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First limits on WIMP nuclear recoil signals in ZEPLIN-II: A two-phase xenon detector for dark matter detection by G.J. Alner; H.M. Araújo; A. Bewick; C. Bungau; B. Camanzi; M.J. Carson; R.J. Cashmore; H. Chagani; V. Chepel; D. Cline; D. Davidge; J.C. Davies; E. Daw; J. Dawson; T. Durkin; B. Edwards; T. Gamble; J. Gao; C. Ghag; A.S. Howard; W.G. Jones; M. Joshi; E.V. Korolkova; V.A. Kudryavtsev; T. Lawson; V.N. Lebedenko; J.D. Lewin; P. Lightfoot; A. Lindote; I. Liubarsky; M.I. Lopes; R. Lüscher; P. Majewski; K. Mavrokoridis; J.E. McMillan; B. Morgan; D. Muna; A.St.J. Murphy; F. Neves; G.G. Nicklin; W. Ooi; S.M. Paling; J. Pinto da Cunha; S.J.S. Plank; R.M. Preece; J.J. Quenby; M. Robinson; G. Salinas; F. Sergiampietri; C. Silva; V.N. Solovov; N.J.T. Smith; P.F. Smith; N.J.C. Spooner; T.J. Sumner; C. Thorne; D.R. Tovey; E. Tziaferi; R.J. Walker; H. Wang; J.T. White; F.L.H. Wolfs is a Physics and Astronomy article available to read on EtoBox.

What is First limits on WIMP nuclear recoil signals in ZEPLIN-II: A two-phase xenon detector for dark matter detection about?

Results are presented from the first underground data run of ZEPLIN-II, a 31 kg two-phase xenon detector developed to observe nuclear recoils from hypothetical weakly interacting massive dark matter particles. Discrimination between nuclear recoils and background electron recoils is afforded by recording both the scintillation and ionisation signals generated within the liquid xenon, with the ratio of these signals being different for the two classes of event. This ratio is calibrated for different incident species using an AmBe neutron source and 60 Co c-ray sources. From our first 31 live days of running ZEPLIN-II, the total exposure following the application of fiducial and stability cuts was 225 kg • days. A background population of radon progeny events was observed in this run, arising from radon emission in the gas purification getters, due to radon daughter ion decays on the surfaces of the walls of the chamber. An acceptance window, defined by the neutron calibration data, of 50% nuclear recoil acceptance between 5 keV ee and 20 keV ee , had an observed count of 29 events, with a summed expectation of 28.6 ± 4.3 c-ray and radon progeny induced background events. These figur

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Author
G.J. Alner; H.M. Araújo; A. Bewick; C. Bungau; B. Camanzi; M.J. Carson; R.J. Cashmore; H. Chagani; V. Chepel; D. Cline; D. Davidge; J.C. Davies; E. Daw; J. Dawson; T. Durkin; B. Edwards; T. Gamble; J. Gao; C. Ghag; A.S. Howard; W.G. Jones; M. Joshi; E.V. Korolkova; V.A. Kudryavtsev; T. Lawson; V.N. Lebedenko; J.D. Lewin; P. Lightfoot; A. Lindote; I. Liubarsky; M.I. Lopes; R. Lüscher; P. Majewski; K. Mavrokoridis; J.E. McMillan; B. Morgan; D. Muna; A.St.J. Murphy; F. Neves; G.G. Nicklin; W. Ooi; S.M. Paling; J. Pinto da Cunha; S.J.S. Plank; R.M. Preece; J.J. Quenby; M. Robinson; G. Salinas; F. Sergiampietri; C. Silva; V.N. Solovov; N.J.T. Smith; P.F. Smith; N.J.C. Spooner; T.J. Sumner; C. Thorne; D.R. Tovey; E. Tziaferi; R.J. Walker; H. Wang; J.T. White; F.L.H. Wolfs
Publisher
Elsevier Science; Elsevier ; Elsevier BV (ISSN 0927-6505)
Published
2007
Language
EN
Field
Physics and Astronomy (Physical Sciences)

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