APA

(2017). Testing early Universe physics with upcoming observations . Perimeter Institute. https://pirsa.org/17030093

MLA

Testing early Universe physics with upcoming observations . Perimeter Institute, Mar. 28, 2017, https://pirsa.org/17030093

BibTex

@misc{ pirsa_PIRSA:17030093,
  doi = {10.48660/17030093},
  url = {https://pirsa.org/17030093},
  author = {},
  keywords = {Cosmology},
  language = {en},
  title = {Testing early Universe physics with upcoming observations },
  publisher = {Perimeter Institute},
  year = {2017},
  month = {mar},
  note = {PIRSA:17030093 see, \url{https://pirsa.org}}
}
            

Abstract

Cosmology has seen great progress thanks to precision measurements and is bound to greatly benefit from upcoming Large Scale Structure and Cosmic Microwave Background data. I will point out a number of interesting directions. In particular, I discuss how the microphysics of inflation may be tested in galaxy surveys through “fossil” signatures originating from squeezed primordial correlations. I further elaborate on the constraining power of CMB spectral distortions on small-scale cosmological fluctuations and on particle decays in the very early Universe in relation to reheating. I also describe some of the possible constraints on inflation and reheating from future B-mode observations.