Ultralight Axions Versus Primordial Black Holes
arXiv:2102.11826 · doi:10.1142/S0217732321502412
Abstract
We reconsider entropy arguments which have been previously argued to support the idea that the dark matter constituents are primordial black holes with many solar masses. It has recently been shown that QCD axions which solve the strong CP problem may have masses in the extended range . Ultralight axions provide so many degrees of freedom that their entropy can exceed that of primordial black holes. This suggests that ultralight axions are more suited than primordial black holes to be constituents of dark matter.
arXiv comment12 pages
References in corpus (14)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Ultralight scalars as cosmological dark matter
- The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations
- Primordial Black Holes as All Dark Matter
- Solving the Hierarchy Problem Discretely
- An even lighter QCD axion
- Constraints on Stupendously Large Black Holes
- Dark matter from an even lighter QCD axion: trapped misalignment
- An ultralight pseudoscalar boson
- A new direction for dark matter research: intermediate mass compact halo objects
- Searching for Dark Matter Constituents with Many Solar Masses
- Non-linearly realized discrete symmetries
- On the Origin and Nature of Dark Matter
- Anomalies and parities for quintessential and ultra-light axions