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SUMMARY:Cosmological Perturbation Theory - Jai-Chan Hwang\, Kyungpook/DAMT
 P
DTSTART:20200518T120000Z
DTEND:20200518T130000Z
UID:TALK141427@talks.cam.ac.uk
CONTACT:David Stefanyszyn
DESCRIPTION:Cosmological perturbation theory is an important theoretical p
 illar \nin the development and success of modern cosmology. Using the ADM 
 (3+1) formulation of Einstein's gravity a perturbation analysis valid to f
 ully nonlinear and exact order is possible. Being fully nonlinear and exac
 t it includes any order perturbation expansion as well as the post-Newtoni
 an approximation. We will explain some consequences of this formulation in
  cosmology and astrophysics. A related work we have devoted during our sta
 y in DAMTP will be explained as well.
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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