Dissipative Dark Cosmology: From Early Matter Dominance to Delayed Compact Objects

TL;DR

This paper proposes a new cosmological model where dissipative dark matter leads to early matter dominance, formation of dark halos, and late-time creation of black holes and compact objects, potentially accounting for dark matter.

Contribution

It introduces a mechanism for dark matter to form primordial black holes and compact objects through a dissipative dark sector and a delayed phase transition.

Findings

Dark matter can dominate early, forming halos that collapse into black holes and compact objects.

Compact objects can have masses from 10^{20} g to 10^{32} g, and black holes from 10^{8} g to 10^{34} g.

Some of these objects could constitute a significant fraction of dark matter.

Abstract

We demonstrate a novel mechanism for producing dark compact objects and black holes through a dark sector, where all the dark matter can be dissipative. Heavy dark sector particles with masses above $10^4$ GeV can come to dominate the Universe and yield an early matter-dominated era before Big Bang Nucleosynthesis (BBN). Density perturbations in this epoch can grow and collapse into tiny dark matter halos, which cool via self interactions. The typical halo size is set by the Hubble length once perturbations begin growing, offering a straightforward prediction of the halo size and evolution depending on ones choice of dark matter model. Once these primordial halos have formed, a thermal phase transition can then shift the Universe back into radiation domination and standard cosmology. These halos can continue to collapse after BBN, resulting in the late-time formation of fragmented dark compact objects and sub-solar mass primordial black holes. We find that these compact objects can constitute a sizable fraction of all of dark matter. The resulting fragments can have masses between $10^{20}$ g to $10^{32}$ g, with radii ranging from $10^{-2}$ m to $10^5$ m, while the black holes can have masses between $10^{8}$ g to $10^{34}$ g. Furthermore, a unique feature of this model is the late-time formation of black holes which can evaporate today. We compare where these objects lie with respect to current primordial black hole and and massive (astrophysical) compact halo object constraints.