NSR Query Results
Output year order : Descending NSR database version of May 2, 2024. Search: Author = H.Togashi Found 7 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
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
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
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
2017YA29 Phys.Rev. C 96, 065804 (2017) Y.Yamamoto, H.Togashi, T.Tamagawa, T.Furumoto, N.Yasutake, Th.A.Rijken Neutron-star radii based on realistic nuclear interactions
doi: 10.1103/PhysRevC.96.065804
2016TO06 Phys.Rev. C 93, 035808 (2016) H.Togashi, E.Hiyama, Y.Yamamoto, M.Takano Equation of state for neutron stars with hyperons using a variational method
doi: 10.1103/PhysRevC.93.035808
2013TO04 Nucl.Phys. A902, 53 (2013) Variational study for the equation of state of asymmetric nuclear matter at finite temperatures
doi: 10.1016/j.nuclphysa.2013.02.014
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