PIRSA:17120002

Video URL

https://pirsa.org/17120002

Is Self-Interacting Dark Matter Undergoing Dark Fusion?

McDermott, S. (2017). Is Self-Interacting Dark Matter Undergoing Dark Fusion?. Perimeter Institute for Theoretical Physics. https://pirsa.org/17120002

McDermott, Samuel. Is Self-Interacting Dark Matter Undergoing Dark Fusion?. Perimeter Institute for Theoretical Physics, Dec. 01, 2017, https://pirsa.org/17120002 

          @misc{ scivideos_PIRSA:17120002,
            doi = {10.48660/17120002},
            url = {https://pirsa.org/17120002},
            author = {McDermott, Samuel},
            keywords = {Particle Physics},
            language = {en},
            title = {Is Self-Interacting Dark Matter Undergoing Dark Fusion?},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2017},
            month = {dec},
            note = {PIRSA:17120002 see, \url{https://scivideos.org/index.php/pirsa/17120002}}
          }

Samuel McDermott Fermi National Accelerator Laboratory (Fermilab)

Talk numberPIRSA:17120002
DOI10.48660/17120002
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

We suggest that two-to-two dark matter fusion may be the relaxation process that resolves the small-scale structure problems of the cold collisionless dark matter paradigm. In order for the fusion cross section to scale correctly across many decades of astrophysical masses from dwarf galaxies to galaxy clusters, we require the fractional binding energy released to be greater than v^n ~ [10^{-(2-3)}]^n, where n=1,2 depends on local dark sector chemistry. The size of the dark-sector interaction cross sections must be sigma ~ 0.1-1 barn, moderately larger than for Standard Model deuteron fusion, indicating a dark nuclear scale Lambda ~ O(100 MeV). Dark fusion firmly predicts constant sigma v below the characteristic velocities of galaxy clusters. Observations of the inner structure of galaxy groups with velocity dispersion of several hundred kilometer per second, of which a handful have been identified, could differentiate dark fusion from a dark photon model.