BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Tracking the nature of DM in the Local Universe
DTSTART;VALUE=DATE-TIME:20190314T104000Z
DTEND;VALUE=DATE-TIME:20190314T110000Z
DTSTAMP;VALUE=DATE-TIME:20260521T052722Z
UID:indico-contribution-326@events.ncbj.gov.pl
DESCRIPTION:Speakers: Wojciech Hellwing (CTF PAS)\nI shall describe some p
 romising features of our Local Universe that can help reveal some feature 
 of a particle DM candidate. Simulations of galaxy and DM structure formati
 on of warm\, cold and self-interacting DM candidates indicate that feature
 s of the Galactic and M31 halo like: tidal streams gaps\, satellite galaxi
 es orbit parameter distribution and their internal properties can differ s
 ignificantly in different DM candidate scenarios. Observations that the LS
 ST will foster will allow us to use these features as potential DM tale-te
 ll.\n\nhttps://events.ncbj.gov.pl/event/10/contributions/326/
LOCATION:
URL:https://events.ncbj.gov.pl/event/10/contributions/326/
END:VEVENT
END:VCALENDAR