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Snowmass2021 Cosmic Frontier White Paper: Calibrations and backgrounds for dark matter direct detection

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arxiv 2203.07623 v2 pith:TWZDM5LP submitted 2022-03-15 hep-ex

Daniel Baxter , Raymond Bunker , Sally Shaw , Shawn Westerdale , Isaac Arnquist , Daniel S. Akerib , Rob Calkins , Susana Cebrián
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James B. Dent Maria Laura di Vacri Jim Dobson Daniel Egana-Ugrinovic Andrew Erlandson Chamkaur Ghag Carter Hall Jeter Hall Scott Haselschwardt Eric Hoppe Chris M. Jackson Yonatan Kahn Alvine Kamaha Mike Kelsey Alexander Kish Noah Kurinsky Matthias Laubenstein Eric H. Miller Eric Morrison Brianna Mount Jayden L. Newstead Stefano Nisi Ibles Olcina John Orrell Sergey Pereverzev Emily Perry Andreas Piepke Sagar Sharma Poudel Karthik Ramanathan Juergen Reichenbacher Tarek Saab Richard Saldanha Claudio Savarese Richard Schnee Silvia Scorza Rajeev Singh Kelly Stifter Burkhant Suerfu Matthew Szydagis Dylan J. Temples Anthony Villano David Woodward Jingke Xu
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classification hep-ex
keywords backgrounddarkdetectiondirectmattercalibrationexperimentsfuture
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Future dark matter direct detection experiments will reach unprecedented levels of sensitivity. Achieving this sensitivity will require more precise models of signal and background rates in future detectors. Improving the precision of signal and background modeling goes hand-in-hand with novel calibration techniques that can probe rare processes and lower threshold detector response. The goal of this white paper is to outline community needs to meet the background and calibration requirements of next-generation dark matter direct detection experiments.

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