Probing the two-body decaying dark matter scenario with weak lensing and the cosmic microwave background

¹ Department of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
e-mail: jozef.bucko@uzh.ch
² Nordita, KTH Royal Institute of Technology and Stockholm University, Hannes Alfens väg 12, 106 91 Stockholm, Sweden
³ Université Paris-Saclay, Université Paris Cité, CEA, CNRS, Astrophysique, Instrumentation et Modélisation Paris-Saclay, 91191 Gif-sur-Yvette, France

Received: 29 August 2023
Accepted: 5 October 2023

Abstract

Decaying dark matter (DDM) scenarios have recently regained attention due to their potential ability to resolve the well-known clustering (or S₈) 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 (ΛDDM) scenario, including intrinsic alignment and baryonic feedback processes. We used the cosmic shear band power spectra from KiDS-1000 data and combined it with temperature and polarisation data from Planck in order to constrain the ΛDDM model. We report new limits on the decay rate and mass splitting parameters that are significantly stronger than previous results, especially in the case of low-mass splittings. Regarding the S₈ tension, we found a reduction from about 3 to 2σ, depending on which statistical measure is applied. We therefore conclude that the two-body ΛDDM model is able to reduce the S₈ tension without convincingly solving it.