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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-3451
DTSTART:20141209T210000Z
DTEND:20141209T220000Z
DTSTAMP:20260312T231401Z
LAST-MODIFIED:20141105T155922Z
LOCATION:5280 Chamberlin Hall
SUMMARY:Boosting Dark Matter Indirect Detection Signals with Black Hol
 es\, Theory Seminar (High Energy/Cosmology)\, Jessie Shelton
DESCRIPTION:Super-massive black holes that grow at the center of dark 
 matter halos distort the dark matter within their zone of influence in
 to a steep density spike.  Besides giving rise to strong enhancements 
 of standard indirect detection signals\, this spike can lead to qualit
 atively new windows into the physics of the early universe.   I will t
 alk about potential dark matter signals from the Milky Way's central b
 lack hole\, some astrophysical caveats\, and the possible use of black
  holes as dark matter accelerators.
URL:https://www.physics.wisc.edu/events/?id=3451
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