We consider the possibility of obtaining normal incident absorption in
the 10-15 mum range, using strained p-type SiGe quantum well structur
es using a full-scale relativistic pseudo-potential method. We predict
the magnitude and the position of the peak absorption response and de
termine the microscopic (band structure) origin of the peaks. We show
that major contributions to the absorption occur away from the centre
of the first Brillouin zone, and thus the energy of the peak response
cannot be accurately predicted by simple particle-in-a-box models. Als
o we discuss the possibilities of engineering the band structures of t
hese systems so as to minimize non-radiative (Auger) recombination. Co
mparisons of the parallel incidence absorption response calculated by
our method with recent experimental results are presented.