We analytically and numerically study the relationship between an energy-de
pendent electron injection spectrum, F-0(E-0, t), and the resulting bremsst
rahlung photon spectrum, J(epsilon, t), With the goal of exploring whether
injection functions could explain energy-dependent time delays observed in
solar hare hard X-rays (HXRs) without any time-of-flight effects. We calcul
ate the inversion of the bremsstrahlung photon spectrum (for the Kramers cr
oss section) and find that the timing of the electron injection function de
pends on the time derivative of the second spectral derivative of the photo
n spectrum. To match the observed delays, a systematic softening of the ele
ctron injection spectrum is required over the duration (approximate to 1 s)
of individual HXR pulses. This requirement is exactly the same as that whi
ch occurs in the time-of-flight model, except there the softening is due to
spatial dispersion of injected electrons of different energy E-0. We show
that such a softening injection rate is not consistent with acceleration mo
dels where the electron acceleration times are comparable with the HXR puls
e lengths, but it can be consistent with models where the acceleration time
s are very short since the injection spectrum variations are then governed
by spectral variations in the acceleration rate. We conclude that accelerat
ion mechanisms cannot be ruled out on the basis of HXR light curves alone a
s an alternative to time-of-flight effects. Observations of HXR images and
of the relationship of HXRs to soft X-ray loops strongly suggest, however,
that time-of-flight effects must be important and must be included in attem
pts to infer primary accelerator properties from HXR light curves. We also
conclude that the agreement of the time-of-flight model with observed energ
y-dependent HXR delays, and the properties of any acceleration model contri
buting to this trend, puts strong constraints on the timescales involved in
the accelerator.