We review the propagation of energetic partons in hot or cold QCD matter, a
s known from recent work. We summarize advances in the understanding of bat
h collisional and radiative energy loss. Our emphasis is on radiative energ
y loss, which has very interesting properties that may help to detect the q
uark-gluon plasma produced in heavy-ion collisions. We describe two differe
nt theoretical approaches, which lead to the same radiated gluon energy spe
ctrum. The case of a longitudinally expanding QCD plasma is investigated. T
he energy lost by a jet with given opening angle is calculated with the aim
of making predictions for the suppression (quenching) of hard jet producti
on. Phenomenological implications for the difference between hot and cold m
atter are discussed. Numerical estimates of the loss suggest that it may be
significantly greater in hot matter than in cold. This makes the magnitude
of the radiative energy loss a remarkable signal for quark-gluon plasma fo
rmation.