H. Chagani
University of Sheffield
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Featured researches published by H. Chagani.
Astroparticle Physics | 2007
D. Yu. Akimov; G. J. Alner; H.M. Araújo; A. Bewick; C. Bungau; A. A. Burenkov; M.J. Carson; H. Chagani; V. Chepel; D. Cline; D. Davidge; E. Daw; J. Dawson; T. Durkin; B. Edwards; T. Gamble; C. Chag; R. Hollingworth; A.S. Howard; W.G. Jones; M. Joshi; K. Mavrokoridis; E.V. Korolkova; A. G. Kovalenko; V.A. Kudryavtsev; I. S. Kuznetsov; T.B. Lawson; V. N. Lebedenko; J.D. Lewin; P. K. Lightfoot
We present details of the technical design, manufacture and testing of the ZEPLIN-III dark matter experiment. ZEPLIN-III is a two-phase xenon detector which measures both the scintillation light and the ionisation charge generated in the liquid by interacting particles and radiation. The instrument design is driven by both the physics requirements and by the technology requirements surrounding the use of liquid xenon. These include considerations of key performance parameters, such as the efficiency of scintillation light collection, restrictions placed on the use of materials to control the inherent radioactivity levels, attainment of high vacuum levels and chemical contamination control. The successful solution has involved a number of novel design and manufacturing features which will be of specific use to future generations of direct dark matter search experiments as they struggle with similar and progressively more demanding requirements.
Astroparticle Physics | 2006
H.M. Araújo; D. Yu. Akimov; G. J. Alner; A. Bewick; C. Bungau; B. Camanzi; M.J. Carson; V. Chepel; H. Chagani; D. Davidge; J.C. Davies; E. Daw; J. Dawson; T. Durkin; B. Edwards; T. Gamble; C. Ghag; R. Hollingworth; A.S. Howard; W.G. Jones; M. Joshi; J. Kirkpatrick; A. G. Kovalenko; V.A. Kudryavtsev; V. N. Lebedenko; T.B. Lawson; J.D. Lewin; P. K. Lightfoot; A. Lindote; I. Liubarsky
We present results from a GEANT4-based Monte Carlo tool for end-to-end simulations of the ZEPLIN-III dark matter experiment. ZEPLIN-III is a two-phase detector which measures both the scintillation light and the ionisation charge generated in liquid xenon by interacting particles and radiation. The software models the instrument response to radioactive backgrounds and calibration sources, including the generation, ray-tracing and detection of the primary and secondary scintillations in liquid and gaseous xenon, and subsequent processing by data acquisition electronics. A flexible user interface allows easy modification of detector parameters at run time. Realistic datasets can be produced to help with data analysis, an example of which is the position reconstruction algorithm developed from simulated data. We present a range of simulation results confirming the original design sensitivity of a few times 10−8 pb to the WIMP-nucleon cross-section.
Journal of Instrumentation | 2008
H. Chagani; P. Majewski; E. Daw; V.A. Kudryavtsev; N.J.C. Spooner
Measurements of the quenching factor for sodium recoils in a 5 cm diameter NaI(Tl) crystal at room temperature have been made at a dedicated neutron facility at the University of Sheffield. The crystal has been exposed to 2.45 MeV mono-energetic neutrons generated by a Sodern GENIE 16 neutron generator, yielding nuclear recoils of energies between 10 and 100 keVnr. A cylindrical BC501A detector has been used to tag neutrons that scatter off sodium nuclei in the crystal. Cuts on pulse shape and time of flight have been performed on pulses recorded by an Acqiris DC265 digitiser with a 2 ns sampling time. Measured quenching factors of Na nuclei range from 19% to 26% in good agreement with other experiments, and a value of 25.2±6.4% has been determined for 10 keV sodium recoils. From pulse shape analysis, the mean times of pulses from electron and nuclear recoils have been compared down to 2 keVee. The experimental results are compared to those predicted by Lindhard theory, simulated by the SRIM Monte Carlo code, and a preliminary curve calculated by Prof. Akira Hitachi.
Physics Letters B | 2007
G. J. Alner; H.M. Araújo; A. Bewick; C. Bungau; B. Camanzi; M.J. Carson; R. 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.B. Lawson; V. N. Lebedenko; J.D. Lewin; P. K. Lightfoot; A. Lindote; I. Liubarsky
The first underground data run of the ZEPLIN-II experiment has set a limit on the nuclear recoil rate in the two-phase xenon detector for direct dark matter searches. In this Letter the results from this run are converted into the limits on spin-dependent WIMP-proton and WIMP-neutron cross-sections. The minimum of the curve for WIMP-neutron cross-section corresponds to 7 × 10−2 pb at a WIMP mass of around 65 GeV.
Astroparticle Physics | 2008
H.M. Araújo; J. Blockley; C. Bungau; M.J. Carson; H. Chagani; E. Daw; B. Edwards; C. Ghag; E.V. Korolkova; V.A. Kudryavtsev; P. K. Lightfoot; A. Lindote; I. Liubarsky; R. Lüscher; P. Majewski; K. Mavrokoridis; J.E. McMillan; A. St. J. Murphy; S. M. Paling; J. Pinto da Cunha; R. Preece; M. Robinson; N.J.T. Smith; P.F. Smith; N.J.C. Spooner; T. J. Sumner; R. Walker; H. Wang; J. T. White
We present the first measurements of the muon-induced neutron flux at the Boulby Underground Laboratory. The experiment was carried out with an 0.73 tonne liquid scintillator that also served as an anticoincidence system for the ZEPLIN-II direct dark matter search. The experimental method exploited the delayed coincidences between high-energy muon signals and gamma-rays from radiative neutron capture on hydrogen or other elements. The muon-induced neutron rate, defined as the average number of detected neutrons per detected muon, was measured as 0.079±0.003 (stat.) neutrons/muon using neutron-capture signals above 0.55 MeV in a time window of 40–190 μs after the muon trigger. Accurate Monte Carlo simulations of the neutron production, transport and detection in a precisely modeled laboratory and experimental setup using the GEANT4 toolkit gave a result 1.8 times higher than the measured value. The difference greatly exceeds all statistical and systematic uncertainties. As the vast majority of neutrons detected in the current setup were produced in lead we evaluated from our measurements the neutron yield in lead as (1.31±0.06)×10-3 neutrons/muon/(g/cm2) for a mean muon energy of about 260 GeV.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2008
G. J. Alner; H.M. Araújo; A. Bewick; C. Bungau; B. Camanzi; M.J. Carson; 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; W.G. Jones; M. Joshi; E.V. Korolkova; V.A. Kudryavtsev; T.B. Lawson; V. N. Lebedenko; J.D. Lewin; P. K. Lightfoot; A. Lindote; I. Liubarsky; M.I. Lopes; R. Lüscher
ZEPLIN II is a two-phase (liquid/gas) xenon dark matter detector searching for WIMP-nucleon interactions. In this paper we describe the data acquisition system used to record the data from ZEPLIN II and the reduction procedures which parameterise the data for subsequent analysis.
arXiv: Instrumentation and Detectors | 2007
H. Chagani; P. Majewski; E. Daw; V.A. Kudryavtsev; N.J.C. Spooner
We present preliminary results of measurements of the quenching factor for Na recoils in NaI(Tl) at room temperature, made at a dedicated neutron facility at the University of Sheffield. Measurements have been performed with a 2.45 MeV mono-energetic neutron generator in the energy range from 10 keV to 100 keV nuclear recoil energy. A BC501A liquid scintillator detector was used to tag neutrons. Cuts on pulse-shape discrimination from the BC501A liquid scintillator detector and neutron time-of-flight were performed on pulses recorded by a digitizer with a 2 ns sampling time. Measured quenching factors range from 19% to 26%, in agreement with other experiments. From pulse-shape analysis, a mean time of pulses from electron and nuclear recoils are compared down to 2 keV electron equivalent energy.
Proceedings of Identification of dark matter 2008 — PoS(idm2008) | 2009
H.M. Araújo; J. Blockley; C. Bungau; M.J. Carson; H. Chagani; E. Daw; B. Edwards; C. Ghag; Elena Korolkova; V.A. Kudryavtsev; P. K. Lightfoot; A. Lindote; I. Liubarsky; R. Lüscher; P. Majewski; K. Mavrokoridis; J.E. McMillan; A. St. J. Murphy; S. M. Paling; J. Pinto da Cunha; R. Preece; M. Robinson; N.J.T. Smith; P.F. Smith; N.J.C. Spooner; T. J. Sumner; R. Walker; H. Wang; J. T. White
The first measurements of the muon-induced neutron flux at the Boulby Underground Laboratory are presented. The experiment was carried out with an 0.73 tonne liquid scintillation detector that also served as an anticoincidence system for the ZEPLIN-II direct dark matter search. The experimental method exploited the delayed coincidences between high-energy muon signals and gamma-rays from radiative neutron capture on hydrogen or other elements. The muon-induced neutron rate, defined as the average number of detected neutr ons per detected muon, was measured as 0.079± 0.003 (stat.) neutrons/muon using neutron-capture signals above 0.55 MeV in a time window of 40-190 μs after the muon trigger. Accurate Monte Carlo simulations of the neutron production, transport and detection in a precisely modeled laboratory and experimental setup using the GEANT4 toolkit gave a result 1.8 times higher than the measured value. The difference greatly exceeds all statistical and systematic uncertainties. As the vast majority of neutrons detected in the current setup were produced in lead we evaluated from our measurements the neutron yield in lead as (1.31± 0.06)× 10 3 neutrons/muon/(g/cm 2 ) for a mean muon energy of about 260 GeV.
arXiv: Astrophysics | 2007
R. Bisset; M.J. Carson; H. Chagani; D. Cline; E. Daw; T. Ferbel; J. Gao; Y.S. Gao; V.A. Kudryavtsev; P. K. Lightfoot; P. Majewski; James A. Maxin; J. B. Miller; W. Ooi; M. Robinson; G. Salinas; U. Schroeder; J. Seifert; F. Sergiampietri; W. Skulski; P.F. Smith; N.J.C. Spooner; Jan Toke; H. Wang; J. T. White; F.L.H. Wolfs; X. Yang
We propose a new concept for a very low background Dark Matter experiment using multi-ton liquid xenon. The detector consists of two concentric spheres and a charge readout device in the centre. Xenon between the two spheres forms a self-shield and veto device. The inner surface of the centre sphere is coated with CsI to form an internal photocathode with minimum of 2π coverage for any event in the active volume. Photoelectrons from the CsI photocathode drift toward the charge readout micro-structure in the centre of the detector. Both scintillation and ionisation is measured simultaneously for background rejection and 3-D event mapping. In addition to external shielding, the low background is achieved by eliminating PMTs and by using low radioactivity pure materials throughout the detector. We present detailed calculations of the charge readout system and design details. The detector is expected to probe the full SUSY parameter space.
Astroparticle Physics | 2007
G. J. Alner; H.M. Araújo; A. Bewick; C. Bungau; B. Camanzi; M.J. Carson; R. 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.B. Lawson; V. N. Lebedenko; J.D. Lewin; P. K. Lightfoot; A. Lindote; I. Liubarsky