Dataset referencing 2010LO03

Phys.Rev. C 81, 031302 (2010)

W.-H.Long, P.Ring, J.Meng, N.Van Giai, C.A.Bertulani

Nuclear halo structure and pseudospin symmetry

NUCLEAR STRUCTURE 40,42,44,46,48,50,52,54,56,58,60,62,64,66,68,70,72,74Ca, 56,58,60,62,64,66,68,70,72,74,76,78,80,82,84,86,88,90,92,94Ni, 80,82,84,86,88,90,92,94,96,98,100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140Zr, 102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140,142,144,146,148,150,152,154,156,158,160,162,164,166,168,170,172,174Sn, 122,124,126,128,130,132,134,136,138,140,142,144,146,148,150,152,154,156,158,160,162,164,166,168,170,172,174,176,178,180,182,184,186,188,190,192,194,196,198Ce; calculated neutron skin thickness (rn-rp) using RHFB with PKA1 plus the D1S pairing force. 140,142,144,146,148,150,152,154,156,158,160,162,164,166,168,170,172,174,176,178,180,182,184,186,188,190,192,194,196,198Ce; calculated neutron and proton densities, neutron single particle energies, Two-body interaction matrix elements Vab, neutron shell gap, halo structure near neutron drip line, and conservation of pseudospin symmetry using relativistic Hartree-Fock-Bogoliubov calculations.

doi: 10.1103/PhysRevC.81.031302

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