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SUMMARY:Future LSS survey and Inflation models - Zhiqi Huang (IPhT Saclay/
 CEA)
DTSTART:20111111T130000Z
DTEND:20111111T140000Z
UID:TALK33685@talks.cam.ac.uk
CONTACT:Ian A. Morrison
DESCRIPTION:We forecast the constraint on the power spectrum of primordial
  scalar metric fluctuations with a Euclid-like future large-volume galaxy 
 survey and Planck CMB observations. While a large-volume galaxy survey can
  only marginally improve the constraint on the spectral index $n_s$ and it
 s running $\\alpha_s$\, we argue that\, for inflation models that predict 
 sharp features in the scalar power spectrum\, the galaxy survey can be an 
 crucial experiment to measure these features.
LOCATION:Pavilion B Potter Room (B1.19)
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