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A dissipative dark sector can result in the formation of compact objects withmasses comparable to stars and planets. In this work, we investigate theformation of such compact objects from a subdominant inelastic dark mattermodel, and study the resulting distributions of these objects. In particular,we consider cooling from dark Bremsstrahlung and a rapid decay process thatoccurs after inelastic upscattering. Inelastic transitions introduce anadditional radiative processes which can impact the formation of compactobjects via multiple cooling channels. We find that having multiple coolingprocesses changes the mass and abundance of compact objects formed, as comparedto a scenario with only one cooling channel. The resulting distribution ofthese astrophysical compact objects and their properties can be used to furtherconstrain and differentiate between dark sectors.

The Effect of Multiple Cooling Channels on the Formation of Dark Compact Objects