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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

David Wark

Professor of Particle Physics

Sub department

  • Particle Physics

Research groups

  • Accelerator Neutrinos
dave.wark@physics.ox.ac.uk
Telephone: 01865 (2)73400
Denys Wilkinson Building, room 626
  • About
  • Publications

Neutral current and day night measurements from the pure D2O phase of SNO

Nuclear and Particle Physics Proceedings Elsevier 118 (2003) 3-14

Authors:

AL Hallin, EW Beier, SD Biller, MG Boulay, MG Bowler, TJ Bowles, SJ Brice, TV Bullard, J Cameron, YD Chan, X Chen, M Chen, BT Cleveland, GA Cox, X Dai, F Dalnoki-Veress, PJ Doe, G Doucas, MR Dragowsky, CA Duba, FA Duncan, M Dunford, JA Dunmore, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, JA Formaggio, MM Fowler, K Frame, W Frati, N Gagnon, K Graham, DR Grant, RL Hahn, ED Hallman, AS Hamer, WB Handler, CK Hargrove, PJ Harvey, R Hazama, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, A Hime, M Howe, P Jagam, NA Jelley, K Kazkaz, PT Keener, JR Klein, T Kutter, CCM Kyba, J Law, IT Lawson, KT Lesko, JR Leslie, I Levine, S Luoma, S Majerus, HB Mak, J Maneira, J Manor, AD Marino, N McCauley, AB McDonald, G McGregor, GG Miller, CW Nally, AJ Noble, EB Norman, CE Okada, JL Orrell, SM Oser, AWP Poon, BC Robertson, RGH Robertson, SSE Rosendahl, VL Rusu, KK Schaffer, MH Schwendener, JJ Simpson, CJ Sims, D Sinclair, P Skensved, MWE Smith, T Spreitzer, N Starinsky, RG Stokstad, LC Stonehill, R Tafirout, N Tagg, R Van Berg, RG Van de Water, CJ Virtue, CE Waltham, DL Wark, N West, JB Wilhelmy, JF Wilkerson, JR Wilson, P Wittich, JM Wouters, M Yeh
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Neutrino masses and mixings — experiments past, present, and future

Nuclear and Particle Physics Proceedings Elsevier 117 (2003) 164-185
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The KATRIN experiment - direct measurement of neutrino masses in the sub-ev region

Proceedings of Science 10 (2003)

Authors:

B Bornschein, K Essig, B Müller, T Thümmler, C Weinheimer, J Herbert, O Malyshev, R Reid, IN Meshkov, Y Syresin, A Osipowicz, T Armbrust, H Blümer, L Bornschein, F Eichelhardt, J Reichenbacher, J Wolf, G Drexlin, K Eitel, R Gumbsheimer, H Hucker, P Plischke, F Schwamm, S Mutterer, H Skacel, M Steidl, A Beglarian, H Gemmecke, S Wüstling, S Bobien, C Day, R Gehring, V Hauer, KP Jüngst, P Komarek, A Kudymov, X Luo, H Neumann, M Noe, L Dörr, M Glugla, J Bonn, F Glück, B Flatt, C Kraus, EW Otten, S Sanchez Majos, VN Aseev, EV Geraskin, O Kazachenko, VM Lobashev, BE Stern, NA Titov, SA Zadorozhny, Y Zakharov, O Dragoun, J Kaspar, A Kovalik, M Rysavy, A Spalek, D Venos, M Zboril, DL Wark, T Burritt, PJ Doe, J Formaggio, T Gadfort, G Harper, M Howe, S McGee, A Myers, RGH Robertson, T VanWechel, JF Wilkerson, M Charlton, AJ Davies, HH Telle

Abstract:

With the evidence for massive neutrinos from recent ν-oscillation experiments, one of the most fundamental tasks of particle physics over the next years will be the determination of the absolute mass scale of neutrinos, which has crucial implications for cosmology, astrophysics and particle physics. The KArlsruhe TRItium Neutrino (KATRIN) experiment is the next-generation direct neutrino mass experiment with a sensitivity to sub-eV ν-masses. It combines an ultra-luminous molecular windowless gaseous tritium source with a high resolution electrostatic retarding spectrometer (MAC-E filter) to measure the spectral shape of β-decay electrons close to the endpoint at 18.6 keV with unprecedented precision. If no neutrino mass signal is found, the KATRIN sensitivity after 3 years of measurements is mν < 0.2 eV/c2 (90 % CL.); a ν-mass signal of mν = 0.35 (0.30) eV/c2 can be measured with 5 (3) σ evidence.

Particle physics: Now you see them, now you don't.

Nature 421:6922 (2003) 485-486
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Solar neutrino results and present status

Physics of Atomic Nuclei 65:12 (2002) 2156-2160

Authors:

VV Gorbachev, JN Abdurashitov, TJ Bowles, ML Cherry, BT Cleveland, R Davis, SR Elliott, VN Gavrin, SV Girin, PP Gurkina, TV Ibragimova, AV Kalikhov, NG Khairnasov, TV Knodel, K Lande, IN Mirmov, JS Nico, AA Shikhin, WA Teasdale, EP Veretenkin, VM Vermul, DL Wark, PS Wildenhain, JF Wilkerson, VE Yants, GT Zatsepin

Abstract:

The solar neutrino capture rate measured by the Russian-American Gallium Experiment on a metallic gallium target SAGE during the time from January 1990 through December 2000 is 77.0-6.2-3.0+6.2+3.5 SNU, where the uncertainties are statistical and systematic, respectively. The experimental procedures and data analysis are presented. © 2002 MAIK. "Nauka/Interperiodica".
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