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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:1
UID:UW-Physics-Event-6321
DTSTART:20210212T200000Z
DTEND:20210212T210000Z
DTSTAMP:20260415T003620Z
LAST-MODIFIED:20210211T223105Z
LOCATION:For zoom link\, sign up at: https://groups.google.com/a/g-gro
 ups.wisc.edu/d/forum/theoryseminars/join
SUMMARY:Phenomenology of Magnetic Black Holes\, Theory Seminar (High E
 nergy/Cosmology)\, Nicholas Orlofsky\, Carleton University
DESCRIPTION:Magnetically charged black holes are interesting solutions
  of the Standard Model and general relativity. They may possess a “h
 airy” electroweak-symmetric corona outside the event horizon\, which
  speeds up their Hawking radiation and leads them to become nearly ext
 remal on short timescales. Their masses could range from the Planck sc
 ale up to the Earth mass. I will present various methods to search for
  primordially produced magnetic black holes and provide estimated uppe
 r limits on their abundance.
URL:https://www.physics.wisc.edu/events/?id=6321
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