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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-7940
DTSTART:20220927T190000Z
DURATION:PT1H0M0S
DTSTAMP:20260414T153416Z
LAST-MODIFIED:20220923T195235Z
LOCATION:Join Zoom Meeting https://berkeley.zoom.us/j/91230714547  Mee
 ting ID: 912 3071 4547
SUMMARY:Distribution Functions of Dark Matter Halos\, Network in Neutr
 inos\, Nuclear Astrophysics\, and Symmetries (N3AS) Seminar\, Axel Gro
 ss \, University of Minnesota
DESCRIPTION:The spherical NFW profile provides a good approximation to
  the density distributions of dark matter halos. In dynamical equilibr
 ium\, this density profile should correspond to a stationary distribut
 ion function of dark matter in phase space. We derive this distributio
 n function and show that it is a good match to those obtained from N-b
 ody simulations.<br>
\n<br>
\nHost: Baha Balantekin<br>
\n<br>
\nJoin 
 Zoom Meeting<br>
\nhttps://berkeley.zoom.us/j/91230714547<br>
\n<br>
\
 nMeeting ID: 912 3071 4547<br>
\n
URL:https://www.physics.wisc.edu/events/?id=7940
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