The Self-Interacting Dark Matter Paradigm
APA
Yu, H. (2016). The Self-Interacting Dark Matter Paradigm . Perimeter Institute. https://pirsa.org/16040058
MLA
Yu, Haibo. The Self-Interacting Dark Matter Paradigm . Perimeter Institute, Apr. 26, 2016, https://pirsa.org/16040058
BibTex
@misc{ pirsa_PIRSA:16040058, doi = {10.48660/16040058}, url = {https://pirsa.org/16040058}, author = {Yu, Haibo}, keywords = {Particle Physics}, language = {en}, title = {The Self-Interacting Dark Matter Paradigm }, publisher = {Perimeter Institute}, year = {2016}, month = {apr}, note = {PIRSA:16040058 see, \url{https://pirsa.org}} }
Astrophysical observations spanning dwarf galaxies to galaxy clusters indicate that dark matter halos are less dense in their central regions compared to expectations from collisionless dark matter N-body simulations. Using detailed fits to dark matter halos of galaxies and clusters, we show that self-interacting dark matter may provide a consistent solution to the dark matter deficit problem across all scales, even though individual systems exhibit a wide diversity in halo properties.