PIRSA:06040009

Video URL

https://pirsa.org/06040009

Expressing the equation of state parameter in terms of the three dimensional cosmic shear

Brustein, R. (2006). Expressing the equation of state parameter in terms of the three dimensional cosmic shear. Perimeter Institute for Theoretical Physics. https://pirsa.org/06040009

Brustein, Ramy. Expressing the equation of state parameter in terms of the three dimensional cosmic shear. Perimeter Institute for Theoretical Physics, Apr. 11, 2006, https://pirsa.org/06040009 

          @misc{ scivideos_PIRSA:06040009,
            doi = {10.48660/06040009},
            url = {https://pirsa.org/06040009},
            author = {Brustein, Ramy},
            keywords = {Cosmology},
            language = {en},
            title = {Expressing the equation of state parameter in terms of the three dimensional cosmic shear},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2006},
            month = {apr},
            note = {PIRSA:06040009 see, \url{https://scivideos.org/pirsa/06040009}}
          }

Ramy Brustein Ben-Gurion University of the Negev

Talk numberPIRSA:06040009
DOI10.48660/06040009
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

We express the total equation of state parameter of a spatially flat Friedman-Robertson-Walker universe in terms of derivatives of the red-shift dependent spin-weighted angular moments of the two-point correlation function of the three dimensional cosmic shear. In the talk I will explain all the technical terms in the first sentence, I will explain how such an expression is obtained and highlight its relevance for determining the expansion history of the universe.