Cosmological Constraints on Unstable Particles: Numerical Bounds and Analytic Approximations

TL;DR

This paper develops numerical bounds and simple analytic formulas to constrain ensembles of unstable particles in the early universe, aiding future theoretical models with cosmological decay constraints.

Contribution

It introduces a comprehensive analysis of cosmological constraints on particle ensembles and provides practical analytic approximations for broad classes of models.

Findings

Numerical bounds on decaying particle ensembles derived from cosmological data.

Analytic approximations applicable to generic unstable particle ensembles.

A reference table summarizing constraints for various scenarios.

Abstract

Many extensions of the Standard Model predict large numbers of additional unstable particles whose decays in the early universe are tightly constrained by observational data. For example, the decays of such particles can alter the ratios of light-element abundances, give rise to distortions in the cosmic microwave background, alter the ionization history of the universe, and contribute to the diffuse photon flux. Constraints on new physics from such considerations are typically derived for a single unstable particle species with a single well-defined mass and characteristic lifetime. In this paper, by contrast, we investigate the cosmological constraints on theories involving entire ensembles of decaying particles --- ensembles which span potentially broad ranges of masses and lifetimes. In addition to providing a detailed numerical analysis of these constraints, we also formulate a set of simple analytic approximations for these constraints which may be applied to generic ensembles of unstable particles which decay into electromagnetically-interacting final states. We then illustrate how these analytic approximations can be used to constrain a variety of toy scenarios for physics beyond the Standard Model. For ease of reference, we also compile our results in the form of a table which can be consulted independently of the rest of the paper. It is thus our hope that this work might serve as a useful reference for future model-builders concerned with cosmological constraints on decaying particles, regardless of the particular model under study.