Video URL

https://pirsa.org/11020078

Understanding Fundamental Physics with Galaxy Clusters

Sehgal, N. (2011). Understanding Fundamental Physics with Galaxy Clusters. Perimeter Institute for Theoretical Physics. https://pirsa.org/11020078

Sehgal, Neelima. Understanding Fundamental Physics with Galaxy Clusters. Perimeter Institute for Theoretical Physics, Feb. 01, 2011, https://pirsa.org/11020078 

          @misc{ scivideos_PIRSA:11020078,
            doi = {10.48660/11020078},
            url = {https://pirsa.org/11020078},
            author = {Sehgal, Neelima},
            keywords = {Cosmology},
            language = {en},
            title = {Understanding Fundamental Physics with Galaxy Clusters},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {feb},
            note = {PIRSA:11020078 see, \url{https://scivideos.org/pirsa/11020078}}
          }

Neelima Sehgal Stony Brook University

DOI 10.48660/11020078
Source Repository PIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

I will discuss a powerful way to examine the nature of dark energy using a measurement of the growth of galaxy clusters over cosmic time. A novel technique that uses the Cosmic Microwave Background as a backlight allows the detection of galaxy clusters out to the time of their first formation. Using this technique, I will present the first constraints on cosmological parameters obtained with the Atacama Cosmology Telescope, as well as exciting prospects for the future.