NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = H.Umeda Found 13 matches. 2018SU20 Phys.Rev. C 98, 034613 (2018) T.Suzuki, S.Chiba, T.Yoshida, K.Takahashi, H.Umeda Neutrino-nucleus reactions on 16O based on new shell-model Hamiltonians NUCLEAR REACTIONS 16O(ν, e-)16F, 16O(ν-bar, e+)16N, 16O(ν, ν'), 16O(ν, e-p)15O, 16O(ν, e-np)14O, 16O(ν, e-pp)14N, 16O(ν, e-3He)13N, 16O(ν, e-α)12N, 16O(ν, e-p3He)12C, 16O(ν, e-pα)11C, 16O(ν-bar, e+n)15N, 16O(ν-bar, e+np)14C, 16O(ν-bar, e+nn)14N, 16O(ν-bar, e+t)13C, 16O(ν-bar, e+α)12B, 16O(ν-bar, e+nα)11B, 16O(ν, ν'n)15O, 16O(ν, ν'p)15N, 16O(ν, ν'np)14N, 16O(ν, ν'pp)14C, 16O(ν, ν't)13N, 16O(ν, ν'3He)13C, 16O(ν, ν'α)12C, 16O(ν, ν'nα)11C, 16O(ν, ν'pα)11B, E=0-100 MeV; calculated 16O spin-dipole strength, total σ(E), partial σ(E) from each multipole of excited product nucleus or single- and multi-particle emission channels using shell-model with new Hamiltonian SFO-tls, and branching ratios for various channels from Hauser-Feshbach statistical model. Comparison with other theoretical predictions. Discussed production yields of 6,7Li, 7,9Be, 10,11B, 11C from supernova simulations using theoretical reaction cross sections. Discussed effects of multiparticle emission channels on nucleosynthesis in core-collapse supernova explosion. Relevance to supernova (SN) neutrino detection at the Super-Kamiokande.
doi: 10.1103/PhysRevC.98.034613
2009SU08 Phys.Rev. C 79, 061603 (2009) T.Suzuki, M.Honma, K.Higashiyama, T.Yoshida, T.Kajino, T.Otsuka, H.Umeda, K.Nomoto Neutrino-induced reactions on 56Fe and 56Ni, and production of 55Mn in population III stars NUCLEAR REACTIONS 56Fe(ν, e), 56Ni(ν, ν'p)(ν, ν'), E not given; calculated charged current reaction σ, GT strengths, and yield of 55Mn through successive electron captures using shell-model Hamiltonian in pf shell. Comparison with experimental data.
doi: 10.1103/PhysRevC.79.061603
2006HA35 Astrophys.J. 648, L47 (2006) T.Hayakawa, N.Iwamoto, T.Kajino, T.Shizuma, H.Umeda, K.Nomoto Principle of universality of γ-process nucleosynthesis in core-collapse supernova explosions
doi: 10.1086/507703
2006HA38 Eur.Phys.J. A 27, Supplement 1, 123 (2006) T.Hayakawa, N.Iwamoto, T.Shizuma, T.Kajino, H.Umeda, K.Nomoto Evidence for p-process nucleosynthesis recorded at the Solar System abundances
doi: 10.1140/epja/i2006-08-017-6
2006NO15 Nucl.Phys. A777, 424 (2006) K.Nomoto, N.Tominaga, H.Umeda, C.Kobayashi, K.Maeda Nucleosynthesis yields of core-collapse supernovae and hypernovae, and galactic chemical evolution
doi: 10.1016/j.nuclphysa.2006.05.008
2005HA50 Nucl.Phys. A758, 525c (2005) T.Hayakawa, N.Iwamoto, T.Shizuma, T.Kajino, H.Umeda, K.Nomoto Scaling relations for the supernova γ-process and the 176Lu nuclear cosmochronometer
doi: 10.1016/j.nuclphysa.2005.05.095
2005NO12 Nucl.Phys. A758, 263c (2005) K.Nomoto, N.Tominaga, H.Umeda, K.Maeda, T.Ohkubo, J.Deng Nucleosynthesis in Hypernovae and Population III Supernovae
doi: 10.1016/j.nuclphysa.2005.05.045
2004HA47 Phys.Rev.Lett. 93, 161102 (2004) T.Hayakawa, N.Iwamoto, T.Shizuma, T.Kajino, H.Umeda, K.Nomoto Evidence for Nucleosynthesis in the Supernova γ Process: Universal Scaling for p Nuclei
doi: 10.1103/PhysRevLett.93.161102
2003NO05 Nucl.Phys. A718, 277c (2003) K.Nomoto, H.Umeda, K.Maeda, T.Ohkubo, J.Deng, P.Mazzali Nucleosynthesis in Hypernovae and Extremely Metal-Poor Stars
doi: 10.1016/S0375-9474(03)00728-0
2003NO08 Prog.Theor.Phys.(Kyoto), Suppl. 151, 44 (2003) K.Nomoto, K.Maeda, H.Umeda, T.Ohkubo, J.Deng, P.Mazzali Nucleosynthesis in Black-Hole-Forming Supernovae and Extremely Metal-Poor Stars
doi: 10.1143/PTPS.151.44
2003OH05 Nucl.Phys. A718, 632c (2003) Pop III Hypernova Nucleosynthesis and Abundance Trends in Extremely Metal-Poor Halo Stars
doi: 10.1016/S0375-9474(03)00907-2
2001NA37 Astrophys.J. 555, 880 (2001) T.Nakamura, H.Umeda, K.Iwamoto, K.Nomoto, M.-A.Hashimoto, W.R.Hix, F.-K.Thielemann Explosive Nucleosynthesis in Hypernovae
doi: 10.1086/321495
1999NA28 Astrophys.J. 517, 193 (1999) T.Nakamura, H.Umeda, K.Nomoto, F.-K.Thielemann, A.Burrows Nucleosynthesis in Type II Supernovae and the Abundances in Metal-Poor Stars
doi: 10.1086/307167
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