Abstract

Leptonic signatures of Dark Matter (DM) are one of the cleanest ways to discover such a secluded form of matter at high energy colliders. We explore the full parameter space relevant to multi-lepton (2- and 3-lepton) signatures at the Large Hadron Collider (LHC) from representative minimal consistent models with scalar and fermion DM. In our analysis, we suggest a new parametrisation of the model parameter spaces in terms of the DM mass and mass differences between DM and its multiplet partners. This parametrisation allows us to explore properties of DM models in their whole parameter space. This approach is generic and quite model-independent since the mass differences are related to the couplings of the DM to the Standard Model (SM) sector. We establish the most up-to-date LHC limits on the inert 2-Higgs Doublet Model (i2HDM) and Minimal Fermion DM (MFDM) model parameter spaces, by using the complementary information stemming from 2- and 3-lepton signatures. We provide a map of LHC efficiencies and cross-section limits for such 2- and 3-lepton signatures allowing one to easily make model-independent reinterpretations of LHC results for analogous classes of models. We also present combined constraints from the LHC, DM relic density and direct search experiments indicating the current status of the i2HDM and MFDM model.

Details

Title
Multilepton signatures from dark matter at the LHC
Author
Belyaev, Alexander 1   VIAFID ORCID Logo  ; Blumenschein, Ulla 2 ; Freegard, Arran 3 ; Moretti, Stefano 4 ; Sengupta, Dipan 5   VIAFID ORCID Logo 

 University of Southampton, School of Physics and Astronomy, Southampton, United Kingdom (GRID:grid.5491.9) (ISNI:0000 0004 1936 9297); Rutherford Appleton Laboratory, Particle Physics Department, Didcot, United Kingdom (GRID:grid.76978.37) (ISNI:0000 0001 2296 6998) 
 Queen Mary University of London, Particle Physics Research Centre, School of Physical and Chemical Sciences, London, United Kingdom (GRID:grid.4868.2) (ISNI:0000 0001 2171 1133) 
 University of Southampton, School of Physics and Astronomy, Southampton, United Kingdom (GRID:grid.5491.9) (ISNI:0000 0004 1936 9297); Queen Mary University of London, Particle Physics Research Centre, School of Physical and Chemical Sciences, London, United Kingdom (GRID:grid.4868.2) (ISNI:0000 0001 2171 1133) 
 University of Southampton, School of Physics and Astronomy, Southampton, United Kingdom (GRID:grid.5491.9) (ISNI:0000 0004 1936 9297); Rutherford Appleton Laboratory, Particle Physics Department, Didcot, United Kingdom (GRID:grid.76978.37) (ISNI:0000 0001 2296 6998); Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden (GRID:grid.8993.b) (ISNI:0000 0004 1936 9457) 
 University of California, San Diego, Department of Physics and Astronomy, La Jolla, United States of America (GRID:grid.266100.3) (ISNI:0000 0001 2107 4242); University of Adelaide, ARC Centre of Excellence for Dark Matter Particle Physics, Department of Physics, Adelaide, Australia (GRID:grid.1010.0) (ISNI:0000 0004 1936 7304) 
Pages
173
Publication year
2022
Publication date
Sep 2022
Publisher
Springer Nature B.V.
e-ISSN
10298479
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2757875762
Copyright
© The Author(s) 2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.