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SUMMARY:Cosmological neutrino mass detection in the next five years - Rupe
 rt Allison (Oxford)
DTSTART:20151209T134500Z
DTEND:20151209T141500Z
UID:TALK61969@talks.cam.ac.uk
CONTACT:Andrew Shannon
DESCRIPTION:Future cosmological measurements should enable the sum of neut
 rino masses to be determined indirectly through their effects on the expan
 sion rate of the Universe and the clustering of matter. I will discuss the
  cosmological effects of neutrinos and how they appear in CMB and large-sc
 ale structure observables. I will outline how the mass measurement may be 
 reached\, step-wise\, using data collected during the coming decade. Final
 ly\, I will explore the dependence of the mass constraint on experimental 
 details and examine degeneracies with other cosmological parameters.
LOCATION:Sackler Lecture Theatre\, IoA
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