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A Design for an Electromagnetic Filter for Precision Energy Measurements at the Tritium Endpoint
M. G. Betti, M. Biasotti, A. Bosca +48
We present a detailed description of the electromagnetic filter for the PTOLEMY project to directly detect the Cosmic Neutrino Background (CNB). Starting with an initial estimate f…
Machine Learning Accelerated Likelihood-Free Event Reconstruction in Dark Matter Direct Detection
U. Simola, B. Pelssers, D. Barge +2
Reconstructing the position of an interaction for any dual-phase time projection chamber (TPC) with the best precision is key to directly detecting Dark Matter. Using the likelihoo…
Signal Yields of keV Electronic Recoils and Their Discrimination from Nuclear Recoils in Liquid Xenon
E. Aprile, J. Aalbers, F. Agostini +116
We report on the response of liquid xenon to low energy electronic recoils below 15 keV from beta decays of tritium at drift fields of 92 V/cm, 154 V/cm and 366 V/cm using the XENO…
The XENON1T Dark Matter Experiment
XENON Collaboration, E. Aprile, J. Aalbers +142
The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out o…
Intrinsic backgrounds from Rn and Kr in the XENON100 experiment
XENON Collaboration, E. Aprile, J. Aalbers +115
In this paper, we describe the XENON100 data analyses used to assess the target-intrinsic background sources radon (Rn), thoron (Rn) and krypton (Kr). We det…
DARWIN: towards the ultimate dark matter detector
J. Aalbers, F. Agostini, M. Alfonsi +116
DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core.…