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Friday, 21 October 2011, 15:30 in AQ3149
Prof. Andrei Frolov (SFU)
Staring at the sky (physics colloquium)
Cosmic microwave background (CMB) carries to us a snapshot of the Universe from the times when it was much younger than it is today. Small anisotropies in CMB temperature are caused by fluctuations of gravitational potential at recombination, which photons have to climb out of. In inflationary cosmology, these are created by primordial quantum fluctuations of the field driving the accelerated expansion of the Universe, and are essentially Gaussian random noise of nearly scale-invariant spectrum. CMB anisotropy spectrum has been mapped out to exquisite precision over the last decade. Is there anything new we could see? In this talk, I will discuss searching for non-Gaussianity in the CMB - the distortions and patterns hidden in the noise, and what they could tell us about the early Univese physics.
Seminars in 2011:
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Modified by Andrei Frolov <frolov@sfu.ca> on 2023-11-01