Speaker
Christopher Chang
Description
Dark matter candidates can arise from a wide range of extensions to the Standard Model. Simplified models with a small number of new particles allow for the optimisation and interpretation of dark matter and collider experiments, without the need for a UV-complete theory. In this talk, I will discuss the results from a recent GAMBIT study of global constraints on vector-mediated simplified dark matter models. I will cover several models with differing spins of the dark matter candidate. Along with these constraints, I will provide new unitarity bounds from the self-scattering of vector dark matter and discuss their effect on collider constraints.
| Collaboration name | GAMBIT |
|---|
Primary author
Co-authors
Pat Scott
(The University of Queensland)
Tomas Gonzalo
(RWTH Aachen)
Felix Kahlhoefer
(RWTH Aachen)
Martin John White
(University of Adelaide (AU))
Anders Kvellestad
(University of Oslo)
