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We present an updated version of the SimProp Monte Carlo code: a simulationscheme to study the propagation of ultra-high-energy cosmic rays throughdiffuse extragalactic background radiation. The new version of the codepresents two important updates: (i) it treats in a full stochastic approach allinteraction channels involving ultra-high-energy cosmic rays and (ii) it takesinto account the production of secondary (cosmogenic) neutrinos. This newversion of SimProp was tested against different simulations code, in particularthe production of secondary neutrinos was compared with the fluxes expected inthe scenario of Engel, Seckel and Stanev.

SimProp v2r2: a Monte Carlo simulation to compute cosmogenic neutrino fluxes