BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Webinar: Gravitational Waves as a New Probe of Dark Matter
DTSTART;VALUE=DATE-TIME:20161108T140000Z
DTEND;VALUE=DATE-TIME:20161108T150000Z
DTSTAMP;VALUE=DATE-TIME:20260504T143107Z
UID:indico-event-2846@indico.ific.uv.es
DESCRIPTION:\n    A dark matter (DM) halo intervening along the line of si
 ght of a gravitational wave (GW) signal could induce a change in the speed
  of GW. We show that this change of speed is observable with the current L
 IGO sensitivity for a class of ultralight DM models which could form a Bos
 e-Einstein condensate (BEC) in the early universe and behave as a single c
 oherent wave instead of individual particles in galaxies. Hence\, we propo
 se to use the deviation in the speed of GW as a new probe of the BEC DM pa
 rameter space. With a multi-messenger approach to GW astronomy and/or with
  extended sensitivity to lower GW frequencies\, the entire BEC DM paramete
 r space can be effectively probed by our new method in the near future.\n 
    \n    Connect from: http://reunion.uv.es/webinar08112016/\n\nhttps://in
 dico.ific.uv.es/event/2846/
LOCATION:IFIC retransmitted from Seminar Room\, 1.1.1
URL:https://indico.ific.uv.es/event/2846/
END:VEVENT
END:VCALENDAR