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NSR database version of April 24, 2024.

Search: Author = M.J.Bojazi

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2018TA12      Phys.Rev. C 97, 055801 (2018)

R.Talwar, M.J.Bojazi, P.Mohr, K.Auranen, M.L.Avila, A.D.Ayangeakaa, J.Harker, C.R.Hoffman, C.L.Jiang, S.A.Kuvin, B.S.Meyer, K.E.Rehm, D.Santiago-Gonzalez, J.Sethi, C.Ugalde, J.R.Winkelbauer

Experimental study of ³⁸Ar + α reaction cross sections relevant to the ⁴¹Ca abundance in the solar system

NUCLEAR REACTIONS ⁴He(³⁸Ar, p), (³⁸Ar, n), (³⁸Ar, α'), E=133 MeV; measured energies and yields of reaction products, energy- and angle integrated σ(E) using multisampling ionization chamber (MUSIC) detector at the ATLAS-ANL facility. Comparison with previous experimental values, and with statistical model calculations using TALYS code. ⁴¹K(p, α)³⁸Ar, ⁴¹Ca(n, α)³⁸Ar, T=0.1-10.0 GK; deduced astrophysical reaction rates, and compared with statistical model calculations, and with REACLIB fits. Discussed relevance to ⁴¹Ca abundance in the solar system.

doi: 10.1103/PhysRevC.97.055801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2302.

2014BO04      Phys.Rev. C 89, 025807 (2014)

M.J.Bojazi, B.S.Meyer

Explosive nucleosynthesis of ¹⁵Na in a massive-star model

NUCLEAR REACTIONS ¹⁴N(α, γ)¹⁸F, ¹⁸F(n, α)¹⁵N, ¹⁸O(p, α)¹⁵N, E at stellar temperatures; calculated mass fraction of ¹⁵N in explosive nucleosynthesis through different pathways in helium-rich outer layers of massive stars over all the 707 zones available in the presupernova stars including neutrino-nucleus interactions, time evolution of mass fractions of neutrons, protons, ^14,15N, ¹⁸O and ¹⁸F; discussed competition between the production and destruction of ¹⁵N, latter through ¹⁵N(p, α)¹²C and ¹⁵N(α, γ)¹⁹F reactions. Comparison of presupernova and postsupernova values, and with previous calculations A simple but realistic model of shock passage using open-source, freely available codes.

doi: 10.1103/PhysRevC.89.025807
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2005RI11      Phys.Rev. C 72, 024311 (2005)

L.A.Riley, M.A.Abdelqader, D.Bazin, M.J.Bojazi, B.A.Brown, C.M.Campbell, J.A.Church, P.D.Cottle, D.-C.Dinca, J.Enders, A.Gade, T.Glasmacher, M.Honma, S.Horibe, Z.Hu, K.W.Kemper, W.F.Mueller, H.Olliver, T.Otsuka, B.C.Perry, B.T.Roeder, B.M.Sherrill, T.P.Spencer, J.R.Terry

Thick-target inverse-kinematics proton scattering from ⁴⁶Ar and the N = 28 shell below ⁴⁸Ca

NUCLEAR REACTIONS ¹H, C(⁴⁶Ar, ⁴⁶Ar'), E ≈ 68 MeV/nucleon; measured Eγ, Iγ, (particle)γ-coin. ⁴⁶Ar deduced levels, J, π, B(E2), deformation lengths. Optical model analysis.

NUCLEAR STRUCTURE ⁴⁶Ar, ⁴⁸Ca, ⁵⁰Ti, ⁵²Cr, ⁵⁴Fe; calculated B(E2), ratio of neutron-to-proton transition matrix elements.

doi: 10.1103/PhysRevC.72.024311
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1494. Data from this article have been entered in the XUNDL database. For more information, click here.