Abstract
Abstract
We explore the impact of non-perturbative effects, namely Sommerfeld enhancement and bound
state formation, on the cosmological production of non-thermal dark matter. For this purpose, we
focus on a class of simplified models with t-channel mediators. These naturally combine the
requirements for large corrections in the early Universe, i.e. beyond the Standard Model states
with long range interactions, with a sizable new physics production cross section at the LHC. We
find that the dark matter yield of the superWIMP mechanism is suppressed considerably due to the
non-perturbative effects under consideration in models with color-charged mediators. In models
with only electrically charged mediators the impact of non-perturbative effects is less pronounced
and gets eclipsed by the impact of a possible Higgs portal interaction. In both cases we find
significant shifts in the cosmologically preferred parameter space of non-thermal dark matter in
these models. We also revisit the implications of LHC bounds on long-lived particles associated
with non-thermal dark matter and find that testing this scenario at the LHC is a bigger challenge
than previously anticipated.
Subject
Astronomy and Astrophysics
Cited by
2 articles.
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