We study the symmetry energy in infinite nuclear matter employing a no
n-relativistic Brueckner-Hartree-Fock approach and using various new n
ucleon-nucleon (NN) potentials, which fit np and pp scattering data ve
ry accurately. The potential models we employ are the recent versions
of the Nijmegen group, Nijm-I, Nijm-II, and Reid93, the Argonne V-18 p
otential and the CD-Bonn potential. All these potentials yield a symme
try energy which increases with density, resolving a discrepancy that
existed for older NN potentials. The origin of remaining differences i
s discussed. (C) 1997 Elsevier Science B.V.