PIRSA:11090091

Constraints on Dark Matter Models from a Fermi-LAT Search for Cosmic-Ray Electrons from the Sun

APA

Siegal-Gaskins, J. (2011). Constraints on Dark Matter Models from a Fermi-LAT Search for Cosmic-Ray Electrons from the Sun. Perimeter Institute. https://pirsa.org/11090091

MLA

Siegal-Gaskins, Jennifer. Constraints on Dark Matter Models from a Fermi-LAT Search for Cosmic-Ray Electrons from the Sun. Perimeter Institute, Sep. 22, 2011, https://pirsa.org/11090091

BibTex

          @misc{ pirsa_PIRSA:11090091,
            doi = {10.48660/11090091},
            url = {https://pirsa.org/11090091},
            author = {Siegal-Gaskins, Jennifer},
            keywords = {Particle Physics},
            language = {en},
            title = {Constraints on Dark Matter Models from a Fermi-LAT Search for Cosmic-Ray Electrons from the Sun},
            publisher = {Perimeter Institute},
            year = {2011},
            month = {sep},
            note = {PIRSA:11090091 see, \url{https://pirsa.org}}
          }
          

Jennifer Siegal-Gaskins Ohio State University

Abstract

No known astrophysical mechanisms are expected to generate a significant high-energy flux of cosmic-ray electrons and positrons (CREs) from the Sun. However, some recently considered classes of dark matter models predict such a signal. We analyzed the CRE events collected by the Fermi-LAT during its first year of operation to search for a flux excess correlated with the Sun's direction, and found no evidence of a significant signal. I will discuss the constraints these results place on secluded dark matter models and inelastic dark matter models.