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2018

Cosmological bounds on dark matter-photon coupling

Kumar, Suresh, Nunes, Rafael C., Yadav, Santosh Kumar

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We investigate an extension of the $\Lambda$CDM model where the dark matter (DM) is coupled to photons, inducing a nonconservation of the numbers of particles for both species, where the DM particles are allowed to dilute throughout the cosmic history with a small deviation from the standard evolution decaying into photons, while the associated scattering processes are assumed to be negligible.

In addition, we consider the presence of massive neutrinos with the effective number of species $N_{\rm eff}$ as a free parameter.
The effects of the DM-photon coupling on the cosmic microwave background (CMB) and matter power spectra are analyzed.
We derive the observational constraints on the model parameters by using the data from CMB, baryonic acoustic oscillation (BAO) measurements, the recently measured new local value of the Hubble constant from the Hubble Space Telescope, and large scale structure (LSS) information from the abundance of galaxy clusters.