PIRSA:22050022

Video URL

https://pirsa.org/22050022

Fundamental physics from remote velocity and quadrupole reconstruction with the cosmic microwave background and galaxy surveys

Hotinli, S. (2022). Fundamental physics from remote velocity and quadrupole reconstruction with the cosmic microwave background and galaxy surveys. Perimeter Institute for Theoretical Physics. https://pirsa.org/22050022

Hotinli, Selim. Fundamental physics from remote velocity and quadrupole reconstruction with the cosmic microwave background and galaxy surveys. Perimeter Institute for Theoretical Physics, May. 03, 2022, https://pirsa.org/22050022 

          @misc{ scivideos_PIRSA:22050022,
            doi = {10.48660/22050022},
            url = {https://pirsa.org/22050022},
            author = {Hotinli, Selim},
            keywords = {Cosmology},
            language = {en},
            title = {Fundamental physics from remote velocity and quadrupole reconstruction with the cosmic microwave background and galaxy surveys},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2022},
            month = {may},
            note = {PIRSA:22050022 see, \url{https://scivideos.org/index.php/pirsa/22050022}}
          }

Selim Hotinli Perimeter Institute for Theoretical Physics

Talk numberPIRSA:22050022
DOI10.48660/22050022
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Next generation cosmic microwave background (CMB) experiments and galaxy surveys will generate a wealth of new data with unprecedented precision on small scales. Correlations between CMB anisotropies and the galaxy density carry valuable cosmological information about the largest scales, creating novel opportunities for inference. It is possible to foresee a future where reconstruction of the gravitational weak-lensing potential, velocity fields and the remote quadrupole field will provide the most precise tests of fundamental physics. The use of the second-order effects in the CMB to extract this information motivate a strong push towards low noise, high resolution frontiers of the upcoming generation CMB experiments. In this talk, I will discuss the prospects to use small-scale kinetic and polarized Sunyaev Zel’dovich effects and the moving-lens effect, in cross-correlation with ongoing galaxy surveys, to extract cosmological information. 

Zoom Link: https://pitp.zoom.us/j/91455862792?pwd=M1hFRDgyOXVKU1U4Z0pLcm1wZGdRQT09