The Distortion of the Cosmic Microwave Background Spectrum Due to Intergalactic Dust

TL;DR

This paper estimates how intergalactic dust emission could interfere with future measurements of the CMB spectrum, revealing it may significantly contaminate signals of early Universe distortions.

Contribution

It provides the first quantitative estimate of intergalactic dust's foreground contamination on CMB spectral distortion measurements.

Findings

Intergalactic dust emission exceeds PIXIE sensitivity at z<0.5.

Upper limit of 0.23% on intergalactic dust contribution to far-infrared background.

Intergalactic dust emission could significantly impact future CMB spectral distortion detection.

Abstract

Infrared emission from intergalactic dust might compromise the ability of future experiments to detect subtle spectral distortions in the Cosmic Microwave Background (CMB) from the early Universe. We provide the first estimate of foreground contamination of the CMB signal due to diffuse dust emission in the intergalactic medium. We use models of the extragalactic background light to calculate the intensity of intergalactic dust emission and find that emission by intergalactic dust at redshifts z<0.5 exceeds the sensitivity of the planned Primordial Inflation Explorer (PIXIE) to CMB spectral distortions by 1-3 orders of magnitude. We place an upper limit of 0.23% on the contribution to the far-infrared background from intergalactic dust emission.