Can decaying dark matter scenarios alleviate both $H_0$ and $\sigma_8$ tensions?

Understand

Current tensions in cosmology, including $H_0$ and $\sigma_8$, provide one of the strong reasons to suspect the existence of physics beyond the standard model of cosmology ($\Lambda$CDM).

• In this paper, we investigate if there is a relation between these tensions and beyond cold dark matter scenarios.
• To model non-CDM, we assume a decaying dark matter (DDM) which is unstable and may decay into two daughter particles, a combination of cold dark matter, warm dark matter, and dark radiation, to explore a vast era of possibilities.
• We checked our model against CMB data and could show that decaying dark matter seems not a promising candidate to address the cosmological tensions.