Boosting dark matter indirect detection with black holes
APA
Shelton, J. (2015). Boosting dark matter indirect detection with black holes. Perimeter Institute. https://pirsa.org/15050031
MLA
Shelton, Jessie. Boosting dark matter indirect detection with black holes. Perimeter Institute, May. 12, 2015, https://pirsa.org/15050031
BibTex
@misc{ pirsa_PIRSA:15050031, doi = {10.48660/15050031}, url = {https://pirsa.org/15050031}, author = {Shelton, Jessie}, keywords = {Particle Physics}, language = {en}, title = {Boosting dark matter indirect detection with black holes}, publisher = {Perimeter Institute}, year = {2015}, month = {may}, note = {PIRSA:15050031 see, \url{https://pirsa.org}} }
Super-massive black holes that grow at the center of dark matter halos distort the dark matter within their zone of influence into a steep density spike. This spike can give rise to strong enhancements of standard indirect detection signals, and can lead to qualitatively new windows onto the physics of the early universe. I will talk about potential dark matter signals from the Milky Way's central black hole, some astrophysical caveats, and the possible use of black holes as dark matter accelerators.