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SUMMARY:Dark Matter Clues from the Faintest Galaxies
DTSTART;VALUE=DATE-TIME:20250618T103000Z
DTEND;VALUE=DATE-TIME:20250618T113000Z
DTSTAMP;VALUE=DATE-TIME:20260808T013243Z
UID:indico-event-8133@indico.ific.uv.es
DESCRIPTION:Lambda Cold Dark Matter (LCDM) is the most successful theory f
 or the formation of structure in the Universe. Although its predictions ha
 ve been verified on large scales\, they are still contested on the scale o
 f dwarf galaxies\, whose dynamical properties are often cited as evidence 
 for the need to revise some of LCDM’s basic tenets. In this context\, I 
 will discuss the recent discovery of the faintest galaxies known to date\,
  and how their properties may be used to place constraints on the clusteri
 ng of dark matter on the smallest galactic and sub-galactic scales\, as we
 ll as on the viability of some of the proposed alternatives to LCDM.\n\n 
 \n\n\n\nLink to the recorded colloquium\n\nhttps://indico.ific.uv.es/event
 /8133/
LOCATION:PCUV Salón de Actos
URL:https://indico.ific.uv.es/event/8133/
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