https://indico.cern.ch/event/191407/
Jinn-Ouk Gong
We overview the theoretical background to understand the cosmological
observables, the cosmic microwave background CMB) and large scale structure
(LSS) of galaxy distribution. We can study the statistical characters of
the primordial perturbations from which both CMB and LSS originated, and
they provide crucial information on the early universe when the energy
scale was far greater than what the LHC can probe. Some recent observations
for CMB and LSS are briefly reviewed.