Video URL
https://pirsa.org/17120019Constraining a Thin Dark Matter Disk with Gaia
APA
Lin, T. (2017). Constraining a Thin Dark Matter Disk with Gaia. Perimeter Institute for Theoretical Physics. https://pirsa.org/17120019
MLA
Lin, Tongyan. Constraining a Thin Dark Matter Disk with Gaia. Perimeter Institute for Theoretical Physics, Dec. 12, 2017, https://pirsa.org/17120019
BibTex
@misc{ scivideos_PIRSA:17120019, doi = {10.48660/17120019}, url = {https://pirsa.org/17120019}, author = {Lin, Tongyan}, keywords = {Particle Physics}, language = {en}, title = {Constraining a Thin Dark Matter Disk with Gaia}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2017}, month = {dec}, note = {PIRSA:17120019 see, \url{https://scivideos.org/pirsa/17120019}} }
Tongyan Lin University of California, San Diego
Abstract
If a component of the dark matter has dissipative interactions, it could collapse to form a thin dark disk in our Galaxy coincident with the baryonic disk. It has been suggested that dark disks could explain a variety of observed phenomena, including periodic comet impacts. Using the first data release from the Gaia mission, we search for a dark disk via its effect on stellar kinematics in the Milky Way. I will present new limits on the presence of a thin dark matter disk, as well as measurements on the matter density in the solar neighborhood.