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NSR database version of April 29, 2024.

Search: Author = G.H.Wang

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2013NI16      Phys.Rev. C 88, 034308 (2013)

Y.F.Niu, Z.M.Niu, N.Paar, D.Vretenar, G.H.Wang, J.S.Bai, J.Meng

Pairing transitions in finite-temperature relativistic Hartree-Bogoliubov theory

NUCLEAR STRUCTURE ¹²⁴Sn; calculated binding energy/nucleon, entropy, neutron radius, charge radius, neutron pairing energy, neutron pairing gap, specific heat and contour plot for the neutron pairing gap as function of temperature. ^{36,38,40,42,44,46,48,50,52,54,56,58,60,62}Ca, ^{54,56,58,60,62,64,66,68,70,72,74,76,78,80,82,84,86,88,90,92}Ni, ^{102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140,142,144,146,148,150,152,154,156,158,160,162,164,166,168,170}Sn, ^{182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262,264}Pb; calculated neutron pairing gap as a function of temperature, neutron pairing gaps at zero temperature and critical temperatures for pairing transition. Finite temperature relativistic Hartree-Bogoliubov (FTRHB) theory based on point-coupling functional PC-PK1 with Gogny or separable pairing forces.

doi: 10.1103/PhysRevC.88.034308
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1990GR04      Nucl.Phys. A510, 346 (1990)

S.Graff, J.Gorres, M.Wiescher, R.E.Azuma, J.King, J.Vise, G.Hardie T.R.Wang

Proton Capture on ²⁸Si and Its Astrophysical Implications

NUCLEAR REACTIONS, ICPND ²⁸Si(p, γ), E=0.37-2.95 MeV; measured σ(E); deduced astrophysical S-factor, total reaction rate. ²⁹P deduced resonances, resonance strengths, Γ, spectroscopic factors.

doi: 10.1016/0375-9474(90)90244-G
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2709.