We introduce the notion of defocusing gravitational lens considering a
MACHO located behind a light source with respect to an observer. The
consequence of defocusing effect is a temporal variability of star lum
inosity which produces a gap instead of a peak as tell-tale signature
in the light curve. A general theory of (de)focusing rays (geodesics)
in a gravitational field is presented. Furthermore, we give estimation
s of the mass of the lens and the optical depth connected to such phen
omenon.