where F is the fraction of the projectile in the interaction zone,
is the nuclear mean-free-path, assumed to be:
![]() |
(26.8) |
where:
In the event that
then
is:
![]() |
(26.10) |
where:
The projectile and target nuclear radii are given by the expression:
where the functions
and
are given in section
26.7. Wilson et al equate this surface area to the
excitation to:
if the collision is peripheral and there is no significant distortion of the nucleus, or
For the abraded region, Wilson et al assume that fragments with a nucleon number of five are unbounded, 90% of fragments with a nucleon number of eight are unbound, and 50% of fragments with a nucleon number of nine are unbound. This was not implemented within the Geant4 version of the abrasion model, and disintegration of the pre-fragment was only simulated by the subsequent de-excitation physics models in the G4DeexcitationHandler (evaporation, etc. or G4WilsonAblationModel) since the yields of lighter fragments were already underestimated compared with experiment.
In addition to energy as a result of the distortion of the fragment,
some energy is assumed to be gained from transfer of kinetic energy across the
boundaries of the nuclei. This is approximated to the average energy
transferred to a nucleon per unit intersection pathlength (assumed to be 13
MeV/fm) and the longest chord-length,
, and for half of the
nucleon-nucleon collisions it is assumed that the excitation energy is:
where:
![]() |
(26.17) |
For the remaining events, the projectile energy is assumed to be unchanged. Wilson et al assume that the energy required to remove a nucleon is 10MeV, therefore the number of nucleons removed from the projectile by ablation is:
where
is the number of loosely-bound spectators
in the interaction region, given by:
The abrasion process is assumed to occur without preference for the nucleon type, i.e. the probability of a proton being abraded from the projectile is proportional to the fraction of protons in the original projectile, therefore:
In order to calculate the charge distribution of the final fragment, Wilson et al assume that the products of the interaction lie near to nuclear stability and therefore can be sampled according to the Rudstam equation (see section 26.6). The other obvious condition is that the total charge must remain unchanged.