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Featured researches published by T. Durkin.


Physical Review D | 2009

Results from the first science run of the ZEPLIN-III dark matter search experiment

V. N. Lebedenko; H.M. Araújo; E. J. Barnes; A. Bewick; R. Cashmore; V. Chepel; A. Currie; D. Davidge; J. Dawson; T. Durkin; B. Edwards; C. Ghag; M. Horn; A.S. Howard; A. J. Hughes; W.G. Jones; M. Joshi; G. Kalmus; A.G. Kovalenko; A. Lindote; I. Liubarsky; M.I. Lopes; R. Lüscher; P. Majewski; A. St. J. Murphy; F. Neves; J. Pinto da Cunha; R. Preece; J. J. Quenby; P.R. Scovell

The ZEPLIN-III experiment in the Palmer Underground Laboratory at Boulby uses a 12 kg two-phase xenon time-projection chamber to search for the weakly interacting massive particles (WIMPs) that may account for the dark matter of our Galaxy. The detector measures both scintillation and ionization produced by radiation interacting in the liquid to differentiate between the nuclear recoils expected from WIMPs and the electron-recoil background signals down to {approx}10 keV nuclear-recoil energy. An analysis of 847 kg{center_dot}days of data acquired between February 27, 2008, and May 20, 2008, has excluded a WIMP-nucleon elastic scattering spin-independent cross section above 8.1x10{sup -8} pb at 60 GeVc{sup -2} with a 90% confidence limit. It has also demonstrated that the two-phase xenon technique is capable of better discrimination between electron and nuclear recoils at low-energy than previously achieved by other xenon-based experiments.


Physical Review Letters | 2009

Limits on the Spin-Dependent WIMP-Nucleon Cross Sections from the First Science Run of the ZEPLIN-III Experiment

V. N. Lebedenko; H.M. Araújo; E. J. Barnes; A. Bewick; R. Cashmore; V. Chepel; A. Currie; D. Davidge; J. Dawson; T. Durkin; B. Edwards; C. Ghag; M. Horn; A.S. Howard; A. J. Hughes; W.G. Jones; M. Joshi; G. Kalmus; A.G. Kovalenko; A. Lindote; I. Liubarsky; M.I. Lopes; R. Lüscher; K. Lyons; P. Majewski; A. St. J. Murphy; F. Neves; J. Pinto da Cunha; R. Preece; J. J. Quenby

We present new experimental constraints on the WIMP-nucleon spin-dependent elastic cross sections using data from the first science run of ZEPLIN-III, a two-phase xenon experiment searching for galactic dark matter weakly interacting massive particles based at the Boulby mine. Analysis of approximately 450 kg x days fiducial exposure allow us to place a 90%-confidence upper limit on the pure WIMP-neutron cross section of sigma(n)=1.9x10(-2) pb at 55 GeV/c(2) WIMP mass. Recent calculations of the nuclear spin structure based on the Bonn charge-dependent nucleon-nucleon potential were used for the odd-neutron isotopes 129Xe and 131Xe. These indicate that the sensitivity of xenon targets to the spin-dependent WIMP-proton interaction could be much lower than implied by previous calculations, whereas the WIMP-neutron sensitivity is impaired only by a factor of approximately 2.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2002

The MINOS light-injection calibration system

P. Adamson; J Alner; B. Anderson; Thomas R. Chase; P.J. Dervan; T. Durkin; E. Falk; P. Harris; D. Michael; R. Morse; R. Nichol; R. Saakyan; C. Smith; Pn Smith; J. Thomas; R. Webb; R. F. White

A description is given of the light-injection calibration system that has been developed for the MINOS long-baseline neutrino oscillation experiment. The system is based upon pulsed blue LEDs monitored by PIN photodiodes. It is designed to measure non-linearities in the PMT gain curves, as well as monitoring any drifts in PMT gain, at the 1% level.


Physics Letters B | 2010

Limits on inelastic dark matter from ZEPLIN-III

D. Yu. Akimov; H.M. Araújo; E. J. Barnes; V. A. Belov; A. Bewick; A. Burenkov; R. Cashmore; V. Chepel; A. Currie; D. Davidge; J. Dawson; T. Durkin; B. Edwards; C. Ghag; A. Hollingsworth; M. Horn; A.S. Howard; A.J. Hughes; W.G. Jones; G. Kalmus; A. S. Kobyakin; A.G. Kovalenko; V. N. Lebedenko; A. Lindote; I. Liubarsky; M.I. Lopes; R. Lüscher; K. Lyons; P. Majewski; A. St. J. Murphy

Abstract We present limits on the WIMP–nucleon cross section for inelastic dark matter from a reanalysis of the 2008 run of ZEPLIN-III. Cuts, notably on scintillation pulse shape and scintillation-to-ionisation ratio, give a net exposure of 63 kg day in the range 20– 80 keV nuclear recoil energy, in which 6 events are observed. Upper limits on signal rate are derived from the maximum empty patch in the data. Under standard halo assumptions a small region of parameter space consistent, at 99% CL, with causing the 1.17 ton yr DAMA modulation signal is allowed at 90% CL: it is in the mass range 45– 60 GeV c − 2 with a minimum CL of 87%, again derived from the maximum patch. This is the tightest constraint yet presented using xenon, a target nucleus whose similarity to iodine mitigiates systematic error from the assumed halo.


Journal of Instrumentation | 2014

Development and testing of an upgrade to the CMS level-1 calorimeter trigger

M. Baber; M. Blake; J. J. Brooke; M. Cepeda Hermida; S. Dasu; T. Durkin; S Fayer; E. Friis; T. Gorski; G. Hall; Kristian Harder; G. Iles; S. J. Ives; J Jones; P. Klabbers; A. Levine; C. Lucas; R. Lucas; Dave M Newbold; J. Marrouche; S. Paramesvaran; T. Perry; A. Rose; Dave Sankey; W. H. Smith; A. Tapper; A. Thea; T. Williams

When the LHC resumes operation in 2015, the higher centre-of-mass energy and high-luminosity conditions will require significantly more sophisticated algorithms to select interesting physics events within the readout bandwidth limitations. The planned upgrade to the CMS calorimeter trigger will achieve this goal by implementing a flexible system based on the μTCA standard, with modules based on Xilinx Virtex-7 FPGAs and up to 144 optical links running at speeds of 10 Gbps. The upgrade will improve the energy and position resolution of physics objects, enable much improved isolation criteria to be applied to electron and tau objects and facilitate pile-up subtraction to mitigate the effect of the increased number of interactions occurring in each bunch crossing. The design of the upgraded system is summarised with particular emphasis placed on the results of prototype testing and the experience gained which is of general application to the design of such systems.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2008

The ZEPLIN II dark matter detector: Data acquisition system and data reduction

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.


Journal of Instrumentation | 2016

Triggering on electrons, jets and tau leptons with the CMS upgraded calorimeter trigger for the LHC RUN II

A. Zabi; F. Beaudette; L. Cadamuro; L. Mastrolorenzo; T. Romanteau; J. B. Sauvan; T. Strebler; J. Marrouche; N. Wardle; R. Aggleton; F. Ball; J. J. Brooke; Dave M Newbold; S. Paramesvaran; D. Smith; M. Baber; A. Bundock; M. Citron; A. Elwood; G. Hall; G. Iles; C. Laner; B. Penning; A. Rose; Alexander Tapper; T. Durkin; Kristian Harder; S. Harper; C. H. Shepherd-Themistocleous; A. Thea

The Compact Muon Solenoid (CMS) experiment has implemented a sophisticated two-level online selection system that achieves a rejection factor of nearly 105. During Run II, the LHC will increase its centre-of-mass energy up to 13 TeV and progressively reach an instantaneous luminosity of 2 × 1034 cm−2 s−1. In order to guarantee a successful and ambitious physics programme under this intense environment, the CMS Trigger and Data acquisition (DAQ) system has been upgraded. A novel concept for the L1 calorimeter trigger is introduced: the Time Multiplexed Trigger (TMT) . In this design, nine main processors receive each all of the calorimeter data from an entire event provided by 18 preprocessors. This design is not different from that of the CMS DAQ and HLT systems. The advantage of the TMT architecture is that a global view and full granularity of the calorimeters can be exploited by sophisticated algorithms. The goal is to maintain the current thresholds for calorimeter objects and improve the performance for their selection. The performance of these algorithms will be demonstrated, both in terms of efficiency and rate reduction. The callenging aspects of the pile-up mitigation and firmware design will be presented.


Journal of Instrumentation | 2017

The CMS Level-1 electron and photon trigger: for Run II of LHC

N. Dev; C. Jessop; F. Meng; Nancy Marinelli; S. Taroni; F. Beaudette; L. Cadamuro; O. Davignon; T. Romanteau; T. Strebler; A. Zabi; J. B. Sauvan; J. Marrouche; N. Wardle; R. Aggleton; F. Ball; J. J. Brooke; Dave M Newbold; S. Paramesvaran; D. Smith; J. Taylor; M. Baber; A. Bundock; M. Citron; A. Elwood; G. Hall; G. Iles; C. Laner; B. Penning; A. Rose

The Compact Muon Solenoid (CMS) employs a sophisticated two-level online triggering system that has a rejection factor of up to 105. Since the beginning of Run II of LHC, the conditions that CMS operates in have become increasingly challenging. The centre-of-mass energy is now 13 TeV and the instantaneous luminosity currently peaks at 1.5 ×1034 cm−2s−1. In order to keep low physics thresholds and to trigger efficiently in such conditions, the CMS trigger system has been upgraded. A new trigger architecture, the Time Multiplexed Trigger (TMT) has been introduced which allows the full granularity of the calorimeters to be exploited at the first level of the online trigger. The new trigger has also benefited immensely from technological improvements in hardware. Sophisticated algorithms, developed to fully exploit the advantages provided by the new hardware architecture, have been implemented. The new trigger system started taking physics data in 2016 following a commissioning period in 2015, and since then has performed extremely well. The hardware and firmware developments, electron and photon algorithms together with their performance in challenging 2016 conditions is presented.


Journal of Instrumentation | 2017

The CMS Level-1 Calorimeter Trigger for the LHC Run II

A. Zabi; F. Beaudette; L. Cadamuro; O. Davignon; T. Romanteau; T. Strebler; M. Cepeda; J. B. Sauvan; N. Wardle; R. Aggleton; F. Ball; J. J. Brooke; Dave M Newbold; S. Paramesvaran; D. Smith; J. Taylor; C. Foudas; M. Baber; A. Bundock; S. Breeze; M. Citron; A. Elwood; G. Hall; G. Iles; C. Laner; B. Penning; A. Rose; A. Shtipliyski; Alexander Tapper; I. Ojalvo

Results from the completed Phase 1 Upgrade of the Compact Muon Solenoid (CMS) Level-1 Calorimeter Trigger are presented. The upgrade was performed in two stages, with the first running in 2015 for proton and heavy ion collisions and the final stage for 2016 data taking. The Level-1 trigger has been fully commissioned and has been used by CMS to collect over 43 fb−1 of data since the start of the Run II of the Large Hadron Collider (LHC). The new trigger has been designed to improve the performance at high luminosity and large number of simultaneous inelastic collisions per crossing (pile-up). For this purpose it uses a novel design, the Time Multiplexed Trigger (TMT), which enables the data from an event to be processed by a single trigger processor at full granularity over several bunch crossings. The TMT design is a modular design based on the μTCA standard. The trigger processors are instrumented with Xilinx Virtex-7 690 FPGAs and 10 Gbps optical links. The TMT architecture is flexible and the number of trigger processors can be expanded according to the physics needs of CMS. Sophisticated and innovative algorithms are now the core of the first decision layer of the experiment. The system has been able to adapt to the outstanding performance of the LHC, which ran with an instantaneous luminosity well above design. The performance of the system for single physics objects are presented along with the optimizations foreseen to maintain the thresholds for the harsher conditions expected during the LHC Run II and Run III periods.


In: Cline, DB, (ed.) (Proceedings) 8th UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe. (pp. 218-+). AMER INST PHYSICS (2009) | 2009

ZEPLIN‐II limits on WIMP‐nucelon interactions

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; V.A. Kudryavtsev; T.B. Lawson; V. N. Lebedenko; J.D. Lewin; P. K. Lightfoot; A. Lindote; I. Liubarsky; M. I. Lopes

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.

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J. Dawson

Imperial College London

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A. Bewick

Imperial College London

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D. Davidge

Imperial College London

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M. Joshi

Imperial College London

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H.M. Araújo

Imperial College London

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W.G. Jones

Imperial College London

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A.S. Howard

Imperial College London

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C. Bungau

Rutherford Appleton Laboratory

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G. J. Alner

Rutherford Appleton Laboratory

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