Constraining primordial non-Gaussianity with large-scale structure
APA
Verde, L. (2010). Constraining primordial non-Gaussianity with large-scale structure. Perimeter Institute. https://pirsa.org/10060023
MLA
Verde, Licia. Constraining primordial non-Gaussianity with large-scale structure. Perimeter Institute, Jun. 17, 2010, https://pirsa.org/10060023
BibTex
@misc{ pirsa_PIRSA:10060023, doi = {10.48660/10060023}, url = {https://pirsa.org/10060023}, author = {Verde, Licia}, keywords = {}, language = {en}, title = {Constraining primordial non-Gaussianity with large-scale structure}, publisher = {Perimeter Institute}, year = {2010}, month = {jun}, note = {PIRSA:10060023 see, \url{https://pirsa.org}} }
Institute of Space Sciences
Talk Type
Abstract
Constraining primordial non-Gaussianity can offer a window into the early universe, and into testing the inflationary paradigm, which is fully complementary to the approach offered by Cosmic Microwave Background polarization.
Large-scale structure and galaxy surveys have recently received renewed attention as a way to constrain primordial non-Gaussianity. I will review the potential and the limitations of this approach and highlight its complementarity to Cosmic Microwave Background observations.