Evaporating Primordial Black Holes in Gamma Ray and Neutrino Telescopes
arXiv:2110.05637 · doi:10.1088/1475-7516/2021/12/051
Abstract
A primordial black hole in the last stages of evaporation and located in the local neighborhood can produce a detectable signal in gamma ray and neutrino telescopes. We re-evaluate the expected gamma ray and neutrino fluxes from these transient point events and discuss the consequences for existing constraints. For gamma rays we improve the current bounds by a factor of few, while for neutrinos we obtain significantly different results than the existing literature. The capability and advantages of neutrino telescopes in the search for primordial black holes is discussed thoroughly. The correlations of gamma ray and neutrino energy and time profiles will be promoted as a powerful tool in identifying the primordial black holes, in case of detection.
arXiv comment17 pages, 7 figures; v2: few clarifications and references added; v3: discussion on rotating PBHs expanded, matches the version published in JCAP
References in corpus (51)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- An Introduction to PYTHIA 8.2
- New cosmological constraints on primordial black holes
- The fate of hints: updated global analysis of three-flavor neutrino oscillations
- Letter of Intent for KM3NeT 2.0
- Primordial Black Holes as Dark Matter: Recent Developments
- Pulsational Pair-Instability Supernovae
- Primordial Black Holes as a dark matter candidate
- Time-integrated Neutrino Source Searches with 10 years of IceCube Data
- The Maximum Mass of a Neutron Star
- Atmospheric neutrino flux calculation using the NRLMSISE00 atmospheric model
- Primordial black holes as a dark matter candidate are severely constrained by the Galactic Center 511 keV gamma-ray line
- INTEGRAL constraints on primordial black holes and particle dark matter
- Mass Measurements of Stellar and Intermediate Mass Black-Holes
- Voyager 1 Further Constrain Primordial Black Holes as Dark Matter
- Black Hole Remnants and Dark Matter
- Neutrino and Positron Constraints on Spinning Primordial Black Hole Dark Matter
- BlackHawk v2.0: A public code for calculating the Hawking evaporation spectra of any black hole distribution
- A brief review on primordial black holes as dark matter
- Constraints on primordial black holes from Galactic gamma-ray background
- IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica
- Dark Matter Spectra from the Electroweak to the Planck Scale
- Direct Detection of Hawking Radiation from Asteroid-Mass Primordial Black Holes
- Planck Constraint on Relic Primordial Black Holes
- On the sensitivity of the HAWC observatory to gamma-ray bursts
- Measurement of the cosmic-ray antiproton spectrum at solar minimum with a long-duration balloon flight over Antarctica
- Constraining primordial black holes as dark matter using the global 21-cm signal with X-ray heating and excess radio background
- Near future MeV telescopes can discover asteroid-mass primordial black hole dark matter
- Do Evaporating Black Holes Form Photospheres?
- Constraining primordial black hole masses with the isotropic gamma ray background
- Pulsational Pair-instability Supernovae. I. Pre-collapse Evolution and Pulsational Mass Ejection
- Probing the stability of superheavy dark matter particles with high-energy neutrinos
- Dirac and Majorana neutrino signatures of primordial black holes
- On the formation of a Hawking-radiation photosphere around microscopic black holes
- Primordial Black Holes: Observational Characteristics of The Final Evaporation
- Constraints on amplitudes of curvature perturbations from primordial black holes
- Calculation of the emergent spectrum and observation of primordial black holes
- Measuring the local dark matter density with LAMOST DR5 and Gaia DR2
- New constraints on the origin of medium-energy neutrinos observed by IceCube
- On the Density of PBH's in the Galactic Halo
- Probing the Particle Spectrum of Nature with Evaporating Black Holes
- Milagro Limits and HAWC Sensitivity for the Rate-Density of Evaporating Primordial Black Holes
- New constraints on the primordial black hole number density from Galactic gamma-ray astronomy
- NEUTRINOS FROM PRIMORDIAL BLACK HOLES
- Constraining the Local Burst Rate Density of Primordial Black Holes with HAWC
- Where do IceCube neutrinos come from? Hints from the diffuse gamma-ray flux
- Primordial black holes in the Dark Ages: Observational prospects for future 21cm surveys
- Cosmological constraints from evaporations of primordial black holes
- Constraints on primordial black holes and primeval density perturbations from the epoch of reionization
- Future Constraints on Primordial Black Holes from XGIS-THESEUS
- Photon spectra from final stages of a primordial black hole evaporation in different theoretical models
Cited by in corpus (16)
- Primordial black hole constraints with Hawking radiation -- a review
- Background of radio photons from primordial black holes
- Light burden of memory: Constraining primordial black holes with high-energy neutrinos
- Black Hole Evaporation Beyond the Standard Model of Particle Physics
- High-Energy and Ultra-High-Energy Neutrinos from Primordial Black Holes
- TeV Dark Matter Searches in the Extragalactic Gamma-Ray Sky
- Determining the spin of light primordial black holes with Hawking radiation
- Electron-target experiment constraints on light dark matter produced in primordial black hole evaporation
- High-energy gamma-ray emission from memory-burdened primordial black holes
- Axion-like particles from primordial black hole evaporation and their detection in neutrino experiments
- Constraining primordial black holes as dark matter using AMS-02 data
- Identifying Spin Properties of Evaporating Black Holes through Asymmetric Neutrino and Photon Emission
- Explaining the PeV Neutrino Fluxes at KM3NeT and IceCube with Quasi-Extremal Primordial Black Holes
- Limits on primordial black holes detectability with Isatis: A BlackHawk tool
- Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints
- Sensitivities on non-spinning and spinning primordial black hole dark matter with global 21 cm troughs