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SUMMARY:Understanding the large-scale structure of the Universe
DTSTART:20190319T121500
DTSTAMP:20260602T162317Z
UID:4e5a64308f2d26d98365b77405d8d99edbfa8fa38c40df8e79ef56a1
CATEGORIES:Conferences - Seminars
DESCRIPTION:Sergey Sibiryakov\nDistribution of matter on super-galactic sc
 ales encodes a wealth of information about the constituents of our Univers
 e\, its evolution and initial conditions. An efficient extraction of this 
 information requires accurate analytic and numerical methods to capture th
 e non-linear dynamics of gravitational clustering starting from stochastic
  primordial density inhomogeneities. I will describe an approach based on 
 path integral representation for the cosmological observables and will ill
 ustrate in a number of applications how it allows us to systematically im
 prove the precision of theoretical predictions. I will also briefly discus
 s the generalisation of these techniques to search for new physics beyond 
 the standard cosmological model.
LOCATION:BSP 233 https://plan.epfl.ch/?room==BSP%20233
STATUS:CONFIRMED
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