The Brueckner-Hartree-Fock approximation extended to include ground-st
ate correlations is applied to neutron matter. Single-particle propert
ies are calculated including neutron mean field, effective mass and me
an free path. The main result is a pronounced enhancement of the effec
tive mass at the Fermi surface whose influence on neutron star propert
ies is discussed. (C) 1998 Elsevier Science B.V.