Current status of Dirac-Brueckner-Hartree-Fock calculations in asymmetric nuclear matter
Abstract
Description
We review the current status of our microscopic calculations in asymmetric nuclear matter. Updated predictions of the equation of state are made available to potential users. We discuss the features of our EoS in relation to the predicted neutron star maximum masses.
8 pages, 4 figures
8 pages, 4 figures