Primordial non-Gaussianity
APA
Vernizzi, F. (2007). Primordial non-Gaussianity. Perimeter Institute. https://pirsa.org/07090001
MLA
Vernizzi, Filippo. Primordial non-Gaussianity. Perimeter Institute, Sep. 18, 2007, https://pirsa.org/07090001
BibTex
@misc{ pirsa_PIRSA:07090001, doi = {10.48660/07090001}, url = {https://pirsa.org/07090001}, author = {Vernizzi, Filippo}, keywords = {Cosmology}, language = {en}, title = {Primordial non-Gaussianity}, publisher = {Perimeter Institute}, year = {2007}, month = {sep}, note = {PIRSA:07090001 see, \url{https://pirsa.org}} }
The Abdus Salam International Centre for Theoretical Physics (ICTP)
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Abstract
The non-Gaussianity of the primordial cosmological perturbations will be strongly constrained by future observations like Planck. It will provide us with important information about the early universe and will be used to discriminate among models. I will review how different models of the early universe can generate different amount and shapes of non-Gaussianity.