NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = T.Muto Found 14 matches. 2010MU15 Nucl.Phys. A835, 370c (2010) Effects of the Λ(1405) on the Structure of Multi-Antikaonic Nuclei NUCLEAR STRUCTURE 15O; calculated K- hypernucleus density distribution, binding energy.
doi: 10.1016/j.nuclphysa.2010.01.221
2009MU03 Phys.Rev. C 79, 035207 (2009) Multi-antikaonic nuclei in relativistic mean-field theory NUCLEAR STRUCTURE 15O; calculated density distribution of protons and neutrons, distribution of strangeness density, chiral angle at center of multi-antikaonic nuclei, baryon number density, Coulomb energy, sign-reversed binding energy per strangeness, effective mass of K-, lowest K- energy. Relativistic mean-field theory, chiral symmetry.
doi: 10.1103/PhysRevC.79.035207
2008MU02 Phys.Rev. C 77, 015810 (2008) Interplay between kaon condensation and hyperons in highly dense matter
doi: 10.1103/PhysRevC.77.015810
2008MU10 Nucl.Phys. A804, 322 (2008) Kaon-condensed hypernuclei as highly dense self-bound objects
doi: 10.1016/j.nuclphysa.2008.02.302
2005MA78 Nucl.Phys. A760, 319 (2005) T.Maruyama, T.Muto, T.Tatsumi, K.Tsushima, A.W.Thomas Kaon condensation and lambda-nucleon loop in the relativistic mean-field approach
doi: 10.1016/j.nuclphysa.2005.06.008
2005MU17 Nucl.Phys. A754, 350c (2005) Kaon condensation in hyperonic matter and properties of neutron stars
doi: 10.1016/j.nuclphysa.2005.02.080
2004MU34 Prog.Theor.Phys.(Kyoto), Suppl. 156, 182 (2004) Kaon Condensation in Hyperonic Matter and Structure of Neutron Stars
doi: 10.1143/PTPS.156.182
2002MU01 Nucl.Phys. A697, 225 (2002) Kaonic Modes in Hyperonic Matter and p-Wave Kaon Condensation
doi: 10.1016/S0375-9474(01)01226-X
2001MU29 Nucl.Phys. A691, 447c (2001) Kaon Dispersion Relations in Hyperonic Matter and Kaon Condensation
doi: 10.1016/S0375-9474(01)01072-7
1999DO36 Nucl.Instrum.Methods Phys.Res. A437, 169 (1999) K.Dobashi, T.Hirose, T.Kumita, Y.Kurihara, T.Muto, T.Omori, T.Okugi, K.Sugiyama, J.Urakawa Generation of Positrons via Pair-Creation from Compton Scattered Gamma-Rays NUCLEAR REACTIONS W(polarized γ, e-e+), E=high; measured positron spectra, polarization features. Comparison with model predictions.
doi: 10.1016/S0168-9002(99)00677-4
1996FU01 Nucl.Phys. A597, 645 (1996) H.Fujii, T.Maruyama, T.Muto, T.Tatsumi Equation of State with Kaon Condensates and Neutron Stars
doi: 10.1016/0375-9474(95)00451-3
1994FU02 Nucl.Phys. A571, 758 (1994) H.Fujii, T.Muto, T.Tatsumi, R.Tamagaki Effects of Weak Interaction on Kaon Condensation and Cooling of Neutron Stars
doi: 10.1016/0375-9474(94)90719-6
1994FU10 Phys.Rev. C50, 3140 (1994) H.Fujii, T.Muto, T.Tatsumi, R.Tamagaki Effects of Symmetry Energy on the Direct URCA Process in the Kaon Condensed Phase
doi: 10.1103/PhysRevC.50.3140
1994MA49 Phys.Lett. 337B, 19 (1994) T.Maruyama, H.Fujii, T.Muto, T.Tatsumi Kaon Condensation and Equation of State in the Relativistic Mean-Field Theory
doi: 10.1016/0370-2693(94)91436-2
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