The Li-abundances recently observed in the low mass secondaries of sev
eral soft X-ray transients have been proposed to come from nuclear rea
ctions in the vicinity of the compact objects during the outbursts of
these systems. This scenario implies a large flux of energetic particl
es in X-ray transients. We show that Li newly produced in an outburst
is mixed into the secondary very quickly, so that the observed abundan
ce must represent the average production over many outbursts. With kno
wn Limits on the Li-depletion rates in low mass stars, we derive minim
al energy fluxes in energetic protons and/or alpha-particles, assuming
that either the secondary or the accretion disk is the main target of
this flux. In both cases, at least a few per cent of the accretion en
ergy must be converted to fast particles with energies exceeding 10 Me
V/nucleon.