NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = H.Mao Found 12 matches. 2018LI25 Phys.Rev. C 97, 054313 (2018) Nucleon properties in the Polyakov quark-meson model
doi: 10.1103/PhysRevC.97.054313
2016JI01 Phys.Rev. C 93, 015202 (2016) Nontopological soliton in the Polyakov quark-meson model
doi: 10.1103/PhysRevC.93.015202
2014MA57 Nucl.Phys. A925, 185 (2014) On the symmetry improved CJT formalism in the O(4) linear sigma model
doi: 10.1016/j.nuclphysa.2014.02.011
2013MA65 Phys.Rev. C 88, 035201 (2013) Chiral soliton model at finite temperature and density
doi: 10.1103/PhysRevC.88.035201
2011SU04 Prog.Part.Nucl.Phys. 66, 385 (2011) T.Suzuki, M.Honma, T.Yoshida, H.Mao, T.Kajino, T.Otsuka Spin-dependent nuclear weak processes and nucleosynthesis in stars NUCLEAR REACTIONS 58Ni(E-, ν)58Co, 60Ni(E-, ν)60Co, 56Co(E-, ν)56Fe, 60Co(E-, ν)60Fe, E<100 keV; 56Ni(ν, p)55Co, 56Ni(ν, γ)56Ni, 56Ni(ν, α)52Fe, 56Ni(ν, n)55Ni, E< 10 MeV; calculated electron capture rates, σ, 55Mn yields. GXPF1A and KB3G effective interactions. RADIOACTIVITY 190Gd, 191Tb, 192Dy, 193Ho, 194Er, 195Tm, 196Yb, 197Lu, 198Hf, 199Ta(β-); calculated T1/2. GXPF1A and KB3G effective interactions, N=126 waiting point.
doi: 10.1016/j.ppnp.2011.01.039
2011SU09 Phys.Rev. C 83, 044619 (2011) T.Suzuki, M.Honma, H.Mao, T.Otsuka, T.Kajino Evaluation of electron capture reaction rates in Ni isotopes in stellar environments NUCLEAR REACTIONS 56,58,60,62,64Ni(e, ν), E at T9=1-10; evaluated Gamow-Teller B(GT) strengths, and electron capture rates at high densities and high temperatures during the core-collapse and postbounce explosive nucleosynthesis in supernovae using shell-model in the fp shell with GXPF1J interaction. Comparison with experimental data.
doi: 10.1103/PhysRevC.83.044619
2011SU27 J.Phys.:Conf.Ser. 312, 042023 (2011) T.Suzuki, T.Yoshida, M.Honma, H.Mao, T.Otsuka, T.Kajino Gamow-Teller and First-Forbidden Transition Strengths in Astrophysical Processes NUCLEAR STRUCTURE 54,56Fe, 56,58,60,62,64Ni; calculated β-decay B(GT) using shell model with GXPF1 and KB3G Hamiltonians. Compared with published data. NUCLEAR REACTIONS 56,58,60Ni(e-, ν), E≈100 keV-1 MeV; calculated capture rates. 58,60Ni(e-, ν), E≈1-10 MeV; calculated β-decay B(GT). Shell model with GXPF1 and KB3G Hamiltonians, compared with data.
doi: 10.1088/1742-6596/312/4/042023
2008MA22 Phys.Rev. C 77, 065205 (2008) Friedberg-Lee model at finite temperature and density
doi: 10.1103/PhysRevC.77.065205
2006MA65 J.Phys.(London) G32, 2187 (2006) H.Mao, N.Petropoulos, S.Shu, W.-Q.Zhao The linear sigma model at a finite isospin chemical potential
doi: 10.1088/0954-3899/32/11/012
2006MA77 Phys.Rev. C 74, 055204 (2006) Soliton solutions of an improved quark mass density-dependent model at finite temperature
doi: 10.1103/PhysRevC.74.055204
2005HU02 Phys.Rev. C 71, 014902 (2005) T.Huang, Y.Li, H.Mao, M.Nagasawa, X.Zhang Signal of the pion string at high-energy collisions NUCLEAR REACTIONS Pb(Pb, X), E(cm)=5.5 TeV; calculated pion spectra, pion string features.
doi: 10.1103/PhysRevC.71.014902
2004MA88 Chin.Phys.Lett. 21, 2155 (2004) Domain Wall in the Linear Sigma Model
doi: 10.1088/0256-307X/21/11/022
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