Space-time picture of deep inelastic lepton-nucleus interactions with cumulative nucleon production

Results are presented of calculations of interactions of neutrinos with energies from 10 to 200 GeV with emulsion nuclei. The calculations have been made within the model which takes account of the space-time characteristics of intranuclera interactions, absorption of particles in a nucleus and evaporation of particles from a residual nucleus. Special attention is paid to the cumulative protons. The theory is compared with the experiment recently performed by the collaboartion of the JINR, IHEP, ITEP, FNAL et al. Some predictive computations are presented. 7 refs.; 3 figs.; 1 tab