2016
DOI: 10.1103/physrevd.93.052014
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Dark matter search results from the PICO-60CF3Ibubble chamber

Abstract: New data are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 36.8 kg of CF3I and located in the SNOLAB underground laboratory. PICO-60 is the largest bubble chamber to search for dark matter to date. With an analyzed exposure of 92.8 live-days, PICO-60 exhibits the same excellent background rejection observed in smaller bubble chambers. Alpha decays in PICO-60 exhibit frequency-dependent acoustic calorimetry, similar but not identical to that reported recently in a… Show more

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Cited by 153 publications
(180 citation statements)
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“…Comparison of our limits with the latest constraints from Super-Kamiokande [2] and PICO [32,33]. Depending on the annihilation channel, IceCube provides the strongest limits above WIMP masses of ∼100-200 GeV.…”
Section: Improved Limits On Wimp Dark Mattermentioning
confidence: 79%
“…Comparison of our limits with the latest constraints from Super-Kamiokande [2] and PICO [32,33]. Depending on the annihilation channel, IceCube provides the strongest limits above WIMP masses of ∼100-200 GeV.…”
Section: Improved Limits On Wimp Dark Mattermentioning
confidence: 79%
“…We take the efficiency function for PICO-60 from Ref. [39] and consider only the contribution to the event rate from scattering events with recoil energies E R < 100 keV at this detector.…”
Section: Direct-detection Constraintsmentioning
confidence: 99%
“…This gives rise to a conservative estimate R < 2 × 10 −6 events kg −1 day −1 for the limit on the scattering rate. For the latter detector, we assume a sensitivity equivalent to that of PICO-500 [41], which translates into a limit R < 3 × 10 −5 events kg −1 day −1 on the scattering rate, and an efficiency function identical to the efficiency function for PICO-60 [39].…”
Section: Direct-detection Constraintsmentioning
confidence: 99%
“…Fig. B.13 shows the AV and V limits translated into the SD and SI planes, respectively, and compared to DD and ID experiments [307,308,309,310,311,312,313,314].…”
Section: B4 Model-dependent Interpretationmentioning
confidence: 99%
“…The CMS SI exclusion contour is compared with the LUX [307], PandaX-II [308], CDMSLite [309], and CRESST-II [310] limits, which have documented the most constraining results in the shown mass range. The SD exclusion contour is compared with limits from the PICO experiments [311,312], the IceCube limit for the tt annihilation channel [313] and the Super-Kamiokande limit for the bb annihilation channel [314]. …”
mentioning
confidence: 99%