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}} }
Ohio State University
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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.