Video URL
https://pirsa.org/17100079Hunting for WIMPs: How low should we go?
APA
Pierce, A. (2017). Hunting for WIMPs: How low should we go?. Perimeter Institute for Theoretical Physics. https://pirsa.org/17100079
MLA
Pierce, Aaron. Hunting for WIMPs: How low should we go?. Perimeter Institute for Theoretical Physics, Oct. 17, 2017, https://pirsa.org/17100079
BibTex
@misc{ scivideos_PIRSA:17100079, doi = {10.48660/17100079}, url = {https://pirsa.org/17100079}, author = {Pierce, Aaron}, keywords = {Particle Physics}, language = {en}, title = {Hunting for WIMPs: How low should we go?}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2017}, month = {oct}, note = {PIRSA:17100079 see, \url{https://scivideos.org/index.php/pirsa/17100079}} }
Aaron Pierce University of Michigan–Ann Arbor
Abstract
Direct detection experiments are rapidly improving their sensitivity to weak scale Dark Matter. A particular interesting (and minimal) possibility is that the Dark matter interacts with ordinary matter via the exchange of weak bosons: the W, Z, and Higgs. Dark matter with substantial coupling to the Higgs boson is already under significant tension from limits on spin-independent scattering. We comment on the power of spin-dependent scattering as a probe of Z-mediated dark matter, both in a simple effective theory, and in the so-called Singlet-Doublet Model, which we argue is a useful benchmark. We also review the case where the cosmology of the WIMP is dominated by co-annihilation processes, focusing on the stop co-annihilation region of the Minimal Supersymmetric Standard Model, and discuss prospects for direct detection in this case.