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NSR database version of May 19, 2024.

Search: Author = Z.W.Zhang

Found 9 matches.

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2022ZH31      Phys.Rev. C 105, 055807 (2022)

Z.-W.Zhang, C.J.Pethick

Superfluid density in disordered pasta phases in neutron star crusts

doi: 10.1103/PhysRevC.105.055807
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2021ZH28      Phys.Rev. C 103, 055807 (2021)

Z.-W.Zhang, C.J.Pethick

Proton superconductivity in pasta phases in neutron star crusts

doi: 10.1103/PhysRevC.103.055807
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2020PE05      Phys.Rev. C 101, 055802 (2020)

C.J.Pethick, Z.-W.Zhang, D.N.Kobyakov

Elastic properties of phases with nonspherical nuclei in dense matter

doi: 10.1103/PhysRevC.101.055802
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2019ZH51      Phys.Rev. C 100, 054304 (2019)

Z.-W.Zhang, L.-W.Chen

Cold dilute nuclear matter with α-particle condensation in a generalized nonlinear relativistic mean-field model

doi: 10.1103/PhysRevC.100.054304
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2017LA10      Eur.Phys.J. A 53, 131 (2017)

C.-l.Lan, Y.-j.Qiu, Q.Wang, Z.-w.Zhang, Q.Zhang, J.-c.Tan, C.-f.Lai, K.-h.Fang

Measurement of fission cross section for 232Th (n, f) 131ZX ( Z = 50 , 51, 52, 53) reaction induced by neutrons around 14 MeV

NUCLEAR REACTIONS 232Th(n, f), E≈14 MeV; measured activation Eγ, Iγ; deduced γ-ray spectra. 131Sb, 131mTe, 131gTe, 131I; deduced activation σ.

doi: 10.1140/epja/i2017-12318-2
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset32765.

2017ZH26      Phys.Rev. C 95, 064330 (2017)

Z.-W.Zhang, L.-W.Chen

Low density nuclear matter with light clusters in a generalized nonlinear relativistic mean-field model

doi: 10.1103/PhysRevC.95.064330
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2016LA26      Eur.Phys.J. A 52, 345 (2016)

C.-L.Lan, S.-T.Liu, T.Lv, Q.Wang, C.-F.Lai, Z.-W.Zhang, K.-H.Fang

Measurement of fission cross-section for the 232Th(n, f )141Ba reaction induced by neutrons around 14 MeV

NUCLEAR REACTIONS 232Th(n, F)141Ba, E=14.1, 14.5, 14.7 MeV; measured off-line discrete Eγ, Iγ; deduced main levels, J, π, 141Ba production σ using activation method.

doi: 10.1140/epja/i2016-16345-1
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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 asym as a function of Z. 56Fe, 112Sn, 150Sm, 208Pb; calculated temperature as a function of the excitation energy per particle, temperature dependence of asym. 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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