Primordial Black Holes, Hawking Radiation and the Early Universe
arXiv:hep-ph/0503267 · doi:10.1142/S0217732305017688
Abstract
The 511 keV gamma emission from the galactic core may originate from a high concentration () of primordial black holes (PBHs) in the core each of whose Hawking radiation includes positrons per second. The PBHs we consider are taken as near the lightest with longevity greater than the age of the universe (mass kg; Schwarzschild radius fm). These PBHs contribute only a small fraction of cold dark matter, . This speculative hypothesis, if confirmed implies the simultaneous discovery of Hawking radiation and an early universe phase transition.
4 Pages
Cited by in corpus (18)
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- Gamma ray bursts and the origin of galactic positrons
- The 511 keV Excess and Primordial Black Holes
- 511 KeV photons from superconducting cosmic strings
- Primordial black holes and the observed Galactic 511 keV line
- Unification of Dark Energy and Dark Matter
- Spectroscopy of a canonically quantized horizon
- The Sensitivity of Future Gamma-Ray Telescopes to Primordial Black Holes
- Black hole radiation spectrum in LQG: Isolated Horizon framework
- Dark Matter: the Connection with Gamma-Ray Astrophysics
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- Quantum amplification effect in a horizon fluctuations
- The Dark Dimension, the Swampland, and the Dark Matter Fraction Composed of Primordial Black Holes