The Self-Interacting Dark Matter Paradigm

APA

Yu, H. (2016). The Self-Interacting Dark Matter Paradigm . Perimeter Institute for Theoretical Physics. https://pirsa.org/16040058

MLA

Yu, Haibo. The Self-Interacting Dark Matter Paradigm . Perimeter Institute for Theoretical Physics, Apr. 26, 2016, https://pirsa.org/16040058

BibTex

          @misc{ scivideos_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 for Theoretical Physics},
            year = {2016},
            month = {apr},
            note = {PIRSA:16040058 see, \url{https://scivideos.org/pirsa/16040058}}
          }
          

Haibo Yu University of California, Riverside

Source Repository PIRSA
Collection

Abstract

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.