Skyrme—Hartree—Fock

Recently in applying the non-relativistic Skyrme Hartree-Fock (SHF) model Brown [19] noted that certain combinations of parameters in the SHF are not well determined by a fit to ground state binding energies alone as a result a wide range of predictions for the EoS for PNM can be obtained. At the same time he found a correlation between the derivative of the neutron star EoS (i.e., basically the symmetry pressure po) and the neutron skin in 208Pb. 

A study of the superheavy region with self-consistent mean field models (employing mean field and Skyrme-Hartree-Fock approaches) yields different results for predicted regions of stability. O Figure 19.16 displays the single-particle spectra for neutrons and protons (Bender et al. 2001) for Sn, the superheavy nucleus 126, and the hyperheavy nucleus 164. They exhibit a significant difference in the nature of the shells of doubly magic tin (where proton and... 

Typel, S., Brown, B.A. Skyrme Hartree-Fock calculations for the a-decay Q values of superheavy nuclei. Phys. Rev. C67, 034313(6) (2003)... 

The static Hartree-Fock problem assumes T-reversal invariance and T-even single-particle density matrix. In this case, Skyrme forces can be limited by only T-even densities psif) Tsif) In the case of dy-... 

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