Can Dark Matter be an artifact of extended theories of gravity?
Sayantan Choudhury, Manibrata Sen, Soumya Sadhukhan

TL;DR
This paper explores extended theories of gravity as a framework to explain dark matter genesis without altering the Standard Model, constraining model parameters through relic abundance and self-interaction observations.
Contribution
It introduces background models of extended gravity theories minimally coupled to the SM, linking them to dark matter production and self-interactions, with constraints from observational data.
Findings
Constraints on dark matter mass and interaction cross sections from Planck data.
Effective theories from extended gravity match SM sector, allowing for dark matter genesis.
Derived bounds on gravity model parameters from dark matter self-interactions.
Abstract
In this article, we propose different background models of extended theories of gravity, which are minimally coupled to the SM fields, to explain the possibility of genesis of dark matter without affecting the SM particle sector. We modify the gravity sector by allowing quantum corrections motivated from (1) local gravity and (2) non-minimally coupled gravity with SM sector and dilaton field. Next we apply conformal transformation on the metric to transform the action back to the Einstein frame. We also show that an effective theory constructed from these extended theories of gravity and SM sector looks exactly the same. Using the relic constraint observed by Planck 2015, we constrain the scale of the effective field theory () as well as the dark matter mass (). We consider two cases- (1) light dark matter (LDM) and (2) heavy dark matter (HDM), and deduce upper…
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