Understanding Fundamental Physics with Galaxy Clusters
APA
Sehgal, N. (2011). Understanding Fundamental Physics with Galaxy Clusters. Perimeter Institute. https://pirsa.org/11020078
MLA
Sehgal, Neelima. Understanding Fundamental Physics with Galaxy Clusters. Perimeter Institute, Feb. 01, 2011, https://pirsa.org/11020078
BibTex
@misc{ pirsa_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}, year = {2011}, month = {feb}, note = {PIRSA:11020078 see, \url{https://pirsa.org}} }
Stony Brook University
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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.