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NSR database version of April 27, 2024.

Search: Author = H.Mao

Found 12 matches.

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2018LI25      Phys.Rev. C 97, 054313 (2018)

Y.Li, J.Hu, H.Mao

Nucleon properties in the Polyakov quark-meson model

doi: 10.1103/PhysRevC.97.054313
Citations: PlumX Metrics

2016JI01      Phys.Rev. C 93, 015202 (2016)

J.Jin, H.Mao

Nontopological soliton in the Polyakov quark-meson model

doi: 10.1103/PhysRevC.93.015202
Citations: PlumX Metrics

2014MA57      Nucl.Phys. A925, 185 (2014)

H.Mao

On the symmetry improved CJT formalism in the O(4) linear sigma model

doi: 10.1016/j.nuclphysa.2014.02.011
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2013MA65      Phys.Rev. C 88, 035201 (2013)

H.Mao, T.Wei, J.Jin

Chiral soliton model at finite temperature and density

doi: 10.1103/PhysRevC.88.035201
Citations: PlumX Metrics

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 T_1/2. GXPF1A and KB3G effective interactions, N=126 waiting point.

doi: 10.1016/j.ppnp.2011.01.039
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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 ^{56,58,60,62,64}Ni(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
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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, ^{56,58,60,62,64}Ni; 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
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2008MA22      Phys.Rev. C 77, 065205 (2008)

H.Mao, M.Yao, W.-Qi.Zhao

Friedberg-Lee model at finite temperature and density

doi: 10.1103/PhysRevC.77.065205
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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
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2006MA77      Phys.Rev. C 74, 055204 (2006)

H.Mao, R.-K.Su, W.-Q.Zhao

Soliton solutions of an improved quark mass density-dependent model at finite temperature

doi: 10.1103/PhysRevC.74.055204
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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
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2004MA88      Chin.Phys.Lett. 21, 2155 (2004)

H.Mao, Y.-D.Li, T.Huang

Domain Wall in the Linear Sigma Model

doi: 10.1088/0256-307X/21/11/022
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