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Application and modeling of an online distillation method to reduce krypton and argon in XENON1T
E. Aprile, K. Abe, F. Agostini +151
A novel online distillation technique was developed for the XENON1T dark matter experiment to reduce intrinsic background components more volatile than xenon, such as krypton or ar…
Emission of Single and Few Electrons in XENON1T and Limits on Light Dark Matter
E. Aprile, K. Abe, F. Agostini +152
Delayed single- and few-electron emissions plague dual-phase time projection chambers, limiting their potential to search for light-mass dark matter. This paper examines the origin…
Material radiopurity control in the XENONnT experiment
E. Aprile, K. Abe, F. Agostini +150
The selection of low-radioactive construction materials is of the utmost importance for rare-event searches and thus critical to the XENONnT experiment. Results of an extensive rad…
The tracking detector of the FASER experiment
FASER Collaboration, Henso Abreu, Claire Antel +77
FASER is a new experiment designed to search for new light weakly-interacting long-lived particles (LLPs) and study high-energy neutrino interactions in the very forward region of…
Ultra-low jitter clock distribution for the trigger electronics of the New Small Wheel for the ATLAS experiment
T. Alexopoulos, T. Geralis, P. Gkountoumis +3
The Large Hadron Collider (LHC) at CERN plans to have a series of upgrades to increase its instantaneous luminosity to 7.5 the nominal luminosity. The increased luminosity drastica…
The trigger and data acquisition system of the FASER experiment
FASER Collaboration, Henso Abreu, Elham Amin Mansour +81
The FASER experiment is a new small and inexpensive experiment that is placed 480 meters downstream of the ATLAS experiment at the CERN LHC. FASER is designed to capture decays of…
First neutrino interaction candidates at the LHC
FASER Collaboration, Henso Abreu, Yoav Afik +73
FASER at the CERN Large Hadron Collider (LHC) is designed to directly detect collider neutrinos for the first time and study their cross sections at TeV energies, where no such…