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Dark Matter Search Results from the PICO-2L C3F8 Bubble Chamber
Journal article   Open access   Peer reviewed

Dark Matter Search Results from the PICO-2L C3F8 Bubble Chamber

C Amole, M Ardid, D M Asner, D Baxter, E Behnke, P Bhattacharjee, H Borsodi, M Bou-Cabo, S J Brice, D Broemmelsiek, …
Physical review letters, v 114(23), pp 231302-231302
12 Jun 2015
PMID: 26196790
url
https://doi.org/10.1103/physrevlett.114.231302View
Accepted (AM)Open Access (Publisher-Specific) Open
url
https://doi.org/10.1103/PhysRevLett.114.231302View
Published, Version of Record (VoR) Open

Abstract

Acoustics - instrumentation Algorithms Fluorocarbons - chemistry Models, Theoretical Neutrons
New data are reported from the operation of a 2 liter C3F8 bubble chamber in the SNOLAB underground laboratory, with a total exposure of 211.5 kg days at four different energy thresholds below 10 keV. These data show that C3F8 provides excellent electron-recoil and alpha rejection capabilities at very low thresholds. The chamber exhibits an electron-recoil sensitivity of <3.5×10(-10) and an alpha rejection factor of >98.2%. These data also include the first observation of a dependence of acoustic signal on alpha energy. Twelve single nuclear recoil event candidates were observed during the run. The candidate events exhibit timing characteristics that are not consistent with the hypothesis of a uniform time distribution, and no evidence for a dark matter signal is claimed. These data provide the most sensitive direct detection constraints on WIMP-proton spin-dependent scattering to date, with significant sensitivity at low WIMP masses for spin-independent WIMP-nucleon scattering.

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Domestic collaboration
International collaboration
Web of Science research areas
Physics, Multidisciplinary
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