Constraining the Rate of Primordial Black-Hole Explosions and Extra Dimension Scale using a Low-Frequency Radio Antenna Array
Sean E. Cutchin, John H. Simonetti, Steven W. Ellingson, Amanda S., Larracuente, Michael J. Kavic

TL;DR
This study uses low-frequency radio observations to set new upper limits on the rate of primordial black-hole explosions and constraints on extra dimension scales, with implications for astrophysics and fundamental physics.
Contribution
It introduces a novel radio-based search method for PBH explosions and provides the strongest observational constraints to date on their explosion rates and extra dimension models.
Findings
No signals detected in 4 hours of data.
Set an upper limit of 4.2 x 10^{-7} pc^{-3} yr^{-1} for PBH explosions.
Constraints on extra dimension scale of 3.0 x 10^{-18} m.
Abstract
An exploding primordial black-hole (PBH) may produce a single pulse of electromagnetic radiation detectable at the low-frequency end of the radio spectrum. Furthermore, a radio transient from an exploding PBH could be a signature of an extra spatial dimension. We describe here an approach for searching for PBH explosions using a low-frequency radio antenna array, and as a practical example, the results of a such a search using the Eight-meter-wavelength Transient Array (ETA). No compelling astrophysical signal was detected in hours of data implying an observational upper limit on the rate of exploding PBHs is for an exploding PBH with a fireball Lorentz factor of for the standard scenario of Page and Hawking. This rate limit is the strongest constraint yet set for PBH explosions with this fireball Lorentz factor.…
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.
