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Reply to: “Critical revision of the ZEPLIN-I sensitivity to WIMP interactions”
Abstract
Recent objections [A. Benoit et al., Phys. Lett. B 637 (2006) 156] to the published ZEPLIN I limit [G.J. Alner et al., Astropart. Phys. 23 (2005) 444] are shown to arise from misunderstandings of the calibration data and procedure, and a misreading of the data in one of the referenced papers.
- Astrophysics
ZEPLIN-I: A Single Phase Liquid Xe Detector for Dark Matter Search
Abstract
Zeplin Station
The UK Dark Matter Collaboration is developing a series of liquid <roman>Xe</roman> detectors to search for the hypothetical weakly interacting massive particles (WIMPs) which may comprise a significant component of the Galactic dark matter. These detectors will be operated at a depth of 1100 m in the Boulby salt mine. The first of these detectors, ZEPLIN-I is a 1.7 litre single phase liquid <roman>Xe</roman> scintillation detector which employs pulse shape discrimination analysis to distinguish nuclear recoils due to WIMPs from electron recoils from background gamma interactions. The current status of ZEPLIN-I is presented in this paper. The detector design will be described and results discussed of tests on the detector performance using various types of radioactive sources in the 10 keV-1MeV energy range. The light yield at the level of 1 photoelectron per 1 keV of deposited energy has been achieved. Clear discrimination between gamma initiated electron recoils and neutron initiated nuclear recoils has been observed. We are going to use this fact to recognize the type of interacting particle once the detector is installed undeground in the Boulby mine.
Zepelini
- Publication:
- Pub Date:
- 2001
- DOI:
- 10.1142/9789812811363_0055
- Bibcode:
- 2001idm..conf..433I