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SUMMARY:The challenge of neutrino mass detection from cosmology - Maria Ar
 chidiacono
DTSTART:20200504T120000Z
DTEND:20200504T130000Z
UID:TALK141424@talks.cam.ac.uk
CONTACT:David Stefanyszyn
DESCRIPTION:Massive neutrinos modify the expansion history of the Universe
  and the formation of structures. Up-to-date cosmological data can provide
  very tight\, yet model dependent\, upper limits on the neutrino mass sum.
  In the next decade one of the goals of precision cosmology will be to pin
  down the absolute neutrino mass.\nIn this talk I will discuss the physica
 l effects induced by massive neutrinos on cosmological observables\, revie
 wing current constraints and elaborating on their interpretation.\nI will 
 then focus on the theoretical challenges of the analysis of data from upco
 ming galaxy surveys\, showing how cosmology can detect a non-zero neutrino
  mass.
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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