Neutrino Fluence influenced by Memory Burdened Primordial Black Holes
Arnab Chaudhuri, Koushik Pal, Rukmani Mohanta

TL;DR
This study examines how quantum gravitational memory effects suppress neutrino signals from primordial black holes, showing that such suppression makes detection with IceCube unlikely under current constraints.
Contribution
It introduces a model incorporating memory burden effects into PBH evaporation, quantifies the impact on neutrino signals, and assesses detectability with current neutrino observatories.
Findings
Memory burden suppresses high-energy neutrino fluence from PBHs.
Heavy neutral lepton emissions can partially offset suppression in certain energy ranges.
Predicted neutrino event rates are well below IceCube sensitivity, even for optimistic scenarios.
Abstract
We study the impact of quantum gravitational memory burden - a backreaction effect that suppresses black hole evaporation - on neutrino signals from primordial black holes (PBHs). This suppression, modeled via a parameter k, reduces the high-energy muon neutrino fluence, particularly during the late stages of evaporation. We also consider beyond the Standard Model scenarios in which heavy neutral leptons (HNLs) are emitted by PBHs and subsequently decay, injecting secondary neutrinos that partially mitigate the suppression in the MeV-GeV range. We compute the full time-integrated neutrino spectrum and evaluate the expected IceCube event rates across the (k, mN) parameter space. We analyze both single source burst scenarios and the cumulative Galactic contribution assuming PBHs trace a realistic dark matter halo distribution. Even under optimistic proximity assumptions, the predicted…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
