ZEPLIN‐II limits on WIMP‐nucelon interactions

Alner, G. J.; Araújo, H. M.; Bewick, A.; Bungau, C.; Camanzi, B.; Carson, M. J.; Cashmore, R. J.; Chagani, H.; Chepel, V.; Cline, D.; Davidge, D.; Davies, J. C.; Daw, E.; Dawson, J.; Durkin, T.; Edwards, B.; Gamble, T.; Gao, J.; Ghag, C.; Howard, A. S.; Jones, W. G.; Joshi, M.; Kudryavtsev, V. A.; Lawson, T.; Lebedenko, V. N.; Lewin, J. D.; Lightfoot, P.; Lindote, A.; Liubarsky, I.; Lopes, M. I.; Lüscher, R.; Majewski, P.; Mavrokoridis, K.; McMillan, J. E.; Morgan, B.; Muna, D.; Murphy, A. St. J.; Neves, F.; Nicklin, G. G.; Ooi, W.; Paling, S. M.; da Cunha, J. Pinto; Plank, S. J. S.; Preece, R. M.; Quenby, J. J.; Robinson, M.; Sergiampietri, F.; Silva, C.; Solovov, V. N.; Smith, N. J. T.; Smith, P. F.; Spooner, N. J. C.; Sumner, T. J.; Thorne, C.; Tovey, D. R.; Tziaferi, E.; Walkeer, R. J.; Wang, H.; White, J.; Wolfs, F. L. H.

doi:doi:10.1063/1.3232184

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ZEPLIN‐II limits on WIMP‐nucelon interactions

AIP Conf. Proc. 1166, pp. 218-223; doi:http://dx.doi.org/10.1063/1.3232184 (6 pages)

SOURCES AND DETECTION OF DARK MATTER AND DARK ENERGY IN THE UNIVERSE: Proceedings of the 8th UCLA Symposium

Date: 20–22 February 2008

Location: Marina del Rey (California)

G. J. Alner¹, H. M. Araújo^2,1, A. Bewick², C. Bungau¹, B. Camanzi¹, M. J. Carson³, R. J. Cashmore⁴, H. Chagani⁵, V. Chepel³, D. Cline⁶, D. Davidge², J. C. Davies³, E. Daw³, J. Dawson², T. Durkin¹, B. Edwards¹, T. Gamble³, J. Gao⁷, C. Ghag⁸, A. S. Howard², W. G. Jones², M. Joshi², V. A. Kudryavtsev³, T. Lawson³, V. N. Lebedenko², J. D. Lewin¹, P. Lightfoot³, A. Lindote⁵, I. Liubarsky², M. I. Lopes², R. Lüscher¹, P. Majewski³, K. Mavrokoridis³, J. E. McMillan³, B. Morgan³, D. Muna³, A. St. J. Murphy⁹, F. Neves⁵, G. G. Nicklin³, W. Ooi⁶, S. M. Paling³, J. Pinto da Cunha⁵, S. J. S. Plank⁹, R. M. Preece¹, J. J. Quenby², M. Robinson³, F. Sergiampietri⁶, C. Silva⁵, V. N. Solovov⁵, N. J. T. Smith¹, P. F. Smith¹, N. J. C. Spooner, T. J. Sumner¹, C. Thorne¹, D. R. Tovey³, E. Tziaferi³, R. J. Walkeer², H. Wang⁶, J. White⁷, and F. L. H. Wolfs⁸

¹Particle Physics Dept., CCLRC Rutherford Appleton Laboratory, UK
²Blackett Laboratory, Imperial College London, UK
³Department of Physics & Astronomy, University of Sheffield, UK
⁴Brasenose College and Department of Physics, University of Oxford, UK
⁵LIP‐Coimbra & Department of Physics of the University of Coimbra, Portugal
⁶Department of Physics & Astronomy, University of California, Los Angeles, USA
⁷Department of Physics, Texas A&M University, USA
⁸Department of Physics and Astronomy, University of Rochester, New York, USA
⁹School of Physics, University of Edinburgh, UK

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Abstract

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ZEPLIN II is a two‐phase xenon detector designed to detect dark matter in the form of Weakly Interacting Massive Particles (WIMPs). Following the first 31‐day underground run in Boulby Mine, UK, the collaboration published dark matter limits in January 2007; the first such limits using two‐phase xenon technology. We outline the key detector design, performance and results here.