Cosmological constraints on the radiation released during structure formation

TL;DR

This paper investigates how future cosmological observations can constrain the density of astrophysical radiation backgrounds produced during structure formation, finding that only exotic sources beyond well-understood processes can be effectively limited.

Contribution

It models the impact of astrophysical radiation on cosmological parameters and forecasts constraints from upcoming surveys like LSST and Euclid.

Findings

Future observations constrain ARB density to <0.008 at 95% confidence.

Known astrophysical processes produce ARB density around 10^{-5}.

Cosmology can mainly constrain exotic or poorly understood radiation sources.

Abstract

During the process of structure formation in the universe matter is converted into radiation through a variety of processes such as light from stars, infrared radiation from cosmic dust and gravitational waves from binary black holes/neutron stars and supernova explosions. The production of this astrophysical radiation background (ARB) could affect the expansion rate of the universe and the growth of perturbations. Here, we aim at understanding to which level one can constraint the ARB using future cosmological observations. We model the energy transfer from matter to radiation through an effective interaction between matter and astrophysical radiation. Using future supernova data from LSST and growth-rate data from Euclid we find that the ARB density parameter is constrained, at the 95% confidence level, to be $\Omega_{ar_0}<0.008$. Estimates of the energy density produced by well-known astrophysical processes give roughly $\Omega_{ar_0}\sim 10^{-5}$. Therefore, we conclude that cosmological observations will only be able to constrain exotic or not-well understood sources of radiation.