Simplified Models of Co-annihilating Dark Matter
APA
Pierce, A. (2015). Simplified Models of Co-annihilating Dark Matter. Perimeter Institute. https://pirsa.org/15090019
MLA
Pierce, Aaron. Simplified Models of Co-annihilating Dark Matter. Perimeter Institute, Sep. 15, 2015, https://pirsa.org/15090019
BibTex
@misc{ pirsa_PIRSA:15090019, doi = {10.48660/15090019}, url = {https://pirsa.org/15090019}, author = {Pierce, Aaron}, keywords = {Particle Physics}, language = {en}, title = {Simplified Models of Co-annihilating Dark Matter}, publisher = {Perimeter Institute}, year = {2015}, month = {sep}, note = {PIRSA:15090019 see, \url{https://pirsa.org}} }
The continued lack of definitive signals at direct detection experiments places many models of weakly interacting dark matter into tension. Direct detection is naturally suppressed in models where the dark matter co-annihilates with another particle in the early universe. The cosmology, direct detection, and LHC signals of such models can often be well understood by considering only the most relevant low-energy degrees of freedom. We draw lessons for the Minimal Supersymmetric Standard Model.