Speaker
Dr
Nicholas Orlofsky
(Carleton University)
Description
Magnetically charged black holes are interesting solutions of the Standard Model and general relativity. They may possess a “hairy” electroweak-symmetric corona outside the event horizon, which speeds up their Hawking radiation and leads them to become nearly extremal on short timescales. Their masses could range from the Planck scale up to the Earth mass. I will present various methods to search for primordially produced magnetic black holes and provide estimated upper limits on their abundance.
Author
Dr
Nicholas Orlofsky
(Carleton University)
Co-authors
Yang Bai
Joshua Berger
Mrunal Korwar
Sida Lu
