Decaying Dark Matter in Halos of Primordial Black Holes
arXiv:1811.05810 · doi:10.1140/epjc/s10052-019-7173-x
Abstract
We investigate photon signatures of general decaying dark-matter particles in halos of primordial black holes. We derive the halo-profile density and the total decay rate for these combined dark-matter scenarios. For the case of axion-like particles of masses below keV, we find strong bounds on the decay constant which are several orders of magnitude stronger than the strongest existing bounds, for all halo masses above solar masses. Using future X-ray measurements, it will be possible to push these bounds on such combined dark-matter scenarios even further.
5 pages, 3 figures; v2: revised in order to match published version
References in corpus (9)
- Primordial Black Holes as Dark Matter
- The Dawn of FIMP Dark Matter: A Review of Models and Constraints
- Microlensing and dynamical constraints on primordial black hole dark matter with an extended mass function
- WIMPs and stellar-mass primordial black holes are incompatible
- Primordial black holes from inflaton and spectator field perturbations in a matter-dominated era
- Dark Matter Density Spikes around Primordial Black Holes
- Novel Constraints on Mixed Dark-Matter Scenarios of Primordial Black Holes and WIMPs
- Primordial Black Holes With Multi-Modal Mass Spectra
- Signatures of Compact Halos of Sterile-Neutrino Dark Matter