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SUMMARY:On the phenomenology of gamma-ray signals emitted from generic cas
 cade processes.
DTSTART;VALUE=DATE-TIME:20151130T110000Z
DTEND;VALUE=DATE-TIME:20151130T120000Z
DTSTAMP;VALUE=DATE-TIME:20260926T141013Z
UID:indico-event-2613@indico.ific.uv.es
DESCRIPTION:Dark matter remains to be the single paradigm which explains a
  handful of unexpected gravitational observations ranging from galactic up
  to cosmic scales. It is a fundamental ingredient of the LCDM model and cu
 rrently an active field of research. If dark matter is of particle nature 
 and interacts similarly to all known constituents of matter\, it may annih
 ilate or decay producing a detectable flux of standard model particles. If
  this fluxes eventually overcome astrophysical backgrounds it enables us t
 o detect indirectly an event of dark matter origin. Gamma rays are one of 
 the possible channels and a promising messenger candidate. We focus on the
 se and explore the different possible signatures of dark matter in the cos
 mic photon flux. Then we explore in more detail the phenomenology of gamma
 -ray arising from cascade processes involving scalars or fermions.\n\nhttp
 s://indico.ific.uv.es/event/2613/
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/2613/
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