Video URL

https://pirsa.org/11090092

Substructure, Sommerfeld, and CR Signals

Slatyer, T. (2011). Substructure, Sommerfeld, and CR Signals. Perimeter Institute for Theoretical Physics. https://pirsa.org/11090092

Slatyer, Tracy. Substructure, Sommerfeld, and CR Signals. Perimeter Institute for Theoretical Physics, Sep. 22, 2011, https://pirsa.org/11090092 

          @misc{ scivideos_PIRSA:11090092,
            doi = {10.48660/11090092},
            url = {https://pirsa.org/11090092},
            author = {Slatyer, Tracy},
            keywords = {Particle Physics},
            language = {en},
            title = {Substructure, Sommerfeld, and CR Signals},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {sep},
            note = {PIRSA:11090092 see, \url{https://scivideos.org/index.php/pirsa/11090092}}
          }

Tracy Slatyer Massachusetts Institute of Technology (MIT) - Department of Physics

DOI 10.48660/11090092
Source Repository PIRSA
Collection
Talk Type Conference
Subject

Abstract

Models of dark matter with Sommerfeld-enhanced annihilation have been proposed to explain the CR excess observed by the PAMELA and Fermi experiments. In such models, the local annihilation signal can easily be dominated by small, dense, cold subhalos, instead of by the smooth DM halo as usually assumed. I will discuss how such a "substructure+Sommerfeld" scenario modifies constraints from the CMB, limits on DM self-interaction, and bounds from measurements of inner-Galaxy gamma rays and the extragalactic diffuse background. These constraints provide stringent limits on the usual smooth-halo scenario, robustly ruling out force carrier masses below ~200 MeV (in the context of explaining the PAMELA/Fermi signals) and causing tension for higher mediator masses, but in the presence of a modest amount of local substructure, force carrier masses down to 20 MeV or even lower can still be consistent with these bounds.