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SUMMARY:Composite strongly interacting dark matter
DTSTART;VALUE=DATE-TIME:20140724T093000Z
DTEND;VALUE=DATE-TIME:20140724T103000Z
DTSTAMP;VALUE=DATE-TIME:20261013T032202Z
UID:indico-event-2265@indico.ific.uv.es
DESCRIPTION:\n    It has been suggested that cold dark matter has difficul
 ties in explaining tentative evidence for noncuspy halo profiles in small 
 galaxies\, and the low velocity dispersions observed in the largest Milky 
 Way satellites ("too big to fail" problem). Strongly self-interacting dark
  matter has been noted as a robust solution to these problems. The elastic
  cross sections required are much larger than predicted by generic CDM mod
 els\, but could naturally be of the right size if dark matter is composite
 . I will present a general way on constraining models where strongly inter
 acting CDM is in the form of dark "atoms" or "molecules"\, or bound states
  of a confining gauge interaction ("hadrons").\n\nhttps://indico.ific.uv.e
 s/event/2265/
LOCATION:IFIC Seminar Room\, 1.1.1
URL:https://indico.ific.uv.es/event/2265/
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