The properties of isospin-asymmetric nuclear matter have been investigated
in the framework of the extended Brueckner-Hartree-Fock approximation at ze
ro temperature. Self-consistent calculations using the Argonne V-14 interac
tion are reported for several values of the asymmetry parameter beta = (N -
Z)/A, ranging from symmetric nuclear matter to pure neutron matter. The bi
nding energy per nucleon fulfills the beta(2) law in the whole asymmetry ra
nge. The symmetry energy is calculated for different densities and discusse
d in comparison with other predictions, At the saturation point it is in fa
irly good agreement with the empirical value. The present approximation, ba
sed on the Landau definition of quasiparticle energy, is investigated in te
rms of the Hugenholtz-Van Hove theorem, which is proved to be fulfilled wit
h a good accuracy at various asymmetries. The isospin dependence of the sin
gle-particle properties is discussed, including mean field, effective mass,
and mean free path of neutrons and protons. The isospin effects in nuclear
physics and nuclear astrophysics are briefly discussed. [S0556-2813(99)031
08-8].