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NSR database version of April 11, 2024.

Search: Author = J.Bliss

Found 4 matches.

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2020BL01      Phys.Rev. C 101, 055807 (2020)

J.Bliss, A.Arcones, F.Montes, J.Pereira

Nuclear physics uncertainties in neutrino-driven, neutron-rich supernova ejecta

NUCLEAR REACTIONS 59,68Fe, 63,71Co, 74,76Ni, 67,77Cu, 72,76,78,79,80Zn, 81Ga, 78,80,82Ge, 83As, 84,85Se, 85,87,88Br, 86,87,88,89,90Kr, 87,89Rb, 88,89,90,91,92,93,94Sr, 94,95Y, 94,95,96,97,98Zr, 97Nb(α, n), T=1-5 GK; calculated abundances of lighter heavy elements with a reaction network under different astrophysical conditions, by varying (α, n) reaction rates within their theoretical uncertainties using a Monte Carlo approach; deduced Spearman's correlation coefficients for Z=36-47, and most important (α, n) reactions affecting the nucleosynthesis in core-collapse supernovae (CCSNe).

doi: 10.1103/PhysRevC.101.055807
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2019HO18      J.Phys.(London) G46, 083001 (2019)

C.J.Horowitz, A.Arcones, B.Cote, I.Dillmann, W.Nazarewicz, I.U.Roederer, H.Schatz, A.Aprahamian, D.Atanasov, A.Bauswein, T.C.Beers, J.Bliss, M.Brodeur, J.A.Clark, A.Frebel, F.Foucart, C.J.Hansen, O.Just, A.Kankainen, G.C.McLaughlin, J.M.Kelly, S.N.Liddick, D.M.Lee, J.Lippuner, D.Martin, J.Mendoza-Temis, B.D.Metzger, M.R.Mumpower, G.Perdikakis, J.Pereira, B.W.O'Shea, R.Reifarth, A.M.Rogers, D.M.Siegel, A.Spyrou, R.Surman, X.Tang, T.Uesaka, M.Wang

r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos

doi: 10.1088/1361-6471/ab0849
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2017BL03      J.Phys.(London) G44, 054003 (2017)

J.Bliss, A.Arcones, F.Montes, J.Pereira

Impact of (α, n) reactions on weak r-process in neutrino-driven winds

NUCLEAR REACTIONS 69Ga, 100Mo(α, n), (α, 2n), E(cm)<24 MeV; calculated yields, abundances using TALYS 1.6 nuclear reaction code. Comparison with available data.

doi: 10.1088/1361-6471/aa63bd
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2014AR01      J.Phys.(London) G41, 044005 (2014)

A.Arcones, J.Bliss

Nucleosynthesis of elements between Sr and Ag in neutron- and proton-rich neutrino-driven winds

doi: 10.1088/0954-3899/41/4/044005
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