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NSR database version of May 9, 2024.

Search: Author = S.S.Bao

Found 6 matches.

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2021BA06      Phys.Rev. C 103, 015804 (2021)

S.S.Bao, J.N.Hu, H.Shen

Impact of strong magnetic fields on the inner crust of neutron stars

doi: 10.1103/PhysRevC.103.015804
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2016BA09      Phys.Rev. C 93, 025807 (2016)

S.S.Bao, H.Shen

Effects of finite size and symmetry energy on the phase transition of stellar matter at subnuclear densities

doi: 10.1103/PhysRevC.93.025807
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2015BA04      Phys.Rev. C 91, 015807 (2015)

S.S.Bao, H.Shen

Impact of the symmetry energy on nuclear pasta phases and crust-core transition in neutron stars

doi: 10.1103/PhysRevC.91.015807
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2014BA12      Phys.Rev. C 89, 045807 (2014)

S.S.Bao, H.Shen

Influence of the symmetry energy on nuclear "pasta" in neutron star crusts

doi: 10.1103/PhysRevC.89.045807
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2014BA45      Phys.Rev. C 90, 045802 (2014)

S.S.Bao, J.N.Hu, Z.W.Zhang, H.Shen

Effects of the symmetry energy on properties of neutron star crusts near the neutron drip density

doi: 10.1103/PhysRevC.90.045802
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2014ZH36      Phys.Rev. C 90, 054302 (2014)

Z.W.Zhang, S.S.Bao, J.N.Hu, H.Shen

Symmetry energy of hot nuclei in the relativistic Thomas-Fermi approximation

NUCLEAR STRUCTURE ⁵⁶Fe, ²⁰⁸Pb; calculated proton and neutron density distributions and rms radii, neutron skin thickness. ⁵⁶Ti, ⁵⁶Cr, ⁵⁶Fe, ⁵⁶Ni, ²⁰⁸Pb, ²⁰⁸Po, ²⁰⁸Rn, ²⁰⁸Ra, ²⁰⁸Th; calculated symmetry energy coefficient a_sym as a function of Z. ⁵⁶Fe, ¹¹²Sn, ¹⁵⁰Sm, ²⁰⁸Pb; calculated temperature as a function of the excitation energy per particle, temperature dependence of a_sym. Relativistic Thomas-Fermi approximation using the relativistic mean-field model for four parameterization NL3, TM1, FSU and IUFSU.

doi: 10.1103/PhysRevC.90.054302
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