  Super Rosenbluth experiments, elastic electron-proton scattering experiments
that eschew traditional electron detection and opt instead for the detection of
the recoiling proton, have several experimental advantages. One claimed
advantage is that radiative corrections are more favorable, i.e., smaller and
with less kinematic dependence. In this paper, we explore this claim by
conducting Monte Carlo simulations of both Super Rosenbluth and traditional
Rosenbluth experiments with different models of radiative effects. When using a
model that employs the peaking approximation, we indeed confirm that reduced
kinematic dependence of the radiative corrections. However, we find that more
sophisticated models that avoid the peaking approximation are unable to produce
numerically stable results, due to a large enhancement to the cross section for
bremsstrahlung radiation from the proton when the invariant squared momentum
transfer $Q^2$ approaches zero. Since this enhancement is not modelled in the
peaking approximation, a more robust approach to radiative corrections in Super
Rosenbluth experiments is needed.
