Cosmological and astrophysical observations indicate the presence of Dark Matter in the universe which cannot be explained by the Standard Model. Searches for Dark Matter are performed by both the ATLAS and CMS experiment at the LHC in events involving large missing transverse momentum in the final state. So far no signal for physics beyond the Standard Model has been found. An overview of the most recent results by both the ATLAS and CMS collaboration based on the full proton-proton collision dataset collected at a centreof-mass energy of 13 TeV in 2015 and 2016 is presented.Cosmological and astrophysical observations indicate the presence of Dark Matter in the universe which cannot be explained by the Standard Model. Searches for Dark Mat...
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 (DM) component in the Universe is inferred from the obser...
The CMS and ATLAS collaborations searched for Dark Matter (DM) particles directly produced in pair. ...
Signatures of large missing transverse momentum recoiling against jets, photons, heavy-flavor quarks...
Evidence of the existence of dark matter is provided by astrophysicalobservations, but its nature or...
Although the existence of Dark Matter (DM) is well established by many astronomical measurements, it...
Dark Matter constitutes more than 80% of the matter in the universe but cannot be accommodated withi...
Astrophysical observations suggest the existence of Dark Matter to explain the composition and evolu...
While it is known that about 85% of the matter in the universe is in the form of Dark Matter (DM), l...
Astrophysical measurements show that around 85\% of the universe consists of dark matter, the origin...
Dark Matter can be produced in large amounts in pp collisions at the Large Hadron Collider (LHC) ass...
Dark Matter comprises approximately 27% of the universe yet little is known about its properties. Da...
Although the existence of Dark Matter is a well-established hypothesis to explain a range of astroph...
Cosmological and astrophysical observations strongly support the presence of a non-baryonic dark mat...
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 (DM) component in the Universe is inferred from the obser...
The CMS and ATLAS collaborations searched for Dark Matter (DM) particles directly produced in pair. ...
Signatures of large missing transverse momentum recoiling against jets, photons, heavy-flavor quarks...
Evidence of the existence of dark matter is provided by astrophysicalobservations, but its nature or...
Although the existence of Dark Matter (DM) is well established by many astronomical measurements, it...
Dark Matter constitutes more than 80% of the matter in the universe but cannot be accommodated withi...
Astrophysical observations suggest the existence of Dark Matter to explain the composition and evolu...
While it is known that about 85% of the matter in the universe is in the form of Dark Matter (DM), l...
Astrophysical measurements show that around 85\% of the universe consists of dark matter, the origin...
Dark Matter can be produced in large amounts in pp collisions at the Large Hadron Collider (LHC) ass...
Dark Matter comprises approximately 27% of the universe yet little is known about its properties. Da...
Although the existence of Dark Matter is a well-established hypothesis to explain a range of astroph...
Cosmological and astrophysical observations strongly support the presence of a non-baryonic dark mat...
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 (DM) component in the Universe is inferred from the obser...