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91探花
Insertion of STC into TRT at the Department of Physics, 91探花
Credit: CERN

Prof Dr Armin Reichold

Professor of Physics

Research theme

  • Accelerator physics
  • Fundamental particles and interactions

Sub department

  • Particle Physics

Research groups

  • Future Colliders
  • SNO+
Armin.Reichold@physics.ox.ac.uk
Telephone: 01865 (2)73358
Denys Wilkinson Building, room 473,617
  • About
  • Publications

Current status and future prospects of the SNO+ experiment

Advances in High Energy Physics Hindawi Publishing Corporation 2016 (2016) 6194250-6194250

Authors:

Steven D Biller, Luca A Cavalli, Jack T Dunger, Nicholas A Jelley, Christopher Jones, Peter G Jones, Jeffrey Lidgard, Krishana Majumdar, Armin Reichold, Laura Segui, Jeffrey C-L Tseng

Abstract:

SNO+ is a large liquid scintillator-based experiment located 2km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12m diameter acrylic vessel which will be filled with about 780 tonnes of ultra-pure liquid scintillator. Designed as a multipurpose neutrino experiment, the primary goal of SNO+ is a search for the neutrinoless double-beta decay (0$\nu\beta\beta$) of 130Te. In Phase I, the detector will be loaded with 0.3% natural tellurium, corresponding to nearly 800 kg of 130Te, with an expected effective Majorana neutrino mass sensitivity in the region of 55-133 meV, just above the inverted mass hierarchy. Recently, the possibility of deploying up to ten times more natural tellurium has been investigated, which would enable SNO+ to achieve sensitivity deep into the parameter space for the inverted neutrino mass hierarchy in the future. Additionally, SNO+ aims to measure reactor antineutrino oscillations, low-energy solar neutrinos, and geoneutrinos, to be sensitive to supernova neutrinos, and to search for exotic physics. A first phase with the detector filled with water will begin soon, with the scintillator phase expected to start after a few months of water data taking. The 0$\nu\beta\beta$ Phase I is foreseen for 2017.

Current Status and Future Prospects of the SNO+ Experiment

(2015)

Authors:

SNO Collaboration, :, S Andringa, E Arushanova, S Asahi, M Askins, DJ Auty, AR Back, Z Barnard, N Barros, EW Beier, A Bialek, SD Biller, E Blucher, R Bonventre, D Braid, E Caden, E Callaghan, J Caravaca, J Carvalho, L Cavalli, D Chauhan, M Chen, O Chkvorets, K Clark, B Cleveland, IT Coulter, D Cressy, X Dai, C Darrach, B Davis-Purcell, R Deen, MM Depatie, F Descamps, F Di Lodovico, N Duhaime, F Duncan, J Dunger, E Falk, N Fatemighomi, R Ford, P Gorel, C Grant, S Grullon, E Guillian, AL Hallin, D Hallman, S Hans, J Hartnell, P Harvey, M Hedayatipour, WJ Heintzelman, RL Helmer, B Hreljac, J Hu, T Iida, CM Jackson, NA Jelley, C Jillings, C Jones, PG Jones, K Kamdin, T Kaptanoglu, J Kaspar, P Keener, P Khaghani, L Kippenbrock, JR Klein, R Knapik, JN Kofron, LL Kormos, S Korte, C Kraus, CB Krauss, K Labe, I Lam, C Lan, BJ Land, S Langrock, A LaTorre, I Lawson, GM Lefeuvre, EJ Leming, J Lidgard, X Liu, Y Liu, V Lozza, S Maguire, A Maio, K Majumdar, S Manecki, J Maneira, E Marzec, A Mastbaum, N McCauley, AB McDonald, JE McMillan, P Mekarski, C Miller, Y Mohan, E Mony, MJ Mottram, V Novikov, HM O'Keeffe, E O'Sullivan, GD Orebi Gann, MJ Parnell, SJM Peeters, T Pershing, Z Petriw, G Prior, JC Prouty, S Quirk, A Reichold, A Robertson, J Rose, R Rosero, PM Rost, J Rumleskie, MA Schumaker, MH Schwendener, D Scislowski, J Secrest, M Seddighin, L Segui, S Seibert, T Shantz, TM Shokair, L Sibley, JR Sinclair, K Singh, P Skensved, A Soerensen, T Sonley, R Stainforth, M Strait, MI Stringer, R Svoboda, J Tatar, L Tian, N Tolich, J Tseng, HWC Tseung, R Van Berg, E V谩zquez-J谩uregui, C Virtue, B von Krosigk, JMG Walker, M Walker, O Wasalski, J Waterfield, RF White, JR Wilson, TJ Winchester, A Wright, M Yeh, T Zhao, K Zuber

Multi-channel absolute distance measurement system with sub ppm-accuracy and 20 m range using frequency scanning interferometry and gas absorption cells

Optics Express Optica Publishing Group 22:20 (2014) 24869-24893

Authors:

John Dale, Ben Hughes, Andrew J Lancaster, Andrew J Lewis, Armin JH Reichold, Matthew S Warden

Resolution of Longitudinal Profile Measures using Coherent Smith-Purcell Radiation with the Number of Gratings and the Number of Pulses Used

(2014)

Authors:

M茅lissa Vieille Grosjean, Joanna Barros, Nicolas Delerue, Faissal Bakkali Taheri, George Doucas, Ivan Vasilyevich Konoplev, Armin Reichold, Christine Isabel Clarke

Reconstruction of longitudinal electrons bunch profiles at FACET, SLAC

IPAC 2014: Proceedings of the 5th International Particle Accelerator Conference (2014) 3453-3455

Authors:

J Barros, N Delerue, S Jenzer, M Vieille Grosjean, F Bakkali Taheri, G Doucas, I Konoplev, A Reichold, C Clarke

Abstract:

The E-203 collaboration is testing a device on FACET at SLAC to measure the longitudinal profile of electron bunches using Smith-Purcell radiation [1]. At FACET the electron bunches have an energy of 20 GeV and a duration of a few hundred femtoseconds [2]. Smith-Purcell radiation is emitted when a charged particle passes close to the surface of a metallic grating. We have studied the stability of the measurement from pulse to pulse and the resolution of the measure depending on the number of gratings used.

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