The radio SZ effect as a probe of the cosmological radio background

Abstract

If there is a substantial cosmological radio background, there should be a radio Sunyaev-Zeldovich (SZ) effect that goes along with it. The radio background Comptonization leads to a slight photon excess at all wavelengths, while Comptonization of the CMB at low frequencies leads to a decrement. For levels of the radio background consistent with observations, these effects cancel each other around $\nu \simeq 735$MHz, with an excess at lower frequencies and a decrement at higher frequencies. Assuming a purely cosmological origin of the observed ARCADE radio excess, at $\nu \lesssim 20\mathrm{GHz}$ the signal scales as $\Delta T/T_{\mathrm{CMB}}\simeq 2y\left[(\nu /735\mathrm{MHz}{)}^{-2.59}-1\right]$ with frequency and the Compton-$y$ parameter of the cluster. For a typical cluster, the total radio SZ signal is at the level of $\Delta T\simeq 1\mathrm{mK}$ around the null, with a steep scaling towards radio frequencies. This is above current raw sensitivity limits for many radio facilities at these wavelengths, providing a unique way to confirm the cosmological origin of the ARCADE excess and probe its properties (e.g., redshift dependence and isotropy). We also give an expression to compute the radio-analogue of the kinematic SZ effect, highlighting that this might provide a new tool to probe large-scale velocity fields and the cosmic evolution of the radio background.

submitted to AAS Journals

References in corpus (2)

• CMB-S4 Science Case, Reference Design, and Project Plan
• Spectral distortion constraints on photon injection from low-mass decaying particles

Cited by in corpus (2)

• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• A closer look at dark photon explanations of the excess radio background