  In minimal Supergravity (mSUGRA) models the lightest supersymmetric particle
(assumed to be the lightest neutralino) provides an excellent cold dark matter
(CDM) candidate. The supersymmetric parameter space is significantly reduced,
if the limits on the CDM relic density, obtained from WMAP data, are used.
Assuming a vanishing trilinear scalar coupling A0 and fixed values of
tan(beta), these limits result in narrow lines of allowed regions in the
m0-m1/2 plane, the so called WMAP strips. In this analysis the trilinear
coupling A0 has been varied within +/-4 TeV. A fixed non vanishing A0 value
leads to a shift of the WMAP strips in the m0-m1/2 plane.
