Although the existence of Dark Matter is a well-established hypothesis to explain a range of astrophysical and cosmological measurements, its nature and particle properties still remain one of the greatest unsolved puzzles of particle and astro-particle physics. The collider experiments have developed a comprehensive search program in this sector looking at a wide spectrum of channels in which a Dark Matter evidence can be traced. In this context the last results using the data sample collected at LHC at the new centre-of-mass energy of 13 TeV will be presented giving an outlook of the Dark Matter search status in the ATLAS experiment
The presence of a non-baryonic dark matter (DM) component in the Universe is inferred from the obser...
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 astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
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...
The presence of a non-baryonic dark matter (DM) component in the Universe is inferred from the obser...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
Although the existence of Dark Matter (DM) is well established by many astronomical measurements, it...
The presence of a non-baryonic dark matter (DM) component in the Universe is inferred from the obser...
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 astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
The astrophysical evidence of dark matter provides some of the most compelling clues to the nature o...
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...
The presence of a non-baryonic dark matter (DM) component in the Universe is inferred from the obser...
The presence of a non-baryonic dark matter component in the Universe is inferred from the observatio...
Although the existence of Dark Matter (DM) is well established by many astronomical measurements, it...
The presence of a non-baryonic dark matter (DM) component in the Universe is inferred from the obser...
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...