Dark matter composes 27% of the universe but its presence is inferred only from gravitational phenomena. Direct detection experiments, such as Xenon1T, attempt to detect the scattering of dark matter particles with the detector target, in this case xenon nuclei. The experiment Xenon1T employs 3.3 tonnes of liquid xenon in a Time Projection Chamber (TPC). The TPC is a detector that employs electromagnetic fields in a sensitive volume for 3-d position reconstruction and particle identification. Since dark matter scattering is a rare event, it is necessary to reduce the background to improve the sensitivity of the detector. It is necessary to monitor two kind of impurities in liquid xenon: radioactive impurities such as krypton (present in com...
An abundance of cosmological evidence suggests that cold dark matter exists and makes up 83% of the ...
The evidence supporting the presence of Dark Matter in the universe ranges over many length scales: ...
As liquid xenon detectors grow in scale, novel techniques are required to maintain sufficient purity...
The XENON1T experiment aims at the direct detection of the well motivated dark matter candidate of w...
The XenonnT experiment, successor of Xenon1T, aims at probing the cross sections of the interaction ...
Over much of the last century evidence has been building for a new component of our universe that in...
The XENON1T experiment is currently the most sensitive in the world for the direct search for dark m...
The XENON program consists in operating and developing double-phase time projection chambers using l...
The currently running Xenon100 experiment and its successor, Xenon1T, use liquid xenon as target and...
The XENON1T experiment is the first ton-scale dual-phase (liquidgas) xenon time projection chamber, ...
Astronomical and cosmological observations indicate that a large amount of the energy content of the...
Currently, one of the most well motivated models of dark matter is the weakly inter- acting massive ...
The XENON program is a phased project using liquid xenon as a sensitive detector medium in search fo...
The quest to directly detect dark matter, in particular weakly interactive massive particles (WIMP),...
One of the most exciting mysteries of modern physics is that of dark matter. While there is a multit...
An abundance of cosmological evidence suggests that cold dark matter exists and makes up 83% of the ...
The evidence supporting the presence of Dark Matter in the universe ranges over many length scales: ...
As liquid xenon detectors grow in scale, novel techniques are required to maintain sufficient purity...
The XENON1T experiment aims at the direct detection of the well motivated dark matter candidate of w...
The XenonnT experiment, successor of Xenon1T, aims at probing the cross sections of the interaction ...
Over much of the last century evidence has been building for a new component of our universe that in...
The XENON1T experiment is currently the most sensitive in the world for the direct search for dark m...
The XENON program consists in operating and developing double-phase time projection chambers using l...
The currently running Xenon100 experiment and its successor, Xenon1T, use liquid xenon as target and...
The XENON1T experiment is the first ton-scale dual-phase (liquidgas) xenon time projection chamber, ...
Astronomical and cosmological observations indicate that a large amount of the energy content of the...
Currently, one of the most well motivated models of dark matter is the weakly inter- acting massive ...
The XENON program is a phased project using liquid xenon as a sensitive detector medium in search fo...
The quest to directly detect dark matter, in particular weakly interactive massive particles (WIMP),...
One of the most exciting mysteries of modern physics is that of dark matter. While there is a multit...
An abundance of cosmological evidence suggests that cold dark matter exists and makes up 83% of the ...
The evidence supporting the presence of Dark Matter in the universe ranges over many length scales: ...
As liquid xenon detectors grow in scale, novel techniques are required to maintain sufficient purity...