NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = T.Kajino Found 125 matches. Showing 1 to 100. [Next]2024SA18 Phys.Lett. B 851, 138581 (2024) H.Sasaki, Y.Yamazaki, T.Kajino, G.J.Mathews Effects of Hoyle state de-excitation on νp–process nucleosynthesis and Galactic chemical evolution NUCLEAR STRUCTURE 12C, 92,94Mo, 96,98Ru; calculated impact of Hoyle states on isotope production in proton-rich neutrino-driven winds.
doi: 10.1016/j.physletb.2024.138581
2022KO31 Astrophys.J. 937, 116 (2022) H.Ko, D.Jang, M.-K.Cheoun, M.Kusakabe, H.Sasaki, X.Yao, T.Kajino, T.Hayakawa, M.Ono, T.Kawano, G.J.Mathews Comprehensive Analysis of the Neutrino Process in Core-collapsing Supernovae ATOMIC MASSES 7Li, 7Be, 11B, 11C, 92Nb, 98Tc, 138La, 180Ta; analyzed available data; deduced abundances for the neutrino flavor change effects due to neutrino self-interaction and shock wave propagation, as well as the matter effects on the neutrino process in core-collapsing supernovae (CCSNe).
doi: 10.3847/1538-4357/ac88cd
2022SC17 J.Phys.(London) G49, 110502 (2022) H.Schatz, A.D.Becerril Reyes, A.Best, E.F.Brown, K.Chatziioannou, K.A.Chipps, C.M.Deibel, R.Ezzeddine, D.K.Galloway, C.J.Hansen, F.Herwig, A.P.Ji, M.Lugaro, Z.Meisel, D.Norman, J.S.Read, L.F.Roberts, A.Spyrou, I.Tews, F.X.Timmes, C.Travaglio, N.Vassh, C.Abia, P.Adsley, S.Agarwal, M.Aliotta, W.Aoki, A.Arcones, A.Aryan, A.Bandyopadhyay, A.Banu, D.W.Bardayan, J.Barnes, A.Bauswein, T.C.Beers, J.Bishop, T.Boztepe, B.Cote, M.E.Caplan, A.E.Champagne, J.A.Clark, M.Couder, A.Couture, S.E.de Mink, S.Debnath, R.J.deBoer, J.den Hartogh, P.Denissenkov, V.Dexheimer, I.Dillmann, J.E.Escher, M.A.Famiano, R.Farmer, R.Fisher, C.Frohlich, A.Frebel, C.Fryer, G.Fuller, A.K.Ganguly, S.Ghosh, B.K.Gibson, T.Gorda, K.N.Gourgouliatos, V.Graber, M.Gupta, W.C.Haxton, A.Heger, W.R.Hix, W.C.G.Ho, E.M.Holmbeck, A.A.Hood, S.Huth, G.Imbriani, R.G.Izzard, R.Jain, H.Jayatissa, Z.Johnston, T.Kajino, A.Kankainen, G.G.Kiss, A.Kwiatkowski, M.La Cognata, A.M.Laird, L.Lamia, P.Landry, E.Laplace, K.D.Launey, D.Leahy, G.Leckenby, A.Lennarz, B.Longfellow, A.E.Lovell, W.G.Lynch, S.M.Lyons, K.Maeda, E.Masha, C.Matei, J.Merc, B.Messer, F.Montes, A.Mukherjee, M.R.Mumpower, D.Neto, B.Nevins, W.G.Newton, L.Q.Nguyen, K.Nishikawa, N.Nishimura, F.M.Nunes, E.O'Connor, B.W.O'Shea, W.-J.Ong, S.D.Pain, M.A.Pajkos, M.Pignatari, R.G.Pizzone, V.M.Placco, T.Plewa, B.Pritychenko, A.Psaltis, D.Puentes, Y.-Z.Qian, D.Radice, D.Rapagnani, B.M.Rebeiro, R.Reifarth, A.L.Richard, N.Rijal, I.U.Roederer, J.S.Rojo, J.S K, Y.Saito, A.Schwenk, M.L.Sergi, R.S.Sidhu, A.Simon, T.Sivarani, A.Skuladottir, M.S.Smith, A.Spiridon, T.M.Sprouse, S.Starrfield, A.W.Steiner, F.Strieder, I.Sultana, R.Surman, T.Szucs, A.Tawfik, F.Thielemann, L.Trache, R.Trappitsch, M.B.Tsang, A.Tumino, S.Upadhyayula, J.O.Valle Martinez, M.Van der Swaelmen, C.Viscasillas Vazquez, A.Watts, B.Wehmeyer, M.Wiescher, C.Wrede, J.Yoon, R.G.T.Zegers, M.A.Zermane, M.Zingale, the Horizon 2020 Collaborations Horizons: nuclear astrophysics in the 2020s and beyond
doi: https://dx.doi.org/10.1088/1361-6471/ac8890
2022YA16 Astrophys.J. 933, 112 (2022) Y.Yamazaki, Z.He, T.Kajino, G.J.Mathews, M.A.Famiano, X.Tang, J.Shi Possibility to Identify the Contributions from Collapsars, Supernovae, and Neutron Star Mergers from the Evolution of the r-process Mass Abundance Distribution
doi: 10.3847/1538-4357/ac721c
2021CH36 Astrophys.J. 915, 78 (2021) H.Cheng, B.-H.Sun, L.-H.Zhu, M.Kusakabe, Y.Zheng, L.C.He, T.Kajino, Z.-M.Niu, T.-X.Li, C.-B.Li, D.-X.Wang, M.Wang, G.-S.Li, K.Wang, L.Song, G.Guo, Z.-Y.Huang, X.-L.Wei, F.-W.Zhao, X.-G.Wu, Y.Abulikemu, J.-C.Liu, P.Fan Measurements of 160Dy(p, γ) at Energies Relevant for the Astrophysical γ Process NUCLEAR REACTIONS 160Dy(p, γ), 161Dy(p, n), E=3.4-7 MeV; measured reaction products, Eγ, Iγ; deduced σ, S-factor, astrophysical reaction rates. Comparison with TALYS, NON-SMOKER calculations.
doi: 10.3847/1538-4357/ac00b1
2021HA21 Phys.Rev. C 103, 045801 (2021) T.Hayakawa, Y.Toh, A.Kimura, S.Nakamura, T.Shizuma, N.Iwamoto, S.Chiba, T.Kajino Isomer production ratio of the 112Cd(n, γ) 113Cd reaction in an s-process branching point NUCLEAR REACTIONS 112Cd(n, γ)113Cd/113mCd, E=66.8-8587 eV neutrons from BL04 neutron beam line of the MLF at J-PARC; measured E(n), I(n) by time-of-flight method, Eγ, Iγ using ANNRI array of two cluster HPGe detectors, eight coaxial HPGe detectors, and BGO Compton-suppression shields. 113Cd; deduced γ-rays intensities decaying to the ground state and the isomer, isomer production ratios for 21 neutron resonances from 66.8 to 8587 eV, minor s-process contribution from the 113Cd isomer to the solar abundance of 115Sn, Jπ of 14 neutron resonances from comparison of experimental γ-ray intensities with the corresponding expected theoretical yields for 1/2-, 1/2+ and 3/2- resonances using CCONE Hauser-Feshbach statistical model calculations.
doi: 10.1103/PhysRevC.103.045801
2021SP02 Eur.Phys.J. A 57, 20 (2021) C.Spitaleri, S.Typel, C.A.Bertulani, A.M.Mukhamedzhanov, T.Kajino, M.Lattuada, A.Cvetinovic, S.Messina, G.L.Guardo, N.Soic, M.Milin, S.S.Perrotta, C.Li, P.Colovic, G.D'Agata, D.Dell'Aquila, C.G.Fatuzzo, M.Gulino, S.Q.Hou, M.La Cognata, D.Lattuada, D.Nurkic, R.Popocovski, N.Skukan, S.Szilner, O.Trippella, M.Uroic, N.Vukman The 3He + 5He → α+α reaction below the Coulomb barrier via the Trojan Horse Method NUCLEAR REACTIONS 9Be(3He, 2α), E=4 MeV; 3He(5He, α), E(cm)<1 Mev; measured reaction products, Eα, Iα; deduced two α-particles σ(θ, E), σ(θ). Comparison with theoretical calculations, Trojan Horse Method (THM).
doi: 10.1140/epja/s10050-020-00324-4
2020HE19 Astrophys.J. 899, 133 (2020) M.He, S.-S.Zhang, M.Kusakabe, S.Xu, T.Kajino Nuclear Structures of 17O and Time-dependent Sensitivity of the Weak s-process to the 16O(n, γ)17O Rate NUCLEAR REACTIONS 16O(n, γ), E(cm)<1 MeV; analyzed available data; deduced resonance parameters, total σ, reaction rates. Comparison with available data.
doi: 10.3847/1538-4357/aba7b4
2019KA42 Prog.Part.Nucl.Phys. 107, 109 (2019) T.Kajino, W.Aoki, A.B.Balantekin, R.Diehl, M.A.Famiano, G.J.Mathews Current status of r-process nucleosynthesis
doi: 10.1016/j.ppnp.2019.02.008
2019KO30 Acta Phys.Pol. B50, 385 (2019) H.Ko, M.-K.Cheoun, M.Kusakabe, T.Kajino, B.Ekinci, Y.Pehlivan Effects of Shock Propagation on Neutrino Oscillation and ν-induced Nucleosynthesis in Supernova NUCLEAR REACTIONS 138Ba(ν, e-)138La, E not given; calculated reaction rates, abundances in supernova in case of shock propagation effect on ν oscillation.
doi: 10.5506/aphyspolb.50.385
2019SU21 J.Phys.(London) G46, 075103 (2019) T.Suzuki, A.B.Balantekin, T.Kajino, S.Chiba Neutrino-13C cross sections at supernova neutrino energies NUCLEAR REACTIONS 13C(ν, E), (ν, ν), E<50 MeV; calculated σ. Comparison with available data.
doi: 10.1088/1361-6471/ab1c11
2018HA31 Phys.Rev.Lett. 121, 102701 (2018) T.Hayakawa, H.Ko, M.-K.Cheoun, M.Kusakabe, T.Kajino, M.D.Usang, S.Chiba, K.Nakamura, A.Tolstov, K.Nomoto, M.-a.Hashimoto, M.Ono, T.Kawano, G.J.Mathews Short-Lived Radioisotope 98Tc Synthesized by the Supernova Neutrino Process NUCLEAR REACTIONS 98Mo(ν, E)98Tc, 99Tc(ν, ν'n)98Tc, 99Ru(ν, ν'p)98Tc, E=1-9 MeV; calculated yields, abundances as a function of interior mass from the Supernova; deduced dominance the charged current reaction on 98Mo reaction.
doi: 10.1103/PhysRevLett.121.102701
2017MA53 Int.J.Mod.Phys. E26, 1741001 (2017) G.J.Mathews, M.Kusakabe, T.Kajino Introduction to big bang nucleosynthesis and modern cosmology COMPILATION 2H, 3,4He, 7Li; compiled isotopic abundances of light nuclei. Comparison with theoretical calculations.
doi: 10.1142/S0218301317410014
2016BE16 Prog.Part.Nucl.Phys. 89, 56 (2016) Frontiers in nuclear astrophysics
doi: 10.1016/j.ppnp.2016.04.001
2016FA05 Phys.Rev. C 93, 045804 (2016) M.A.Famiano, A.B.Balantekin, T.Kajino Low-lying resonances and relativistic screening in Big Bang nucleosynthesis NUCLEAR REACTIONS 7Be(3He, γ)10C*, E=0.2-2 MeV; calculated integrand of thermonuclear reaction rate (TRR) for energy-dependent width, effects of relativistic electron screening, integrand of the reaction rate for a narrow resonance, ratio of screened to bare TRR for the nonresonant component of the TRR only, thermonuclear reaction rates for several resonances for possible 10C+γ, 9B+p and 2α+2p particle-decay channels in the 10C compound nucleus; deduced destruction of 7Be during the Big Bang nucleosynthesis.
doi: 10.1103/PhysRevC.93.045804
2016HA37 Phys.Rev. C 94, 055803 (2016) T.Hayakawa, Y.Toh, M.Huang, T.Shizuma, A.Kimura, S.Nakamura, H.Harada, N.Iwamoto, S.Chiba, T.Kajino Measurement of the isomer production ratio for the 112Cd(n, γ)113Cd reaction using neutron beams at J-PARC NUCLEAR REACTIONS 112Cd(n, γ), E<5 keV; measured Eγ, Iγ, time-of-flight spectra, nγ-coin, γ-ray intensity ratios versus neutron energy using the Accurate Neutron-Nucleus Reaction Measurement Instrument (ANNRI) at J-PARC facility; deduced isomer production ratio as function of neutron energies, including neutron resonances. Relevance to s-process branching point for nucleosynthesis.
doi: 10.1103/PhysRevC.94.055803
2016SH37 Phys.Rev. C 94, 045804 (2016) J.W.Shin, M.-K.Cheoun, T.-S.Park, T.Kajino New neutrino source for the study of solar neutrino physics in the vacuum-matter transition region NUCLEAR REACTIONS 27Al(p, n)27Si, E=5-20 MeV; analyzed σ(E) data with hadronic models of GEANT4 and the nuclear data model; calculated normalized energy distribution of electron-neutrinos through the radioactive decay of 27Si in 0-5 MeV range, close to solar neutrino physics; proposed target systems required for future solar neutrino experiments. 2H(ν, e-)2p, (ν, ν), 37Cl(ν, e-)37Ar, 71Ga(ν, e-)71Ge, E=0-5 MeV; calculated total reaction rates by electron-neutrino spectra, expected event rates and their ratios for LENA-type detector.
doi: 10.1103/PhysRevC.94.045804
2015CH18 J.Phys.(London) G42, 345102 (2015) M.-K.Cheoun, K.S.Kim, H.Kim, W.Y.So, T.Maruyama, T.Kajino In-medium effect with muon-neutrino and anti-muon-neutrino quasi-elastic scattering from 12C nucleons
doi: 10.1088/0954-3899/42/4/045102
2015LO04 Phys.Rev.Lett. 114, 192501 (2015) G.Lorusso, S.Nishimura, Z.Y.Xu, A.Jungclaus, Y.Shimizu, G.S.Simpson, P.-A.Soderstrom, H.Watanabe, F.Browne, P.Doornenbal, G.Gey, H.S.Jung, B.Meyer, T.Sumikama, J.Taprogge, Zs.Vajta, J.Wu, H.Baba, G.Benzoni, K.Y.Chae, F.C.L.Crespi, N.Fukuda, R.Gernhauser, N.Inabe, T.Isobe, T.Kajino, D.Kameda, G.D.Kim, Y.-K.Kim, I.Kojouharov, F.G.Kondev, T.Kubo, N.Kurz, Y.K.Kwon, G.J.Lane, Z.Li, A.Montaner-Piza, K.Moschner, F.Naqvi, M.Niikura, H.Nishibata, A.Odahara, R.Orlandi, Z.Patel, Zs.Podolyak, H.Sakurai, H.Schaffner, P.Schury, S.Shibagaki, K.Steiger, H.Suzuki, H.Takeda, A.Wendt, A.Yagi, K.Yoshinaga β-Decay Half-Lives of 110 Neutron-Rich Nuclei across the N=82 Shell Gap: Implications for the Mechanism and Universality of the Astrophysical r Process RADIOACTIVITY 134,135,136,137,138,139Sn, 128,129,130,131,132,133,134,135,136,137In, 126,127,128,129,130,131,132,133,134Cd, 124,125,126,127,128,129,130,131,132Ag, 121,122,123,124,125,126,127,128,129Pd, 118,119,120,121,122,123,124,125,126,127Rh, 116,117,118,119,120,121,122,123,124Ru, 112,113,114,115,116,117,118,119,120,121Tc, 109,110,111,112,113,114,115,116,117,118Mo, 107,108,109,110,111,112,113,114,115Nb, 106,107,108,109,110,111,112Zr, 104,105,106,107,108,109Y, 103,104,105,106Sr, 102,103Rb(β-) [from Be(238U, X), E=345 MeV/nucleon]; measured decay products, Eγ, Iγ; deduced T1/2; Calculated r-process abundances. Comparison with available data.
doi: 10.1103/PhysRevLett.114.192501
2014KO41 Eur.Phys.J. A 50, 136 (2014) T.Komatsubara, S.Kubono, T.Hayakawa, T.Shizuma, A.Ozawa, Y.Ito, Y.Ishibashi, T.Moriguchi, H.Yamaguchi, D.Kahl, S.Hayakawa, D.N.Binh, A.A.Chen, J.Chen, K.Setoodehnia, T.Kajino Excited states above the proton threshold in 26Si
doi: 10.1140/epja/i2014-14136-4
2014MA13 Phys.Rev. C 89, 035801 (2014) T.Maruyama, J.Hidaka, T.Kajino, N.Yasutake, T.Kuroda, T.Takiwaki, M.-K.Cheoun, C.-Y.Ryu, G.J.Mathews Rapid spin deceleration of magnetized protoneutron stars via asymmetric neutrino emission
doi: 10.1103/PhysRevC.89.035801
2013CH40 Phys.Rev. C 87, 065502 (2013) M.K.Cheoun, K.S.Choi, K.S.Kim, K.Saito, T.Kajino, K.Tsushima, T.Maruyama Effects of the density-dependent weak form factors on the neutrino reaction via neutral current for the nucleon in nuclear matter and 12C NUCLEAR REACTIONS 12C(ν, ν'), (ν-bar, ν-bar'), E<80 MeV; calculated density-dependent form factors for electron neutrino and electron antineutrino collisions with 12C, σ(E). Large asymmetry in the antineutrino cross sections due to difference in helicities of neutrino and antineutrino. Quark-meson-coupling (QMC) model.
doi: 10.1103/PhysRevC.87.065502
2013FA04 J.Phys.:Conf.Ser. 445, 012025 (2013) M.Famiano, R.N.Boyd, T.Kajino, B.Meyer, Y.Motizuki, I.Roederer Implementing the r-process in metal-poor stars via black hole collapse and relevance to the light element enhancement
doi: 10.1088/1742-6596/445/1/012025
2013HE21 Phys.Lett. B 725, 287 (2013) J.J.He, S.Z.Chen, C.E.Rolfs, S.W.Xu, J.Hu, X.W.Ma, M.Wiescher, R.J.de Boer, T.Kajino, M.Kusakabe, L.Y.Zhang, S.Q.Hou, X.Q.Yu, N.T.Zhang, G.Lian, Y.H.Zhang, X.H.Zhou, H.S.Xu, G.Q.Xiao, W.L.Zhan A drop in the 6Li(p, γ)7Be reaction at low energies NUCLEAR REACTIONS 6Li(p, γ), E(cm)<1 MeV; measured reaction products, Eγ, Iγ; deduced S-factors, positive-parity resonance. Comparison with available data, SUSY assisted Big-bang Nucleosynthesis models.
doi: 10.1016/j.physletb.2013.07.044
2013KA31 J.Phys.:Conf.Ser. 445, 012024 (2013) Nuclear weak interactions, supernova nucleosynthesis and neutrino oscillation
doi: 10.1088/1742-6596/445/1/012024
2013MA52 J.Phys.:Conf.Ser. 445, 012023 (2013) G.J.Mathews, M.Meixner, J.P.Olson, I.-S.Suh, T.Kajino, T.Maruyama, J.Hidaka, C.-Y.Ryu, M.-K.Cheoun, N.Q.Lan Updates of the nuclear equation of state for core-collapse supernovae and neutron stars: effects of 3-body forces, QCD, and magnetic fields
doi: 10.1088/1742-6596/445/1/012023
2013SU17 J.Phys.(London) G40, 085101 (2013) Element synthesis in the supernova environment and neutrino oscillations NUCLEAR REACTIONS 12,13C, 4He, 56Fe, 56Ni(ν, E), (ν, ν'), E<60 MeV; calculated σ, production yields, Gamow-Teller strengths. GXPF1J and KB3G interactions, comparison with experimental data.
doi: 10.1088/0954-3899/40/8/083101
2012CH25 Phys.Rev. C 85, 065807 (2012) M.-K.Cheoun, E.Ha, T.Hayakawa, S.Chiba, K.Nakamura, T.Kajino, G.J.Mathews Neutrino induced reactions for ν-process nucleosynthesis of 92Nb and 98Tc NUCLEAR REACTIONS 92Zr(ν, e)92Nb, 93Nb[ν, ν'n)92Nb, 93Nb(ν-bar, ν-bar'n]92Nb, 98Mo(ν, e)98Tc, 99Ru(ν, ν'p)98Tc, 99Ru(ν-bar, ν-bar'p)98Tc, E<80 MeV; calculated B(GT) strength distributions, energy and temperature dependent σ in charge current (CC) and neutral current (NC) reactions. Quasiparticle random phase approximation calculations. Nucleosynthesis of odd-odd 98Tc and 92Nb nuclei by the ν-process in core-collapse supernovae.
doi: 10.1103/PhysRevC.85.065807
2012CH38 Prog.Theor.Phys.(Kyoto), Suppl. 196, 476 (2012) Neutrino Induced Reactions with the Nuclei in Core Collapsing Supernovae NUCLEAR REACTIONS 40Ar, 138Ba, 139La, 181Ta, 180Hf(ν, e), E not given; calculated σ, Gamow-Teller strength distributions. QRPA calculations, comparison with experimental data.
doi: 10.1143/PTPS.196.476
2012CH42 Eur.Phys.J. A 48, 137 (2012) High-lying excited states in Gamow Teller strength and their roles in neutrino reactions NUCLEAR REACTIONS 40Ar(ν, ν'), (ν, e), (ν-bar, e+), E=0-80 MeV; calculated B(GT) strength distribution, σ. Compared with data. NUCLEAR STRUCTURE 90Zr, 90Nb; calculated B(GT) strength distribution below ≈ 20 MeV using QRPA and pnQRPA.
doi: 10.1140/epja/i2012-12137-y
2012NI06 Phys.Rev. C 85, 048801 (2012) N.Nishimura, T.Kajino, G.J.Mathews, S.Nishimura, T.Suzuki Impact of new β-decay half-lives on r-process nucleosynthesis ATOMIC MASSES A=110-120; analyzed effect of newly measured β decay half-lives of neutron-rich nuclei on r-process nucleosynthesis, thermodynamic properties, elemental abundance distributions, integrated mass-averaged total final abundance distributions of r-process elements. MHD (magnetohydrodynamic) supernova model, and FRDM, RIBF, and RIBF networks.
doi: 10.1103/PhysRevC.85.048801
2012RY01 Phys.Rev. C 85, 045803 (2012) C.-Y.Ryu, T.Maruyama, T.Kajino, G.J.Mathews, M.-K.Cheoun Spin change of a proto-neutron star by the emission of neutrinos
doi: 10.1103/PhysRevC.85.045803
2012SU02 Phys.Rev. C 85, 015802 (2012) T.Suzuki, T.Yoshida, T.Kajino, T.Otsuka β decays of isotones with neutron magic number of N=126 and r-process nucleosynthesis RADIOACTIVITY 204Pt, 205Au, 206Hg(β-); N=126, Z=64-73(β-); calculated half-lives using shell model, Gamow-Teller and first-forbidden transitions, r process nucleosynthesis, elemental abundance.
doi: 10.1103/PhysRevC.85.015802
2012SU15 Phys.Rev. C 86, 015502 (2012) T.Suzuki, A.B.Balantekin, T.Kajino Neutrino capture on 13C NUCLEAR REACTIONS 12C(ν, e)12N, E=20-60 MeV; 13C(ν, e)13N, E=2-20 MeV; 13C(ν, ν'), E=2-20 MeV; calculated σ(E), B(GT), B(M1) using shell-model calculations. Comparison with experimental data. Discussed implications for the scintillation counter-based experiments to measure electron neutrinos from a core-collapse supernova.
doi: 10.1103/PhysRevC.86.015502
2012SU20 Prog.Theor.Phys.(Kyoto), Suppl. 196, 382 (2012) T.Suzuki, M.Honma, T.Otsuka, T.Kajino Gamow-Teller Strengths in Ni Isotopes and Nuclear Weak Processes RADIOACTIVITY 56,58,60Ni(EC); calculated electron capture rates at high densities in stellar environment, Gamow-Teller strengths. GXPF1J, KB3G interactions, comparison with experimental data.
doi: 10.1143/PTPS.196.382
2011CH07 Phys.Rev. C 83, 028801 (2011) Reactions on 40Ar involving solar neutrinos and neutrinos from core-collapsing supernovae NUCLEAR REACTIONS 40Ar(ν, e+)40Cl, 40Ar(ν, ν'), E=0-80 MeV; calculated σ, G-T strengths for solar neutrinos and neutrinos from core-collapsing supernovae using quasiparticle random phase approximation (QRPA).
doi: 10.1103/PhysRevC.83.028801
2011KU30 J.Phys.:Conf.Ser. 312, 042012 (2011) M.Kusakabe, T.Kajino, G.J.Mathews SUSY-catalyzed big bang nucleosynthesis as a solution of lithium problems
doi: 10.1088/1742-6596/312/4/042012
2011RY01 Phys.Rev. C 83, 018802 (2011) C.Y.Ryu, T.Maruyama, T.Kajino, M.-K.Cheoun Properties of a proto-neutron star with smeared trapped neutrinos
doi: 10.1103/PhysRevC.83.018802
2011SU04 Prog.Part.Nucl.Phys. 66, 385 (2011) T.Suzuki, M.Honma, T.Yoshida, H.Mao, T.Kajino, T.Otsuka Spin-dependent nuclear weak processes and nucleosynthesis in stars NUCLEAR REACTIONS 58Ni(E-, ν)58Co, 60Ni(E-, ν)60Co, 56Co(E-, ν)56Fe, 60Co(E-, ν)60Fe, E<100 keV; 56Ni(ν, p)55Co, 56Ni(ν, γ)56Ni, 56Ni(ν, α)52Fe, 56Ni(ν, n)55Ni, E< 10 MeV; calculated electron capture rates, σ, 55Mn yields. GXPF1A and KB3G effective interactions. RADIOACTIVITY 190Gd, 191Tb, 192Dy, 193Ho, 194Er, 195Tm, 196Yb, 197Lu, 198Hf, 199Ta(β-); calculated T1/2. GXPF1A and KB3G effective interactions, N=126 waiting point.
doi: 10.1016/j.ppnp.2011.01.039
2011SU09 Phys.Rev. C 83, 044619 (2011) T.Suzuki, M.Honma, H.Mao, T.Otsuka, T.Kajino Evaluation of electron capture reaction rates in Ni isotopes in stellar environments NUCLEAR REACTIONS 56,58,60,62,64Ni(e, ν), E at T9=1-10; evaluated Gamow-Teller B(GT) strengths, and electron capture rates at high densities and high temperatures during the core-collapse and postbounce explosive nucleosynthesis in supernovae using shell-model in the fp shell with GXPF1J interaction. Comparison with experimental data.
doi: 10.1103/PhysRevC.83.044619
2011SU27 J.Phys.:Conf.Ser. 312, 042023 (2011) T.Suzuki, T.Yoshida, M.Honma, H.Mao, T.Otsuka, T.Kajino Gamow-Teller and First-Forbidden Transition Strengths in Astrophysical Processes NUCLEAR STRUCTURE 54,56Fe, 56,58,60,62,64Ni; calculated β-decay B(GT) using shell model with GXPF1 and KB3G Hamiltonians. Compared with published data. NUCLEAR REACTIONS 56,58,60Ni(e-, ν), E≈100 keV-1 MeV; calculated capture rates. 58,60Ni(e-, ν), E≈1-10 MeV; calculated β-decay B(GT). Shell model with GXPF1 and KB3G Hamiltonians, compared with data.
doi: 10.1088/1742-6596/312/4/042023
2010CH05 Phys.Rev. C 81, 028501 (2010) M.-K.Cheoun, E.Ha, S.Y.Lee, K.S.Kim, W.Y.So, T.Kajino Neutrino reactions on 12C by the quasiparticle random-phase approximation (QRPA) NUCLEAR REACTIONS 12C(ν, e)12N, E=0-80 MeV; calculated σ using quasiparticle random phase approximation calculations. Comparison with experimental data.
doi: 10.1103/PhysRevC.81.028501
2010CH40 Phys.Rev. C 82, 035504 (2010) M.-K.Cheoun, E.Ha, T.Hayakawa, T.Kajino, S.Chiba Neutrino reactions on 138La and 180Ta via charged and neutral currents by the quasiparticle random-phase approximation NUCLEAR REACTIONS 139La, 181Ta(ν, ν'), 138Ba(ν, e)138La, 180Hf(ν, e)180Ta, E=0-80 MeV; calculated σ by neutral and charged current reactions using standard quasi-particle random phase approximation (QRPA) with neutron-proton pairing and neutron-neutron and proton-proton pairing correlations. Astrophysical relevance. RADIOACTIVITY 138Ba, 180Hf(β-); calculated Gamow-Teller strength distribution B(GT) using QRPA.
doi: 10.1103/PhysRevC.82.035504
2010HA13 Phys.Rev. C 81, 052801 (2010) T.Hayakawa, T.Kajino, S.Chiba, G.J.Mathews New estimate for the time-dependent thermal nucleosynthesis of 180Tam NUCLEAR STRUCTURE 180Ta, 180mTa; calculated time-dependent production and transition widths of 180gTa 180mTa in ν and γ processes in supernovae. Comparison with production of 138La in ν process.
doi: 10.1103/PhysRevC.81.052801
2010HA27 Phys.Rev. C 82, 058801 (2010) T.Hayakawa, P.Mohr, T.Kajino, S.Chiba, G.J.Mathews Reanalysis of the (J=5) state at 592 keV in 180Ta and its role in the υ-process nucleosynthesis of 180Ta in supernovae NUCLEAR STRUCTURE 180mTa; analyzed production and freeze out of 180mTa through the influence of a spin 5 state at 592 keV. Implication for coproduction by neutrino nucleosynthesis with an electron neutrino temperature of kT AP 4 MeV. 180Ta; discussed low-K and high-K rotational band structures; deduced astrophysical reaction rates.
doi: 10.1103/PhysRevC.82.058801
2009HA11 Phys.Lett. B 674, 276 (2009) T.Hashimoto, H.Ishiyama, Y.X.Watanabe, Y.Hirayama, N.Imai, H.Miyatake, S.C.Jeong, M.-H.Tanaka, N.Yoshikawa, T.Nomura, S.Mitsuoka, K.Nishio, T.K.Sato, A.Osa, S.Ichikawa, M.Matsuda, H.Ikezoe, S.K.Das, Y.Mizoi, T.Fukuda, A.Sato, T.Shimoda, K.Otsuki, T.Kajino A new measurement of the astrophysical 8Li(d, t)7Li reaction NUCLEAR REACTIONS 2H(8Li, t), E=0.18, 0.24, 0.30, 0.40, 0.46, 0.60, 0.75 MeV/nucleon; measured charged-particle spectra, σ, σ(θ), σ(E); deduced 7Li excitation energy spectra, astrophysical reaction rate. Comparison with other data.
doi: 10.1016/j.physletb.2009.03.031
2009HA14 Phys.Rev. C 79, 059802 (2009) T.Hayakawa, T.Shizuma, T.Kajino, K.Ogawa, H.Nakada Reply on "138La-138Ce-136Ce nuclear cosmochronometer of the supernova neutrino process"
doi: 10.1103/PhysRevC.79.059802
2009HA48 Astrophys.J. 707, 859 (2009) T.Hayakawa, T.Shizuma, S.Chiba, T.Kajino, Y.Hatsukawa, N.Iwamoto, N.Shinohara, H.Harada Neutron Capture Cross Section to 113Cd Isomer and s-Process Contribution to Rare p-Nuclide 115Sn NUCLEAR REACTIONS 112Cd(n, γ), E thermal; measured reaction products, Eγ, Iγ; deduced isomeric state s, resonance integral. Comparison with JENDL-3.3 evaluated nuclear data library, Hauser-Feshbach statistical model calculations.
doi: 10.1088/0004-637X/707/2/859
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
2008CH05 Phys.Rev. C 77, 015809 (2008) S.Chiba, H.Koura, T.Hayakawa, T.Maruyama, T.Kawano, T.Kajino Direct and semi-direct capture in low-energy (n, γ) reactions of neutron-rich tin isotopes and its implications for r-process nucleosynthesis NUCLEAR REACTIONS 16O(n, γ), E=0.01-10 MeV; 124,126,128,130,134,136,138Sn(n, γ), E=30 keV; 122Sn(n, γ), E=1 keV-20 MeV; 208Pb(n, γ), E=0-20 MeV; calculated neutron capture cross sections. 132Sn(n, γ), E=1 keV-20 MeV; calculated neutron capture cross sections, reaction rates. 132,133Sn; calculated levels, J, π, compared with experiment.
doi: 10.1103/PhysRevC.77.015809
2008FA01 J.Phys.(London) G35, 025203 (2008) M.A.Famiano, R.N.Boyd, T.Kajino, K.Otsuki, M.Terasawa, G.J.Mathews Effects of β-decays of excited-state nuclei on the astrophysical r-process
doi: 10.1088/0954-3899/35/2/025203
2008HA20 Phys.Rev. C 77, 065802 (2008) T.Hayakawa, T.Shizuma, T.Kajino, K.Ogawa, H.Nakada 138La-138Ce-136Ce nuclear cosmochronometer of the supernova neutrino process NUCLEAR STRUCTURE 138La, 140Pr; calculated levels, J, π. Evaluated the 138La-138Ce-136Ce chain as a nuclear cosmochronometer. Comparison with experimental data.
doi: 10.1103/PhysRevC.77.065802
2008HA21 Phys.Rev. C 77, 068801 (2008) T.Hayakawa, T.Shizuma, S.Miyamoto, S.Amano, K.Horikawa, K.Ishihara, M.Mori, K.Kawase, M.Kando, N.Kikuzawa, S.Chiba, T.Mochizuki, T.Kajino, M.Fujiwara Half-life of the 164Ho by the (γ, n) reaction from laser Compton scattering gamma rays at the electron storage ring NewSUBARU NUCLEAR REACTIONS 165Ho(γ, n), E=3.3-16.7 MeV; measured Eγ, Iγ, half-life; calculated σ. 164Ho; deduced levels, J, π. RADIOACTIVITY 164Ho(β+), (β-); measured Eγ, Iγ. 164Dy, 164Er; deduced levels, J, π.
doi: 10.1103/PhysRevC.77.068801
2008KU08 Astrophys.J. 680, 846 (2008) M.Kusakabe, T.Kajino, R.N.Boyd, T.Yoshida, G.J.Mathews The X- solution to the 6Li and 7Li big bang nucleosynthesis problems
doi: 10.1086/588548
2007KU31 Phys.Rev. D 76, 121302 (2007) M.Kusakabe, T.Kajino, R.N.Boyd, T.Yoshida, G.J.Mathews Simultaneous solution to the 6Li and 7Li big bang nucleosynthesis problems from a long-lived negatively charged leptonic particle
doi: 10.1103/PhysRevD.76.121302
2007SU08 Prog.Part.Nucl.Phys. 59, 486 (2007) T.Suzuki, S.Chiba, Ta.Yoshida, K.Higashiyama, M.Honma, T.Kajino, T.Otsuka Advances in shell-model calculations and neutrino-induced reactions NUCLEAR REACTIONS 12C(ν, ν'), (ν, e), (ν, ν'p), (ν, ν'n), 56Fe(ν, e), 58.60,62,64Ni(ν, e), E not given; calculated supernova neutrino induced cross sections using new shell model hamiltonian.
doi: 10.1016/j.ppnp.2007.01.013
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
2006HA51 Phys.Rev.C 74, 065802 (2006) T.Hayakawa, S.Miyamoto, Y.Hayashi, K.Kawase, K.Horikawa, S.Chiba, K.Nakanishi, H.Hashimoto, T.Ohta, M.Kando, T.Mochizuki, T.Kajino, M.Fujiwara Half-life of 184Re populated by the (γ, n) reaction from laser Compton scattering γ rays at the electron storage ring NewSUBARU RADIOACTIVITY 184,184mRe(EC), (β+) [from 185Re(γ, n)]; measured Eγ, Iγ, T1/2. 184W deduced transitions. NUCLEAR REACTIONS 185Re(γ, n), E ≈ 2-20 MeV; measured β-delayed Eγ, Iγ; deduced isomer yield ratio.
doi: 10.1103/PhysRevC.74.065802
2006SU15 Phys.Rev. C 74, 034307 (2006) T.Suzuki, S.Chiba, T.Yoshida, T.Kajino, T.Otsuka Neutrino-nucleus reactions based on new shell model Hamiltonians NUCLEAR REACTIONS 12C(ν, ν'), (ν, e), E=spectrum; calculated σ for decay-at-rest neutrinos. 4He, 12C(ν, ν'), (ν, e), E=spectrum; 12C(ν, ν'n), (ν, ν'p), (ν, ν'α), E=spectrum; calculated σ, branching ratios for supernova neutrinos. Shell model, implications for isotope production in supernovae discussed.
doi: 10.1103/PhysRevC.74.034307
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
2005HA60 Astrophys.J. 628, 533 (2005) T.Hayakawa, T.Shizuma, T.Kajino, S.Chiba, N.Shinohara, T.Nakagawa, T.Arima New s-Process Path and Its Implications for a 187Re-187Os Nucleo-Cosmochronometer NUCLEAR REACTIONS 185Re(n, γ), E=thermal; measured isomer yield ratio. Activation technique, astrophysical implications discussed.
doi: 10.1086/430198
2005HO25 Nucl.Phys. A758, 296c (2005) S.Honda, W.Aoki, T.Kajino, H.Ando, T.C.Beers The Origin of Light Neutron-Capture Elements in Very Metal-Poor Stars
doi: 10.1016/j.nuclphysa.2005.05.052
2005LI19 Phys.Rev. C 71, 052801 (2005) Z.H.Li, W.P.Liu, X.X.Bai, B.Guo, G.Lian, S.Q.Yan, B.X.Wang, S.Zeng, Y.Lu, J.Su, Y.S.Chen, K.S.Wu, N.C.Shu, T.Kajino The 8Li(d, p)9Li reaction and the astrophysical 8Li(n, γ)9Li reaction rate NUCLEAR REACTIONS 2H(8Li, 9Li), E=39 MeV; measured particle spectra, σ(θ). 8Li(n, γ), E=low; deduced astrophysical reaction rates.
doi: 10.1103/PhysRevC.71.052801
2005MA06 Phys.Rev. D 71, 021302 (2005) G.J.Mathews, T.Kajino, T.Shima Big bang nucleosynthesis with a new neutron lifetime
doi: 10.1103/PhysRevD.71.021302
2005NA38 At.Data Nucl.Data Tables 91, 77 (2005) T.Nakagawa, S.Chiba, T.Hayakawa, T.Kajino Maxwellian-average neutron-induced reaction cross sections and astrophysical reaction rates for kT = 1 keV to 1 MeV calculated from microscopic neutron cross section library JENDL-3.3 COMPILATION Z=1-96; A=1-247; compiled, analyzed Maxwellian averaged neutron capture σ, neutron-induced fission σ, astrophysical reaction rates. Other neutron-induced reactions discussed.
doi: 10.1016/j.adt.2005.08.002
2005OT02 Nucl.Phys. A758, 316c (2005) K.Otsuki, G.J.Mathews, T.Ashenfelter, T.Kajino Neutron-capture elements in Galactic globular clusters
doi: 10.1016/j.nuclphysa.2005.05.057
2005SA47 Nucl.Phys. A758, 639c (2005) T.Sasaqui, T.Kajino, K.Otsuki, G.J.Mathews, T.Nakamura Light-Mass Cluster Reactions in Supernova R-Process
doi: 10.1016/j.nuclphysa.2005.05.115
2005SA58 Astrophys.J. 634, 534 (2005) T.Sasaqui, T.Kajino, A.B.Balantekin Supernova neutrino effects on r-process nucleosynthesis in black hole formation
doi: 10.1086/491730
2005YA19 Nucl.Phys. A758, 791c (2005) D.G.Yamazaki, K.Ichiki, T.Kajino Primordial Magnetic Field at the Photon Last Scattering Surface
doi: 10.1016/j.nuclphysa.2005.05.194
2005YO09 Nucl.Phys. A758, 35c (2005) Supernova Neutrino Process and its Impact on the Galactic Chemical Evolution of the Light Elements
doi: 10.1016/j.nuclphysa.2005.05.011
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
2004KA49 Prog.Theor.Phys.(Kyoto), Suppl. 154, 301 (2004) T.Kajino, T.Sasaqui, K.Otsuki, K.Ichiki, M.Orito, G.J.Mathews, S.Chiba Fusion Reactions in Supernovae and the Early Universe
doi: 10.1143/PTPS.154.301
2003FA11 Nucl.Phys. A718, 392c (2003) M.A.Famiano, R.N.Boyd, T.Kajino Light Element Nucleosynthesis From Jet-Cloud Interactions in Active Galactic Nuclei
doi: 10.1016/S0375-9474(03)00808-X
2003HO20 Nucl.Phys. A718, 674c (2003) S.Honda, W.Aoki, H.Ando, T.Kajino New Detections of r-Process Elements in Extremely Metal-Poor Stars with Subaru/HDS
doi: 10.1016/S0375-9474(03)00885-6
2003IC02 Nucl.Phys. A718, 383c (2003) K.Ichiki, M.Yahiro, T.Kajino, M.Orito, G.J.Mathews Constraints on the Nature of Cosmological Constant - from Big Bang Nucleosynthesis and CMB anisotropies -
doi: 10.1016/S0375-9474(03)00805-4
2003IC03 Nucl.Phys. A718, 386c (2003) K.Ichiki, M.Yahiro, T.Kajino, M.Orito, G.J.Mathews Observational Constraints on Dark Radiation in Brane Cosmology
doi: 10.1016/S0375-9474(03)00811-X
2003IW03 Nucl.Phys. A718, 193c (2003) N.Iwamoto, G.J.Mathews, M.Y.Fujimoto, T.Kajino, W.Aoki A New Model for s-Process Nucleosynthesis in Low-Mass, Low-Metallicity AGB Stars
doi: 10.1016/S0375-9474(03)00714-0
2003IW04 Nucl.Phys. A719, 57c (2003) N.Iwamoto, T.Kajino, G.J.Mathews, M.Y.Fujimoto Nucleosynthesis in low-mass, low-metallicity AGB stars
doi: 10.1016/S0375-9474(03)00958-8
2003KA52 Nucl.Phys. A718, 295c (2003) Quest for Supernova R-Process: New Data in Astronomy and Nuclear Physics, and Theoretical Modeling
doi: 10.1016/S0375-9474(03)00730-9
2003KA53 Nucl.Phys. A718, 659c (2003) S.Kawanomoto, K.T.Suzuki, H.Ando, T.Kajino First detection of 7Li/6Li-ratio in the interstellar medium beyond the Solar-system, and its impact on primordial 7Li
doi: 10.1016/S0375-9474(03)00880-7
2003MA43 Nucl.Phys. A718, 15c (2003) G.J.Mathews, K.Ichiki, T.Kajino, M.Orito, M.Yahiro New Paradigms for Primordial Nucleosynthesis
doi: 10.1016/S0375-9474(03)00674-2
2003OR02 Nucl.Phys. A719, 1c (2003) M.Orito, T.Kajino, K.Ichiki, M.Yahiro, G.J.Mathews, Y.Wang BBN and CMB constraints on universal lepton asymmetry, quintessential inflation, and brane world cosmology
doi: 10.1016/S0375-9474(03)00950-3
2003OT01 Nucl.Phys. A718, 677c (2003) K.Otsuki, G.J.Mathews, T.Kajino Nuclear Cosmochronometer and Universality in the r-Process Abundance Distribution
doi: 10.1016/S0375-9474(03)00886-8
2003OT02 Nucl.Phys. A721, 1024c (2003) K.Otsuki, G.J.Mathews, T.Kajino, S.Honda, W.Aoki, A.Aprahamian, K.Vaughan Nuclear Cosmochronometry and Universality in the r-Process Abundances
doi: 10.1016/S0375-9474(03)01276-4
2003TE10 Nucl.Phys. A718, 641c (2003) M.Terasawa, K.Sumiyoshi, T.Kajino The r-Process in Neutrino-Driven Winds from a Typical Neutron Star with M = 1.4M(solar)
doi: 10.1016/S0375-9474(03)00910-2
2002KA38 Nucl.Phys. A704, 165c (2002) T.Kajino, S.Wanajo, G.J.Mathews R-Process Nucleosynthesis in Core-Collapse Supernova Explosion
doi: 10.1016/S0375-9474(02)00777-7
2002KA78 Prog.Theor.Phys.(Kyoto), Suppl. 146, 247 (2002) Recent Progress in Cosmology and Nuclear Astrophysics
doi: 10.1143/PTPS.146.247
2002SU19 Nucl.Phys. A709, 467 (2002) K.Sumiyoshi, H.Utsunomiya, S.Goko, T.Kajino Astrophysical Reaction Rate for α(αn, γ)9Be by Photodisintegration NUCLEAR REACTIONS 9Be(γ, n), E ≈ 1.5-4.5 MeV; measured σ; deduced resonance parameters, astrophysical reaction rate for α(αn, γ).
doi: 10.1016/S0375-9474(02)01058-8
2002TE14 Astrophys.J. 578, L137 (2002) M.Terasawa, K.Sumiyoshi, S.Yamada, H.Suzuki, T.Kajino r-Process nucleosynthesis in neutrino-driven winds from a typical neutron star with M = 1.4 M(solar)
doi: 10.1086/344698
2001AO03 Astrophys.J. 561, 346 (2001) W.Aoki, S.G.Ryan, J.E.Norris, T.C.Beers, H.Ando, N.Iwamoto, T.Kajino, G.J.Mathews, M.Y.Fujimoto Neutron Capture Elements in s-Process-Rich, Very Metal-Poor Stars
doi: 10.1086/323230
2001FA08 Astrophys.J. 547, L21 (2001) M.Famiano, J.Vandegrif, R.N.Boyd, T.Kajino, P.Osmer Production of 2H, 3He, and 7Li from Interactions between Jets and Clouds
doi: 10.1086/318879
2001OR03 Nucl.Phys. A688, 17c (2001) M.Orito, T.Kajino, G.J.Mathews, R.N.Boyd Primordial Nucleosynthesis and Neutrinos with Mass and Degeneracy
doi: 10.1016/S0375-9474(01)00660-1
2001SU12 Nucl.Phys. A688, 478c (2001) K.Sumiyoshi, M.Terasawa, H.Suzuki, S.Yamada, H.Toki, G.J.Mathews, T.Kajino Relativistic Simulations of Supernovae and the r-Process; A new relativistic EOS and nuclear reaction network
doi: 10.1016/S0375-9474(01)00761-8
2001SU23 Astrophys.J. 562, 880 (2001) K.Sumiyoshi, M.Terasawa, G.J.Mathews, T.Kajino, S.Yamada, H.Suzuki r-Process in Prompt Supernova Explosions Revisited
doi: 10.1086/323524
2001TE04 Nucl.Phys. A688, 581c (2001) M.Terasawa, K.Sumiyoshi, T.Kajino, I.Tanihata, G.J.Mathews, K.Langanke New Nuclear Reaction Flow During r-Process Nucleosynthesis in Supernovae: The critical role of light neutron-rich nuclei
doi: 10.1016/S0375-9474(01)00795-3
2001TE05 Astrophys.J. 562, 470 (2001) M.Terasawa, K.Sumiyoshi, T.Kajino, G.J.Mathews, I.Tanihata New Nuclear Reaction Flow During r-Process Nucleosynthesis in Supernova: Critical role of light, neutron-rich nuclei
doi: 10.1086/323526
1998KA10 Nucl.Phys. A629, 538c (1998) Neutrinos and Big-Bang Nucleosynthesis
doi: 10.1016/S0375-9474(97)00734-3
1997KA46 Nucl.Phys. A621, 572c (1997) Big-Bang vs. Galactic Origin of Elements in Metal-Deficient Stars
doi: 10.1016/S0375-9474(97)00305-9
1997KU19 Nucl.Phys. A621, 195c (1997) S.Kubono, M.Hosaka, P.Strasser, V.Guimaraes, S.C.Jeong, I.Katayama, T.Miyachi, T.Nomura, M.H.Tanaka, Y.Fuchi, H.Kawashima, S.Kato, C.C.Yun, H.Orihara, T.Niizeki, H.Miyatake, T.Shimoda, T.Kajino, S.Wanajo Study of the Early Stage of the Rapid-Proton Process
doi: 10.1016/S0375-9474(97)00237-6
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