The astrophysical evidence of dark matter provides some of the most compelling clues to the nature of physics beyond the Standard Model. From these clues, ATLAS has developed a broad and systematic search program for dark matter production in LHC collisions. In the framework of Simplified models the searches are divided into invisible and visible channels, corresponding to dark matter searches, with a missing energy signature, and dark matter mediator searches, looking for bump in invariant mass distributions
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...
The astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
Compelling astrophysical evidence for dark matter makes it important and interesting to look for sig...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
Cosmological and astrophysical observations strongly support the presence of a non-baryonic dark mat...
The astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...
The astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
Compelling astrophysical evidence for dark matter makes it important and interesting to look for sig...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
Cosmological and astrophysical observations strongly support the presence of a non-baryonic dark mat...
The astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...
Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. The search ...