Mapping dark matter on the largest and smallest scales
APA
Holder, G. (2016). Mapping dark matter on the largest and smallest scales. Perimeter Institute. https://pirsa.org/16060023
MLA
Holder, Gilbert. Mapping dark matter on the largest and smallest scales. Perimeter Institute, Jun. 16, 2016, https://pirsa.org/16060023
BibTex
@misc{ pirsa_PIRSA:16060023, doi = {10.48660/16060023}, url = {https://pirsa.org/16060023}, author = {Holder, Gilbert}, keywords = {Cosmology}, language = {en}, title = {Mapping dark matter on the largest and smallest scales}, publisher = {Perimeter Institute}, year = {2016}, month = {jun}, note = {PIRSA:16060023 see, \url{https://pirsa.org}} }
University of Illinois Urbana-Champaign
Talk Type
Subject
Abstract
Using lensing of the CMB we can make maps of the dark matter distribution on the largest cosmological scales, perhaps allowing new insights into gravity, particle physics, and cosmology. With high-resolution maps of distant star-forming galaxies we can map dark matter on small scales within individual galaxies, measuring the small-scale clumping properties of dark matter.