Randomness in the Dark Sector: Emergent Mass Spectra and Dynamical Dark Matter Ensembles
Keith R. Dienes, Jacob Fennick, Jason Kumar, Brooks Thomas

TL;DR
This paper explores how random processes can generate mass spectra in dark sectors, resulting in a naturally balanced ensemble of dark matter components with potential observable signals.
Contribution
It introduces a statistical model for emergent dark sector mass spectra, demonstrating their compatibility with Dynamical Dark Matter and analyzing observational prospects.
Findings
Density of states decreases with mass and has an upper limit.
Emergent spectra balance cosmological abundances and decay widths.
Randomly generated spectra are compatible with dark matter phenomenology.
Abstract
In general, non-minimal models of the dark sector such as Dynamical Dark Matter posit the existence of an ensemble of individual dark components with differing masses, cosmological abundances, and couplings to the Standard Model. Perhaps the most critical among these features is the spectrum of masses, as this goes a long way towards determining the cosmological abundances and lifetimes of the corresponding states. Many different underlying theoretical structures can be imagined for the dark sector, each giving rise to its own mass spectrum and corresponding density of states. In this paper, by contrast, we investigate the spectrum of masses that emerges statistically from underlying processes which are essentially random. We find a density of states which decreases as a function of mass and actually has an upper limit beyond which . We also demonstrate that…
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