Constraints on decaying dark matter from weak lensing and cluster counts
  We revisit a cosmological constraint on dark matter decaying into dark
radiation at late times. In Enqvist et al. (2015), we mainly focused on the
effects of decaying dark matter (DDM) on the cosmic microwave background (CMB)
and nonlinear matter power spectrum. Extending our previous analysis, here we
use N-body simulation to investigate how DDM affects the halo mass function.
This allows us to incorporate the cluster counts observed by the
Sunyaev-Zel'dovich effect to study a bound on the lifetime of DDM. We also
update the data of CMB and cosmic shear power spectrum with the Planck 2015
results and KiDS450 observations, respectively. From these cosmological
observations, we obtain an lower bound on the lifetime $\Gamma^{-1}\ge
175\,$Gyr from the Planck2015 results (CMB+SZ cluster count) combined with the
KiDS450 and the recent measurements of the baryon acoustic scale.
