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Muto, Takumi*; Maruyama, Toshiki; Tatsumi, Toshitaka*
Symmetry (Internet), 17(2), p.270_1 - 270_24, 2025/02
Times Cited Count：0 Percentile：0.00(Multidisciplinary Sciences)Xia, C.-J.*; Maruyama, Toshiki; Yasutake, Nobutoshi*; Tatsumi, Toshitaka*
Physical Review D, 110(11), p.114024_1 - 114024_14, 2024/12
Times Cited Count：1 Percentile：35.96(Astronomy & Astrophysics)Yasutake, Nobutoshi*; Maruyama, Toshiki
Physical Review D, 109(4), p.043056_1 - 043056_11, 2024/02
Times Cited Count：2 Percentile：55.99(Astronomy & Astrophysics)Xia, C.-J.*; Maruyama, Toshiki; Yasutake, Nobutoshi*; Tatsumi, Toshitaka*; Zhang, Y.-X.*
Physics Letters B, 839, p.137769_1 - 137769_5, 2023/04
Times Cited Count：2 Percentile：43.87(Astronomy & Astrophysics)Xia, C.-J.*; Maruyama, Toshiki; Yasutake, Nobutoshi*; Tatsumi, Toshitaka*
Physical Review D, 106(6), p.063020_1 - 063020_14, 2022/09
Times Cited Count：6 Percentile：43.45(Astronomy & Astrophysics)Muto, Takumi*; Maruyama, Toshiki; Tatsumi, Toshitaka*
Progress of Theoretical and Experimental Physics (Internet), 2022(9), p.093D03_1 - 093D03_37, 2022/09
Times Cited Count：2 Percentile：27.99(Physics, Multidisciplinary)Ohshima, Hiroyuki; Morishita, Masaki*; Aizawa, Kosuke; Ando, Masanori; Ashida, Takashi; Chikazawa, Yoshitaka; Doda, Norihiro; Enuma, Yasuhiro; Ezure, Toshiki; Fukano, Yoshitaka; et al.
Sodium-cooled Fast Reactors; JSME Series in Thermal and Nuclear Power Generation, Vol.3, 631 Pages, 2022/07
This book is a collection of the past experience of design, construction, and operation of two reactors, the latest knowledge and technology for SFR designs, and the future prospects of SFR development in Japan. It is intended to provide the perspective and the relevant knowledge to enable readers to become more familiar with SFR technology.
Miao, Z.-Q.*; Xia, C.-J.*; Lai, X.-Y.*; Maruyama, Toshiki; Xu, R.-X.*; Zhou, E.-P.*
International Journal of Modern Physics E, 31(4), p.2250037_1 - 2250037_20, 2022/04
Times Cited Count：11 Percentile：84.55(Physics, Nuclear)Xia, C.-J.*; Sun, B. Y.*; Maruyama, Toshiki; Lon, W.-H.*; Li, A.*
Physical Review C, 105(4), p.045803_1 - 045803_14, 2022/04
Times Cited Count：16 Percentile：91.60(Physics, Nuclear)Muto, Takumi*; Maruyama, Toshiki; Tatsumi, Toshitaka*
Physics Letters B, 820, p.136587_1 - 136587_6, 2021/09
Times Cited Count：11 Percentile：76.75(Astronomy & Astrophysics)no abstracts in English
Xia, C.-J.*; Maruyama, Toshiki; Yasutake, Nobutoshi*; Tatsumi, Toshitaka*; Zhang, Y.-X.*
Physical Review C, 103(5), p.055812_1 - 055812_13, 2021/05
Times Cited Count：16 Percentile：86.03(Physics, Nuclear)Xia, C.-J.*; Maruyama, Toshiki; Yasutake, Nobutoshi*; Tatsumi, Toshitaka*; Shen, H.*; Togashi, Hajime*
Physical Review D, 102(2), p.023031_1 - 023031_18, 2020/07
Times Cited Count：29 Percentile：81.87(Astronomy & Astrophysics)no abstracts in English
Muto, Takumi*; Maruyama, Toshiki; Tatsumi, Toshitaka*; Takatsuka, Tatsuyuki*
JPS Conference Proceedings (Internet), 26, p.024019_1 - 024019_4, 2019/11
Maslov, K.*; Yasutake, Nobutoshi*; Blaschke, D.*; Ayriyan, A.*; Grigorian, H.*; Maruyama, Toshiki; Tatsumi, Toshitaka*; Voskresensky, D. N.*
Physical Review C, 100(2), p.025802_1 - 025802_11, 2019/08
Times Cited Count：56 Percentile：97.23(Physics, Nuclear)The effect of pasta phases on the quark-hadron phase transition is investigated for a set of relativistic mean-field equations of state for both hadron and quark matter. The results of the full numerical solution with pasta phases are compared with those of an interpolating construction used in previous works, for which we demonstrate an adequate description of the numerical results. For each pair of quark and hadron matter models the critical value of the surface tension is determined, above which the phase transition becomes close to the Maxwell construction. This result agrees well with earlier theoretical estimates. The study is extended to neutron star matter in beta equilibrium with electrons and muons and is applied to investigate the effect of pasta phases on the structure of hybrid compact stars and the robustness of a possible third family solution.
Lee, T.-G.*; Yasutake, Nobutoshi*; Maruyama, Toshiki; Tatsumi, Toshitaka*
Proceedings of Science (Internet), 281, p.326_1 - 326_8, 2017/05
Muto, Takumi*; Maruyama, Toshiki; Tatsumi, Toshitaka*
JPS Conference Proceedings (Internet), 14, p.020809_1 - 020809_3, 2017/02
Times Cited Count：0 Percentile：0.00(Astronomy & Astrophysics)Noda, Tsuneo*; Hashimoto, Masaaki*; Matsuo, Yasuhide*; Yasutake, Nobutoshi*; Maruyama, Toshiki; Tatsumi, Toshitaka*
JPS Conference Proceedings (Internet), 14, p.020805_1 - 020805_3, 2017/02
Times Cited Count：0 Percentile：0.00(Astronomy & Astrophysics)Lee, T.-G.*; Nishiyama, Kazuya*; Yasutake, Nobutoshi*; Maruyama, Toshiki; Tatsumi, Toshitaka*
JPS Conference Proceedings (Internet), 14, p.020808_1 - 020808_3, 2017/02
Times Cited Count：0 Percentile：0.00(Astronomy & Astrophysics)Yasutake, Nobutoshi*; Chen, H.*; Maruyama, Toshiki; Tatsumi, Toshitaka*
Journal of Physics; Conference Series, 665(1), p.012068_1 - 012068_4, 2016/01
Times Cited Count：7 Percentile：89.47(Astronomy & Astrophysics)Yasutake, Nobutoshi*; Benic, S.*; Blaschke, D.*; Maruyama, Toshiki; Tatsumi, Toshitaka*
Acta Astronomica Sinica, 56(Suppl.), p.85 - 87, 2015/11
We study quark-hadron phase transition in neutron stars. The finite-size effects of mixed-phase structure should be taken into account in the phase transition of multi-component system. The phase transition strongly depends on the models for quark and hadron matter, surface tension, neutrino fraction, and temperature. We find that with strong surface tension the equation of state (EOS) becomes similar to that of a Maxwell construction, while weak surface tension yields bulk Gibbs condition. We also find that the mass-radius relation obtained by our EOS is consistent to the observation.
