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The LHC Dark Matter Working Group (LHC DM WG) brings together theorists and experimentalists to define guidelines and recommendations for the benchmark models, interpretation, and characterisation necessary for broad and systematic searches for dark matter at the LHC. As examples, the group develops and promotes well-defined signal models, specifying the assumptions behind them and describing the conditions under which they should be used. It works to improve the set of tools available to the experiments, such as higher- precision calculations of the backgrounds. It assists theorists with understanding and making use of LHC results.
The LHC DM WG develops and maintains close connections with theorists and other experimental particle DM searches (e.g. Direct and Indirect Detection experiments) in order help verify and constrain particle physics models of astrophysical excesses, to understand how collider searches and non-collider experiments complement one another, and to help build a comprehensive understanding of viable dark matter models.
The WG activity builds on the experience of the previous ATLAS-CMS Dark Matter Forum, whose findings are documented in this paper
WG documents and meeting agendas: see links in the right menu
Topics currently under discussion:
- Recommendations for simple models featuring t-channel production of dark matter
- Connecting dark boson models to cosmological observables
- Theoretical issues for single top simplified models
- ATLAS: Oleg Brandt and Christian Ohm (past: Caterina Doglioni, Antonio Boveia)
- CMS: Phil Harris (past: Sarah Malik, Steve Mrenna (Dark Matter Forum), Oliver Buchmueller, Steven Lowette)
- LHCb: Xabier Cid Vidal
- Theory: Uli Haisch and Tim Tait
- LPCC: Michelangelo Mangano
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