BlackHawk: A tool for computing Black Hole evaporation

Auffinger, Jérémy; Arbey, Alexandre

doi:10.22323/1.392.0024

Cited by 2 publications

(1 citation statement)

References 32 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…Since the preceding TOOLS2020 conference [26], BlackHawk has received much upgrades, including the possibility of BSM particle emission, HR from non-standard BH solutions and a careful treatment of hadronization at low-and high-energy. BlackHawk continues to be updated to incorporate new features, the last to date being the Isatis tool that computes automatically the constraints on PBHs from HR with a wide range of instruments [27].…”

Section: Discussionmentioning

confidence: 99%

Beyond the Standard Model with BlackHawk v2.0

Auffinger¹,

Arbey²

2022

Proceedings of Computational Tools for High Energy Physics and Cosmology — PoS(CompTools2021)

Self Cite

View full text Add to dashboard Cite

We present the new version of BlackHawk v2. . BlackHawk is a public code designed to compute the Hawking radiation (HR) spectra of (primordial) black holes (PBHs). In the version 2. , we have added several non-standard BH metrics: charged, higher dimensional and polymerized black holes, in addition to the usual rotating (Kerr) BHs. BlackHawk also embeds some additional scripts and numerical tables that can prove useful in e.g. dark matter (DM) studies. We will describe these new features and provide some examples of the capabilities of the code. A tutorial for BlackHawk is available on the TOOLS2021 website: https://indico.cern.ch/event/1 76291/contributions/46 9967/

show abstract

Section: Discussionmentioning

confidence: 99%

Beyond the Standard Model with BlackHawk v2.0

Auffinger¹,

Arbey²

2022

Proceedings of Computational Tools for High Energy Physics and Cosmology — PoS(CompTools2021)

Self Cite

View full text Add to dashboard Cite

show abstract

Current and future neutrino limits on the abundance of primordial black holes

Bernal

Muñoz-Albornoz

Palomares‐Ruiz

et al. 2022

J. Cosmol. Astropart. Phys.

View full text Add to dashboard Cite

Primordial black holes (PBHs) formed in the early Universe are sources of neutrinos emitted via Hawking radiation. Such astrophysical neutrinos could be detected at Earth and constraints on the abundance of comet-mass PBHs could be derived from the null observation of this neutrino flux. Here, we consider non-rotating PBHs and improve constraints using Super-Kamiokande neutrino data, as well as we perform forecasts for next-generation neutrino (Hyper-Kamiokande, JUNO, DUNE) and dark matter (DARWIN, ARGO) detectors, which we compare. For PBHs less massive than ∼ few × 1014 g, PBHs would have already evaporated by now, whereas more massive PBHs would still be present and would constitute a fraction of the dark matter of the Universe. We consider monochromatic and extended (log-normal) mass distributions, and a PBH mass range spanning from 1012 g to ∼ 1016 g. Finally, we also compare our results with previous ones in the literature.

show abstract

BlackHawk: A tool for computing Black Hole evaporation

Cited by 2 publications

References 32 publications

Beyond the Standard Model with BlackHawk v2.0

Beyond the Standard Model with BlackHawk v2.0

Current and future neutrino limits on the abundance of primordial black holes

Contact Info

Product

Resources

About