NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = H.Nagakura Found 6 matches. 2023FU01 Prog.Part.Nucl.Phys. 129, 104018 (2023) Nuclei in core-collapse supernovae engine
doi: 10.1016/j.ppnp.2022.104018
2023SU01 Prog.Theor.Exp.Phys. 2023, 013E02 (2023) K.Sumiyoshi, S.Furusawa, H.Nagakura, A.Harada, H.Togashi, K.Nakazato, H.Suzuki Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
doi: 10.1093/ptep/ptac167
2020MI13 Phys.Rev.Lett. 125, 122501 (2020) S.Michimasa, M.Kobayashi, Y.Kiyokawa, S.Ota, R.Yokoyama, D.Nishimura, D.S.Ahn, H.Baba, G.P.A.Berg, M.Dozono, N.Fukuda, T.Furuno, E.Ideguchi, N.Inabe, T.Kawabata, S.Kawase, K.Kisamori, K.Kobayashi, T.Kubo, Y.Kubota, C.S.Lee, M.Matsushita, H.Miya, A.Mizukami, H.Nagakura, H.Oikawa, H.Sakai, Y.Shimizu, A.Stolz, H.Suzuki, M.Takaki, H.Takeda, S.Takeuchi, H.Tokieda, T.Uesaka, K.Yako, Y.Yamaguchi, Y.Yanagisawa, K.Yoshida, S.Shimoura Mapping of a New Deformation Region around 62Ti ATOMIC MASSES 61,62,63,64V, 58,59,60,61,62Ti, 55,56,57,58,59,60Sc; measured time of flight, charge, magnetic rigidity; deduced mass excesses. Comparison with AME2016 and available data. RADIOACTIVITY 59,61Ti, 56,58Sc(IT) [from 9Be(70Zn, X), E=345 MeV/nucleon]; measured decay products, Eγ, Iγ; deduced γ-ray energies and intensities, T1/2. Comparison with available data.
doi: 10.1103/PhysRevLett.125.122501
2018MI08 Phys.Rev.Lett. 121, 022506 (2018) S.Michimasa, M.Kobayashi, Y.Kiyokawa, S.Ota, D.S.Ahn, H.Baba, G.P.A.Berg, M.Dozono, N.Fukuda, T.Furuno, E.Ideguchi, N.Inabe, T.Kawabata, S.Kawase, K.Kisamori, K.Kobayashi, T.Kubo, Y.Kubota, C.S.Lee, M.Matsushita, H.Miya, A.Mizukami, H.Nagakura, D.Nishimura, H.Oikawa, H.Sakai, Y.Shimizu, A.Stolz, H.Suzuki, M.Takaki, H.Takeda, S.Takeuchi, H.Tokieda, T.Uesaka, K.Yako, Y.Yamaguchi, Y.Yanagisawa, R.Yokoyama, K.Yoshida, S.Shimoura Magic Nature of Neutrons in Ca54 : First Mass Measurements of 55-57Ca ATOMIC MASSES 55,56,57Ca, 48Ar, 44,46Cl, 40,42P, 40Si; measured charge, TOF, magnetic rigidity, and flight path length between the timing detectors; deduced m/q spectrum of reference masses, mass excesses. Comparison with AME2016 evaluation.
doi: 10.1103/PhysRevLett.121.022506
2017FU02 Phys.Rev. C 95, 025809 (2017) S.Furusawa, H.Nagakura, K.Sumiyoshi, C.Kato, S.Yamada Dependence of weak interaction rates on the nuclear composition during stellar core collapse
doi: 10.1103/PhysRevC.95.025809
2017FU05 J.Phys.(London) G44, 94001 (2017) S .Furusawa, H.Togashi, H.Nagakura, K.Sumiyoshi, S.Yamada, H.Suzuki, M.Takano A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
doi: 10.1088/1361-6471/aa7f35
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