NSR Query Results
Output year order : Descending NSR database version of April 29, 2024. Search: Author = K.Nakazato Found 8 matches. 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
2023SU10 Nucl.Phys. A1038, 122719 (2023) T.Suzuki, K.Nakazato, M.Sakuda Neutrino-induced reactions on 18O and implications of 18O mixture in water Cherenkov detectors on supernova neutrino events NUCLEAR REACTIONS 16,18O(ν, e-), (ν-bar, e+), (ν, ν'), E<80MeV; calculated σ; deduced contributions from Gamow-Teller transitions. Comparison with available data.
doi: 10.1016/j.nuclphysa.2023.122719
2022SU14 Astrophys.J. 934, 15 (2022) Y.Suwa, A.Harada, M.Harada, Y.Koshio, M.Mori, F.Nakanishi, K.Nakazato, K.Sumiyoshi, R.A.Wendell Observing Supernova Neutrino Light Curves with Super-Kamiokande. III. Extraction of Mass and Radius of Neutron Stars from Synthetic Data
doi: 10.3847/1538-4357/ac795e
2018NA08 Phys.Rev. C 97, 035804 (2018) K.Nakazato, H.Suzuki, H.Togashi Heavy nuclei as thermal insulation for protoneutron stars
doi: 10.1103/PhysRevC.97.035804
2017TO07 Nucl.Phys. A961, 78 (2017) H.Togashi, K.Nakazato, Y.Takehara, S.Yamamuro, H.Suzuki, M.Takano Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces
doi: 10.1016/j.nuclphysa.2017.02.010
2011NA22 Phys.Rev. C 83, 065811 (2011) K.Nakazato, K.Iida, K.Oyamatsu Curvature effect on nuclear "pasta": Is it helpful for gyroid appearance?
doi: 10.1103/PhysRevC.83.065811
2010SU32 Nucl.Phys. A835, 295c (2010) K.Sumiyoshi, K.Nakazato, C.Ishizuka, A.Ohnishi, S.Yamada, H.Suzuki Emergence of hyperons in failed supernovae with short neutrino bursts
doi: 10.1016/j.nuclphysa.2010.01.205
2009NA19 Phys.Rev.Lett. 103, 132501 (2009) K.Nakazato, K.Oyamatsu, S.Yamada Gyroid Phase in Nuclear Pasta
doi: 10.1103/PhysRevLett.103.132501
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