NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = V.Barnard Found 4 matches. 2002WI15 Eur.Phys.J. A 15, 59 (2002) M.Wiescher, V.Barnard, J.L.Fisker, J.Gorres, K.Langanke, G.Martinez-Pinedo, F.Rembges, H.Schatz, F.K.Thielemann Nuclear-reaction rates in the thermonuclear runaway phase of accreting neutron stars NUCLEAR REACTIONS 46Cr, 55Cu, 59Ga(p, γ), E=low; calculated astrophysical reaction rates.
doi: 10.1140/epja/i2001-10226-8
2001FI23 At.Data Nucl.Data Tables 79, 241 (2001) J.L.Fisker, V.Barnard, J.Gorres, K.Langanke, G.Martinez-Pinedo, M.C.Wiescher Shell Model Based Reaction Rates for rp-Process Nuclei in the Mass Range A = 44-63 NUCLEAR REACTIONS 44,45,46Ti, 45,46,47V, 45,46,47,48,49,50Cr, 45,46,47,48,49,50,51,52,53Mn, 50,51,52,53,54,55,56Fe, 50,51,52,53,54,55,56,57Co, 55,56,57,58,59Ni, 54,55,56,57,58,59,60,61Cu, 59,60,61,62,63Zn, 59,60,61,62,63Ga(p, γ), E not given; calculated astrophysical reaction rates vs temperature. NUCLEAR STRUCTURE 45,46,47V, 46,47,48Cr, 46,47,48,49,50,51Mn, 46,47,48,49,50,51,52,53,54Fe, 51,52,53,54,55,56,57Co, 51,52,53,54,55,56,57,58Ni, 56,57,58,59,60Cu, 55,56,57,58,59,60,61,62Zn, 60,61,62,63,64Ga, 60,61,62,63,64Ge; calculated levels, J, π, decay widths. Shell model.
doi: 10.1006/adnd.2001.0867
2001SC21 Phys.Rev.Lett. 86, 3471 (2001) H.Schatz, A.Aprahamian, V.Barnard, L.Bildsten, A.Cumming, M.Ouellette, T.Rauscher, F.-K.Thielemann, M.Wiescher End Point of the rp Process on Accreting Neutron Stars NUCLEAR STRUCTURE Z=27-54; calculated astrophysical abundances; deduced rp-process endpoint.
doi: 10.1103/PhysRevLett.86.3471
2001SC29 Nucl.Phys. A688, 150c (2001) H.Schatz, A.Aprahamian, V.Barnard, L.Bildsten, A.Cumming, M.Ouellette, T.Rauscher, F.-K.Thielemann, M.Wiescher The Endpoint of the rp-Process on Accreting Neutron Stars
doi: 10.1016/S0375-9474(01)00688-1
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