Author:
Depta Paul Frederik,Hufnagel Marco,Schmidt-Hoberg Kai
Abstract
Abstract
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,
can easily be extended also to other
scenarios.
For the most recent version of this manual, please visit the GitHub repository at
https://github.com/skumblex/acropolis.
Subject
Astronomy and Astrophysics
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