  The remarkable agreement between observations of the primordial light element
abundances and the corresponding theoretical predictions within the standard
cosmological history provides a powerful method to constrain physics beyond the
standard model of particle physics (BSM). For a given BSM model these
primordial element abundances are generally determined by (i) Big Bang
Nucleosynthesis and (ii) possible subsequent disintegration processes. The
latter potentially change the abundances due to late-time high-energy
injections which may be present in these scenarios. While there are a number of
public codes for the first part, no such code is currently available for the
second. Here we close this gap and present ACROPOLIS, A generiC fRamework fOr
Photodisintegration Of LIght elementS. The widely discussed cases of decays as
well as annihilations can be run without prior coding knowledge within example
programs. Furthermore, due to its modular structure, ACROPOLIS can easily be
extended also to other scenarios.
