PIRSA:09060046

Slightly nonminimal Hidden sector,Slightly nonthermal relic abundance, and Indirect Detection

APA

Nelson, A. (2009). Slightly nonminimal Hidden sector,Slightly nonthermal relic abundance, and Indirect Detection . Perimeter Institute for Theoretical Physics. https://pirsa.org/09060046

MLA

Nelson, Ann. Slightly nonminimal Hidden sector,Slightly nonthermal relic abundance, and Indirect Detection . Perimeter Institute for Theoretical Physics, Jun. 12, 2009, https://pirsa.org/09060046

BibTex

          @misc{ scivideos_PIRSA:09060046,
            doi = {10.48660/09060046},
            url = {https://pirsa.org/09060046},
            author = {Nelson, Ann},
            keywords = {Particle Physics, Cosmology},
            language = {en},
            title = {Slightly nonminimal Hidden sector,Slightly nonthermal relic abundance, and Indirect Detection },
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2009},
            month = {jun},
            note = {PIRSA:09060046 see, \url{https://scivideos.org/pirsa/09060046}}
          }
          
Talk numberPIRSA:09060046
Source RepositoryPIRSA

Abstract

I consider a the dark matter relic abundance computation in a model where the dark matter annihilates into a light mediator rather than directly into the standard model. Obtaining the correct relic abundance in such a model may imply a different annihilation cross section than is implied by the usual WIMP decoupling computation. I show that the maximum annihilation cross section is obtained when the hidden sector decouples from the standard model before the dark matter annihilates into the mediator particles, and may be as much as a factor of 5 larger than the standard WIMP value.