Improved Limits on Spin-Dependent WIMP-Proton Interactions from a Two Liter CF$_3$I Bubble Chamber
E. Behnke, J. Behnke, S.J. Brice, D. Broemmelsiek, J.I. Collar, P.S., Cooper, M. Crisler, C.E. Dahl, D. Fustin, J. Hall, J.H. Hinnefeld, M. Hu, I., Levine, E. Ramberg, T. Shepherd, A. Sonnenschein, M. Szydagis

TL;DR
This paper reports on a bubble chamber experiment that sets new limits on spin-dependent WIMP-proton interactions, using acoustic discrimination to reduce backgrounds and observing three candidate events consistent with neutron background.
Contribution
It introduces an effective acoustic discrimination method in a CF$_3$I bubble chamber to improve background rejection in dark matter searches.
Findings
Established the strongest direct detection limits for WIMP-proton spin-dependent scattering for WIMP masses >20 GeV/c$^{2}$
Demonstrated effective background discrimination using ultrasound signals
Observed three candidate events consistent with neutron background
Abstract
Data from the operation of a bubble chamber filled with 3.5 kg of CFI in a shallow underground site are reported. An analysis of ultrasound signals accompanying bubble nucleations confirms that alpha decays generate a significantly louder acoustic emission than single nuclear recoils, leading to an efficient background discrimination. Three dark matter candidate events were observed during an effective exposure of 28.1 kg-day, consistent with a neutron background. This observation provides the strongest direct detection constraint to date on WIMP-proton spin-dependent scattering for WIMP masses GeV/c.
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