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Testing Early Universe Physics with Upcoming Observations – Emanuela Dimastrogiovanni

Date: Wed. February 10th, 2016, 12:30 pm-1:30 pm
Location: Rockefeller 221

Cosmology has seen tremendous progress thanks to precision measurements and is bound to greatly benefit from upcoming Large Scale Structure and Cosmic Microwave Background data. I will point out a number of interesting directions. In particular, I discuss how the microphysics of inflation may be tested in galaxy surveys through “fossil” signatures originating from squeezed primordial correlations. I further elaborate on the constraining power of CMB spectral distortions on small-scale cosmological fluctuations and on particle decays in the very early Universe in relation to reheating. I also describe some of the possible constraints on inflation and reheating from future B-mode observations.

Page last modified: May 12, 2016