PIRSA:10060013

Video URL

https://pirsa.org/10060013

Holographic Non-Gaussianity

Skenderis, K. (2010). Holographic Non-Gaussianity. Perimeter Institute for Theoretical Physics. https://pirsa.org/10060013

Skenderis, Kostas. Holographic Non-Gaussianity. Perimeter Institute for Theoretical Physics, Jun. 15, 2010, https://pirsa.org/10060013 

          @misc{ scivideos_PIRSA:10060013,
            doi = {10.48660/10060013},
            url = {https://pirsa.org/10060013},
            author = {Skenderis, Kostas},
            keywords = {Quantum Fields and Strings},
            language = {en},
            title = {Holographic Non-Gaussianity},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2010},
            month = {jun},
            note = {PIRSA:10060013 see, \url{https://scivideos.org/index.php/pirsa/10060013}}
          }

Kostas Skenderis University of Southampton

Talk numberPIRSA:10060013
DOI10.48660/10060013
Source RepositoryPIRSA
Collection
Talk Type Conference
Subject

Abstract

We discuss holographic models for the inflationary epoch. We show how cosmological observables such as the primordial spectrum and non-Gaussianities can be computed via computations of correlation functions of a dual three dimensional QFT (without gravity!) We present a general class of models that have the following universal features: (i) they have a nearly scale invariant spectrum of small amplitude primordial fluctuations, (ii) the scalar spectral index runs as alpha_s = - (n_s-1), (iii) the three point function of density perturbations is exactly equal to the sum of the local and equilateral form with f_{NL}^{local} = 6 f_{NL}^{equil} = 20/3.