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Session 73 - White Dwarfs, Neutron Stars and Pulsars.
Display session, Thursday, June 13
With the relativistic extended Thomas-Fermi method, we study the dense matter in the inner crust of neutron stars based on the Zimanyi amp; Moszkowski (1990, ZM) model in the relativistic mean field theory. We also compare these results with those based on the Boguta amp; Bodmer (1977, BB) model with a resent satisfactory parameter set.
Program listing for Thursday