Reducing DRIFT Backgrounds with a Submicron Aluminized-Mylar Cathode
James B.R. Battat, Ed Daw, Alexei Dorofeev, Anthony C. Ezeribe,, Jennifer R. Fox, Jean-Luc Gauvreau, Michael Gold, Lydia Harmon, John Harton,, Randy Lafler, Robert J. Lauer, Eric R. Lee, Dinesh Loomba, Alexander Lumnah,, John Matthews, Eric H. Miller, Frederic Mouton

TL;DR
This paper demonstrates that using a submicron aluminized-mylar cathode significantly reduces background events caused by alpha decays in the DRIFT-IId dark matter detector, enabling near-background-free operation.
Contribution
The study introduces a new thin-film aluminized-mylar cathode that drastically lowers alpha-induced backgrounds, improving dark matter detection sensitivity.
Findings
Background rate reduced from 500/day to 1/day.
Cathode contamination measured at 3.3 ppt U-234 and 73 ppb U-238.
Alpha decay suppression factor of 70 compared to previous cathodes.
Abstract
Background events in the DRIFT-IId dark matter detector, mimicking potential WIMP signals, are predominantly caused by alpha decays on the central cathode in which the alpha particle is completely or partially absorbed by the cathode material. We installed a 0.9 micron thick aluminized-mylar cathode as a way to reduce the probability of producing these backgrounds. We study three generations of cathode (wire, thin-film, and radiologically clean thin-film) with a focus on the ratio of background events to alpha decays. Two independent methods of measuring the absolute alpha decay rate are used to ensure an accurate result, and agree to within . Using alpha range spectroscopy, we measure the radiologically cleanest cathode version to have a contamination of ppt U and ppb U. This cathode reduces the probability of producing an RPR from an alpha…
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