NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = T.Takatsuka Found 23 matches. 2016MA23 Eur.Phys.J. A 52, 65 (2016) K.Masuda, T.Hatsuda, T.Takatsuka Hyperon puzzle, hadron-quark crossover and massive neutron stars
doi: 10.1140/epja/i2016-16065-6
2016MA63 Nucl.Phys. A956, 817 (2016) K.Masuda, T.Hatsuda, T.Takatsuka Hot Neutron Stars with Hadron-Quark Crossover
doi: 10.1016/j.nuclphysa.2016.03.054
2013SO02 Nucl.Instrum.Methods Phys.Res. B295, 1 (2013) T.Sonoda, M.Wada, H.Tomita, C.Sakamoto, T.Takatsuka, T.Furukawa, H.Iimura, Y.Ito, T.Kubo, Y.Matsuo, H.Mita, S.Naimi, S.Nakamura, T.Noto, P.Schury, T.Shinozuka, T.Wakui, H.Miyatake, S.Jeong, H.Ishiyama, Y.X.Watanabe, Y.Hirayama, K.Okada, A.Takamine Development of a resonant laser ionization gas cell for high-energy, short-lived nuclei ATOMIC PHYSICS Fe, Co, Nb, Cu; measured laser wavelength for resonance ionization, transport efficiency. Comparison with calculations.
doi: 10.1016/j.nimb.2012.10.009
2006TA06 Prog.Theor.Phys.(Kyoto) 115, 355 (2006) T.Takatsuka, S.Nishizaki, Y.Yamamoto, R.Tamagaki Occurrence of Hyperon Superfluidity in Neutron Star Cores
doi: 10.1143/PTP.115.355
2006TA23 Prog.Theor.Phys.(Kyoto) 116, 573 (2006) Baryonic 3P2-Dominant Superfluidity under Combined Pion Condensation with Δ Isobar. I
doi: 10.1143/PTP.116.573
2004NI19 Prog.Theor.Phys.(Kyoto), Suppl. 156, 154 (2004) S.Nishizaki, Y.Yamamoto, T.Takatsuka Hyperon Mixing and EOS of Neutron Star Cores
doi: 10.1143/PTPS.156.154
2004TA22 Nucl.Phys. A738, 387 (2004) Baryon superfluidity and neutrino emissivity of neutron stars
doi: 10.1016/j.nuclphysa.2004.04.067
2004TA23 Prog.Theor.Phys.(Kyoto) 112, 37 (2004) Baryon Superfluidity and Neutrino Emissivity of Neutron Stars
doi: 10.1143/PTP.112.37
2004TA42 Prog.Theor.Phys.(Kyoto), Suppl. 156, 84 (2004) Hyperon-Mixed Neutron Stars
doi: 10.1143/PTPS.156.84
2003TA34 Nucl.Phys. A721, 1003c (2003) Temperature Effects on Hyperon Superfluids in Neutron Stars
doi: 10.1016/S0375-9474(03)01272-7
2002NI09 Prog.Theor.Phys.(Kyoto) 108, 703 (2002) S.Nishizaki, Y.Yamamoto, T.Takatsuka Hyperon-Mixed Neutron Star Matter and Neutron Stars
doi: 10.1143/PTP.108.703
2002TA06 Eur.Phys.J. A 13, 213 (2002) T.Takatsuka, S.Nishizaki, Y.Yamamoto Necessity of Extra Repulsion in Hypernuclear Systems: Suggestion from neutron stars
doi: 10.1007/s10050-002-8744-y
2002TA29 Prog.Theor.Phys.(Kyoto), Suppl. 146, 279 (2002) T.Takatsuka, S.Nishizaki, Y.Yamamoto, R.Tamagaki Superfluidity of Hyperon-Mixed Neutron Stars
doi: 10.1143/PTPS.146.279
2001NI10 Prog.Theor.Phys.(Kyoto) 105, 607 (2001) S.Nishizaki, Y.Yamamoto, T.Takatsuka Effective YN and YY Interactions and Hyperon-Mixing in Neutron Star Matter - Y = Λ Case -
doi: 10.1143/PTP.105.607
2001TA18 Prog.Theor.Phys.(Kyoto) 105, 1059 (2001) Dependence on Spin and Isospin of Short-Range Nuclear Force in Modified OPEG
doi: 10.1143/PTP.105.1059
2001TA28 Nucl.Phys. A691, 254 (2001) T.Takatsuka, S.Nishizaki, Y.Yamamoto, R.Tamagaki Energy Gap of Hyperon Pairing in Hypernuclear Systems
doi: 10.1016/S0375-9474(01)01040-5
2001YA17 Nucl.Phys. A691, 432c (2001) Y.Yamamoto, S.Nishizaki, T.Takatsuka Hyperons in Neutron Stars
doi: 10.1016/S0375-9474(01)01069-7
2000TA14 Nucl.Phys. A670, 222c (2000) Λ-Hyperon Superfluidity in Neutron Star Cores
doi: 10.1016/S0375-9474(00)00104-4
2000YA16 Prog.Theor.Phys.(Kyoto) 103, 981 (2000) Y.Yamamoto, S.Nishizaki, T.Takatsuka Single-Particle Potentials and Effective Masses of Hyperons in Hyperonic Nuclear Systems
doi: 10.1143/PTP.103.981
1999TA34 Prog.Theor.Phys.(Kyoto) 102, 1043 (1999) Superfluidity of Λ-Hyperons Admixed in Neutron Star Cores
doi: 10.1143/PTP.102.1043
1995TA19 Nucl.Phys. A588, 365c (1995) Hot Versus Cold Neutron Stars
doi: 10.1016/0375-9474(95)00162-T
1994NI13 Prog.Theor.Phys.(Kyoto) 92, 93 (1994) S.Nishizaki, T.Takatsuka, J.Hiura Properties of Hot Asymmetric Nuclear Matter
doi: 10.1143/ptp/92.1.93
1991NI05 Prog.Theor.Phys.(Kyoto) 86, 853 (1991) S.Nishizaki, T.Takatsuka, N.Yahagi, J.Hiura Effective Two-Nucleon Interaction in Asymmetric Nuclear Matter NUCLEAR REACTIONS 1n(n, n), (p, p), E ≈ astrophysical; calculated effective interaction parameters. Asymmetric nuclear matter.
doi: 10.1143/ptp/86.4.853
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