Speaker
Martin Bucher
(APC/CNRS)
Description
Most of the emphasis so far on connecting CMB observations to theories of the primordial universe has focused
on exploiting the primordial power spectrum. However the constraints established on the maximum amount of
non-Gaussianity allowed severely limit the scope for alternative models. I will review these developments as
well as the prospects for improving on current observations. I will also present some new ways in which the
presently available data can be analyzed.
Primary author
Martin Bucher
(APC/CNRS)
