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SUMMARY:Webinar: Re-Examining Astrophysical Constraints on the Dark Matter
  Model
DTSTART;VALUE=DATE-TIME:20141111T140000Z
DTEND;VALUE=DATE-TIME:20141111T150000Z
DTSTAMP;VALUE=DATE-TIME:20261013T060310Z
UID:indico-event-2366@indico.ific.uv.es
DESCRIPTION:\n    The cosmological model based on cold dark matter (CDM) a
 nd dark energy has been hugely successful in describing the observed evolu
 tion and large scale structure of our Universe.  However\, at small scale
 s (in the smallest galaxies and at the centers of larger galaxies)\, a num
 ber of observations seem to conflict with the predictions CDM cosmology\, 
 leading to recent interest in Warm Dark Matter (WDM) and Self-Interacting 
 Dark Matter (SIDM) models. These small scales\, though\, are also regions 
 dominated by the influence of baryons. I will present results from high re
 solution cosmological galaxy simulations that include both baryons and dar
 k matter to show that baryonic physics can significantly alter the dark ma
 tter structure and substructure of galaxies\, revolutionizing our expectat
 ions for galaxy structure and influencing our interpretation of the Dark M
 atter model.\n\nhttps://indico.ific.uv.es/event/2366/
LOCATION:IFIC retransimetted from Seminar Room\, 1.1.1
URL:https://indico.ific.uv.es/event/2366/
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