Eγ, Iγ, (recoil)γ-coin using bismuth-germanate scintillator array for γ detection. Windowless hydrogen gas target; deduced energies of resonances, resonance strengths for the 386-, 515- and 689-keV proton resonances, astrophysical reaction rates for temperature range of 150-500 MK, abundances of ³⁸Ar, ³⁹K, and ⁴⁰Ca in the hottest oxygen-neon novae.

doi: 10.1103/PhysRevC.97.025802
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2284. Data from this article have been entered in the XUNDL database. For more information, click here.

2016LO03      Phys.Rev.Lett. 116, 132701 (2016)

G.Lotay, G.Christian, C.Ruiz, C.Akers, D.S.Burke, W.N.Catford, A.A.Chen, D.Connolly, B.Davids, J.Fallis, U.Hager, D.A.Hutcheon, A.Mahl, A.Rojas, X.Sun

Direct Measurement of the Astrophysical ³⁸K(p, γ)³⁹Ca Reaction and Its Influence on the Production of Nuclides toward the End Point of Nova Nucleosynthesis

NUCLEAR REACTIONS ¹H(³⁸K, γ), E=386, 515, 689 keV; measured reaction products, Eγ, Iγ; deduced yields, resonance parameters, astrophysical reaction rates. Comparison with available data.

doi: 10.1103/PhysRevLett.116.132701
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2284. Data from this article have been entered in the XUNDL database. For more information, click here.