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.
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eLISA: Astrophysics and cosmology in the millihertz regime
Pau Amaro-Seoane,Sofiane Aoudia,Stanislav Babak,Pierre Binétruy,Emanuele Berti,Alejandro Bohé,Chiara Caprini,Monica Colpi,Neil J. Cornish,Karsten Danzmann,Jean-François Dufaux,Jonathan R. Gair,Oliver Jennrich,Philippe Jetzer,Antoine Klein,Ryan N. Lang,Alberto Lobo,Tyson Littenberg,Sean T. McWilliams,Gijs Nelemans,Antoine Petiteau,Edward K. Porter,Bernard F. Schutz,Alberto Sesana,Robin Stebbins,T. J. Sumner,Michele Vallisneri,Stefano Vitale,Marta Volonteri,H. Ward +29 more
TL;DR: The European New Gravitational wave Observatory (eLISA) as discussed by the authors is the first mission to survey the low-frequency gravitational wave band (about 0.1 mHz to 1 Hz), with sufficient sensitivity to detect interesting individual astrophysical sources out to z = 15.
ReportDOI
LUX-ZEPLIN (LZ) Conceptual Design Report
D. S. Akerib,D. S. Akerib,R. M. Preece,V. Bugaev,T. K. Edberg,Hoff,Patrick Bauer,A. Currie,J. Mock,D. White,V. M. Gehman,S. D. Worm,M. F. Marzioni,D. Markley,C. M. Ignarra,E. M. Boulton,Sergey Burdin,Bhawna Gomber,C. E. Dahl,E. Druszkiewicz,Eli Woods,S. A. Hertel,Daniel McKinsey,P.R. Scovell,T.W. Hurteau,Olevitch,T. A. Shutt,T. J. R. Davison,K. C. Oliver-Mallory,P. Ford,B. Holbrook,C. Ghag,K. Sundarnath,B. N. Edwards,A. Khazov,R.M. Gerhard,J.S. Saba,M. Elnimr,A.A. Chiller,S. Balashov,Wolfgang Lorenzon,L. Reichhart,J. Busenitz,Carl W. Akerlof,V. B. Francis,A. Konovalov,Matthew Szydagis,Mikkel B. Johnson,J. Reichenbacher,H. Kraus,Wenzhao Wei,Laura Manenti,M. Cascella,D. Woodward,Minfang Yeh,C. Carels,S. Luitz,Witherell,W. Skulski,Sridhara Dasu,X. Ji,W. T. Emmet,N.J. Gantos,J. E. Cutter,A. Tomás,K. O'Sullivan,F. G. O'Neill,J. E. Y. Dobson,J. Thomson,J. H. Buckley,K.J. Thomas,I. Stancu,M.J. Barry,T.J. Martin,A. Lindote,M. E. Monzani,R. Bunker,K. T. Lesko,Chao Zhang,Mani Tripathi,S. J. Haselschwardt,L. Tvrznikova,P. A. Terman,Duncan Carlsmith,M. R. While,D. Khaitan,R.G. Jacobsen,J. O'Dell,A. Harris,E. K. Pease,J. Va’vra,J. Lin,K. Skarpaas,Elena Korolkova,S.K. Young,W. Craddock,T. J. Whitis,B. N. Ratcliff,M. C. Carmona-Benitez,J. Liu,R. J. Gaitskell,C. Chiller,H.J. Krebs,K. Kazkaz,N.A. Larsen,R. Bramante,M. G. D. van der Grinten,Richard Rosero,C. R. Hall,E. Holtom,C. Lee,C. O. Vuosalo,V. N. Solovov,C. Rhyne,T. J. Sumner,S. Powell,P. Beltrame,R. C. Webb,M. G. D. Gilchriese,C. Fu,J. A. Morad,S. Kyre,D. R. Tiedt,L. de Viveiros,B. P. Tennyson,D. Q. Huang,C. Silva,A. Bernstein,T. P. Biesiadzinski,J. Balajthy,J.P. Rodrigues,S. J. Patton,M.R. Stark,F.-T. Liao,S. Stephenson,W. H. Lippincott,Yue Meng,K. Pushkin,L. Wang,Michael Schubnell,X. Bai,K. J. Palladino,D.Yu. Akimov,W. H. To,A. V. Kumpan,Alexander Bolozdynya,A. St. J. Murphy,A. Dobi,D. J. Taylor,A.V. Khromov,Ethan Bernard,K. E. Boast,D.C. Malling,P. Sorensen,Peter Majewski,F. Neves,F.L.H. Wolfs,V.V. Sosnovtsev,A. J. Bailey,H. N. Nelson,S. Shaw,J. J. Cherwinka,M.I. Lopes,X. Liu,E. H. Miller,C. Chan,V. A. Kudryavtsev,J.R. Verbus,R. L. Mannino,Dongming Mei,C. H. Faham,S. Uvarov,T.M. Stiegler,R. W. Schnee,M. Pangilinan,Henrique Araujo,S. Alsum,W. J. Wisniewski,H. J. Rose,K. Kamdin,M. Sarychev,A. Manalaysay,W. Ji,J. Yin,W. C. Taylor,W. R. Edwards,J.P. da Cunha,Y. Ju,A. Piepke,W.L. Waldron,C. E. Tull,B. G. Lenardo,Ben Carlson,S. Fiorucci,James Nikkel +194 more
TL;DR: The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report as mentioned in this paper. And the LZ detector will be located at the Sanford Underground Research Facility in South Dakota.
Journal ArticleDOI
Results from the first science run of the ZEPLIN-III dark matter search experiment
V. N. Lebedenko,Henrique Araujo,E. J. Barnes,A. Bewick,R. J. Cashmore,V. Chepel,A. Currie,D. C. R. Davidge,J. V. Dawson,T. Durkin,B. N. Edwards,C. Ghag,M. Horn,A. S. Howard,A. J. Hughes,W. G. Jones,Manasvita Joshi,G. E. 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. M. Preece,J. J. Quenby,P.R. Scovell,C. Silva,V. N. Solovov,N. J. T. Smith,P.F. Smith,V.N. Stekhanov,T. J. Sumner,C. Thorne,R.J. Walker +37 more
TL;DR: 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 as discussed by the authors.
Journal ArticleDOI
The European Large Area ISO Survey - I. Goals, definition and observations
Seb Oliver,Michael Rowan-Robinson,David M. Alexander,Omar Almaini,Marc Balcells,A. C. Baker,Xavier Barcons,Marco Barden,I. Bellas-Velidis,F. Cabrera-Guerra,Ruth Carballo,C. J. Cesarsky,Paolo Ciliegi,David L. Clements,H. Crockett,Luigi Danese,A. Dapergolas,B. Drolias,N. Eaton,Andreas Efstathiou,E. Egami,D. Elbaz,Dario Fadda,M. Fox,Alberto Franceschini,R. Genzel,P. Goldschmidt,Matthew J. Graham,José Ignacio González-Serrano,Eduardo Gonzalez-Solares,Gian Luigi Granato,Carlotta Gruppioni,U. Herbstmeier,Philippe Héraudeau,Manasvita Joshi,E. Kontizas,M. Kontizas,Jari Kotilainen,D. Kunze,F. La Franca,Carlo Lari,Andy Lawrence,Dietrich Lemke,M. J. D. Linden-Vørnle,M. J. D. Linden-Vørnle,Robert G. Mann,Isabel Márquez,Josefa Masegosa,Kalevi Mattila,Richard G. McMahon,George K. Miley,V. Missoulis,Bahram Mobasher,Thierry Morel,Hans Ulrik Nørgaard-Nielsen,Alain Omont,P. Papadopoulos,Ismael Perez-Fournon,J.-L. Puget,D. Rigopoulou,Brigitte Rocca-Volmerange,Stephen Serjeant,Laura Silva,T. J. Sumner,Christian Surace,Petri Vaisanen,P. van der Werf,A. Verma,L. Vigroux,M. Villar-Martin,Chris J. Willott +70 more
TL;DR: The European Large Area ISO Survey (ELAIS) as mentioned in this paper was the largest single Open Time project conducted by ISO, mapping an area of 12deg^2 at 15μm and at 90μm with ISOPHOT.
Journal ArticleDOI
Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment.
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,A. W. Bradley,R. Bramante,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,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,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,D.C. Malling,A. Manalaysay,R. L. Mannino,M. F. Marzioni,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. C. Oliver-Mallory,R. A. Ott,K. J. Palladino,M. Pangilinan,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,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,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,Michael S. Witherell,F.L.H. Wolfs,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.