Probing the two-body decaying dark matter scenario with weak lensing and the cosmic microwave background
Jozef Bucko, Sambit K. Giri, Fabian Hervas Peters, Aurel Schneider

TL;DR
This study investigates a two-body decaying dark matter model using weak lensing and CMB data, finding it can reduce the $S_8$ tension but not fully resolve it, with new constraints on decay parameters.
Contribution
First fully non-linear weak lensing analysis of the two-body decaying dark matter scenario including baryonic effects and intrinsic alignments, providing stronger constraints and insights.
Findings
Significantly improved limits on decay rate and mass splitting.
Reduction of the $S_8$ tension from 3 to 2 sigma.
Model cannot fully resolve the $S_8$ tension.
Abstract
Decaying dark matter (DDM) scenarios have recently regained attention due to their potential ability to resolve the well-known clustering (or ) tension between weak lensing (WL) and cosmic microwave background (CMB) measurements. In this paper, we investigate a well-established model where the original dark matter particle decays into a massless particle and a massive daughter particle. The latter obtains a velocity kick during the decay process that results in the suppression of the matter power spectrum at scales that are observable with WL shear observations. We perform the first fully non-linear WL analysis of this two-body decaying dark matter (DDM) scenario, including intrinsic alignment and baryonic feedback processes. We used the cosmic shear band power spectra from \textit{KiDS-1000} data and combined it with temperature and polarisation data from \texttt{Planck}…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Scientific Research and Discoveries
