The absorption of nucleons passing through any number of nuclei is calculated with due consideration of all fluctuations of energy loss. For the probability ω (
, E) d
for an energy loss
by a nucleon with energy E hitting a nucleon at rest, a law of the form ω d
= ω(
/E) d
/E is assumed, a law suggested by meson theory and Bremsstrahlung. It is shown that, with a primary spectrum, following a power law, the absorption is strictly exponential for any thickness of the absorber and for all energies of the nucleons, apart from small deviations at low energies due to the latitude cut-off. This agrees well with recent experimental results. The experiments also permit some conclusions about the shape of the function ω, and it is shown that ω must be a fairly broad distribution extending up to
/E = 1, possibly favouring, but not to a very large extent, low values of
/E. The average energy loss of a fast nucleon hitting a nucleon at rest is determined by the experiments within very narrow limits. The conclusions that can be drawn about ω, the total cross-section for meson production and the average energy loss are all compatible with the theory of Hamilton, Heitler and Peng, in its later version