Hartree-Fock-Bogoliubov Mass Models and the Equation of State of Neutron-Star Crusts

Details Hartree-Fock-Bogoliubov Mass Models and the Equation of State of Neutron-Star Crusts Hartree-Fock-Bogoliubov Mass Models and the Equation of State of Neutron-Star Crusts

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1128...29p&link_type=abstract

BULK NUCLEAR PROPERTIES: 5th ANL/MSU/JINA/INT FRIB Workshop. AIP Conference Proceedings, Volume 1128, pp. 29-39 (2009).

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3

Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Few-Body Systems, Mass And Neutron Distributions, Coulomb Energies, Nuclear Matter Aspects Of Neutron Stars

Scientific paper

We review the evolution of the Skyrme-Hartree-Fock-Bogoliubov mass
models of the Brussels-Montreal group, with particular emphasis on the
steps leading up to the most recent of these models, HFB-17. The
extension of these models to the calculation of the equation of state of
the inner crust of neutron stars is discussed.

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