1993
DOI: 10.1016/0370-2693(93)91306-8
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Detection rate of weakly interacting massive particles

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Cited by 27 publications
(28 citation statements)
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“…The calculated energy thresholds for 25µm Al, 29µm Zn and 17µm Sn granules are shown in Fig.5. The recoil energies due to neutral-current scattering of dark matter are expected to be of the order of a few keV [5]. Note that such energy thresholds can be reached with the presently used superconducting granules and in principle even lower ones could be reached using smaller granules.…”
Section: Energy Thresholdmentioning
confidence: 99%
“…The calculated energy thresholds for 25µm Al, 29µm Zn and 17µm Sn granules are shown in Fig.5. The recoil energies due to neutral-current scattering of dark matter are expected to be of the order of a few keV [5]. Note that such energy thresholds can be reached with the presently used superconducting granules and in principle even lower ones could be reached using smaller granules.…”
Section: Energy Thresholdmentioning
confidence: 99%
“…Integrating over that region could hide a fluctuation that might actually be present in the data. The cross-over energy depends on the mass of the WIMP [26][27][28] and other parameters [28,29]. This experiment integrated up to a large final energy (50 keV) -consistent with the mean energy deposited by a 10 TeV WIMP-and ramped the initial energy from 12.5 to 18 keV thus ensuring sensitivity to fluctuations of WIMPs with masses up to 1 TeV [29].…”
Section: A Modulation Significancementioning
confidence: 99%
“…2 at the temperature of 40mK. The recoil energies due to neutral-current scatterings of dark matter particles in Sn detectors are expected to be of the order of a few keV [10]. Such thresholds can be reached with 17µm Sn granules at magnetic thresholds of h∼0.01.…”
Section: Recoil Energy Threshold In Ssgmentioning
confidence: 99%