T
T. J. Sumner
Researcher at Imperial College London
Publications - 342
Citations - 18702
T. J. Sumner is an academic researcher from Imperial College London. The author has contributed to research in topics: Dark matter & Xenon. The author has an hindex of 62, co-authored 329 publications receiving 16405 citations. Previous affiliations of T. J. Sumner include University of Rochester & University of Florida.
Papers
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Journal ArticleDOI
Low-temperature study of 35 photomultiplier tubes for the ZEPLIN III experiment
Henrique Araujo,A. Bewick,D. C. R. Davidge,J. V. Dawson,T Ferbel,A. S. Howard,W. G. Jones,M. K. Joshi,V. N. Lebedenko,I. Liubarsky,J. J. Quenby,T. J. Sumner,F. Neves +12 more
TL;DR: In this paper, a set of 35 photomultiplier tubes (ETL D730/9829Q) intended for use in the ZEPLIN III Dark Matter detector, was tested from room temperature down to −100°C, with the aim of confirming their suitability for detecting xenon scintillation light at 175 nm while immersed in the cryogenic liquid.
Journal ArticleDOI
Status of ZEPLIN II and ZEPLIN IV study
David B. Cline,Youngho Seo,F. Sergiampietri,H. Wang,J. T. White,J. Gao,P. Picchi,G. Mannocchi,L. Periale,F. Pietropaolo,G. J. Alner,S. P. Hart,J.D. Lewin,R. M. Preece,P.F. Smith,N. J. T. Smith,N. J. C. Spooner,Daniel Tovey,J. J. Quenby,T. J. Sumner,W. G. Jones,I. Liubarsky +21 more
TL;DR: ZEPLIN II as discussed by the authors is a 30-kg two-phase discriminating xenon detector to be installed in Boulby Mine, UK, for the direct detection of WIMP dark matter.
Journal ArticleDOI
Electrostatic charging of cubic test masses in the LISA mission
TL;DR: In this article, a Monte Carlo simulation of electrostatic charging of the LISA test masses by cosmic-ray protons and alpha particles has been developed using the Geant4 toolkit.
Journal ArticleDOI
Chromatographic separation of radioactive noble gases from xenon
D. S. Akerib,D. S. Akerib,D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,T. P. Biesiadzinski,T. P. Biesiadzinski,E. M. Boulton,R. Bramante,R. Bramante,R. Bramante,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,A.A. Chiller,C. Chiller,T. Coffey,A. Currie,J. E. Cutter,T. J. R. Davison,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,S. A. Hertel,D. P. Hogan,M. Horn,M. Horn,D. Q. Huang,C. M. Ignarra,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,W. Ji,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,C. Lee,C. Lee,B. G. Lenardo,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. O’Sullivan,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,K. J. Palladino,K. J. Palladino,E. K. Pease,K. Pech,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,T. A. Shutt,T. A. Shutt,C. Silva,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,W. H. To,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,T. J. Whitis,T. J. Whitis,Michael S. Witherell,F.L.H. Wolfs,K. Yazdani,Sarah Young,Chao Zhang +123 more
TL;DR: The Large Underground Xenon (LUX) experiment operates at the Sanford Underground Research Facility to detect nuclear recoils from the hypothetical Weakly Interacting Massive Particles (WIMPs) on a liquid xenon target as discussed by the authors.
Journal ArticleDOI
Position Reconstruction in LUX
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,Adam Bernstein,T. P. Biesiadzinski,E. M. Boulton,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,A. Currie,J. E. Cutter,T. J. R. Davison,A. Dobi,E. Druszkiewicz,Blair Edwards,S. R. Fallon,A. Fan,S. Fiorucci,R. J. Gaitskell,J. Genovesi,C. Ghag,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,R. G. Jacobsen,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N. A. Larsen,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O'Sullivan,K. C. Oliver-Mallory,K. J. Palladino,E. K. Pease,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,V. Velan,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,Michael S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +92 more
TL;DR: In this paper, the authors used an iterative method to recover the photomultiplier tube (PMT) light response directly from the calibration data using a two dimensional functional form to account for the photons reflected on the inner walls of the detector.