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Insertion of STC into TRT at the Department of Physics, Oxford
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

Absolute multilateration between spheres

Measurement Science and Technology IOP Publishing 28:4 (2017) 1-11

Authors:

JE Muelaner, W Wadsworth, M Azini, G Mullineux, B Hughes, Armin Reichold

Abstract:

Environmental effects typically limit the accuracy of large scale coordinate measurements in applications such as aircraft production and particle accelerator alignment. This paper presents an initial design for a novel measurement technique with analysis and simulation showing that that it could overcome the environmental limitations to provide a step change in large scale coordinate measurement accuracy. Referred to as absolute multilateration between spheres (AMS), it involves using absolute distance interferometry to directly measure the distances between pairs of plain steel spheres. A large portion of each sphere remains accessible as a reference datum, while the laser path can be shielded from environmental disturbances. As a single scale bar this can provide accurate scale information to be used for instrument verification or network measurement scaling. Since spheres can be simultaneously measured from multiple directions, it also allows highly accurate multilateration-based coordinate measurements to act as a large scale datum structure for localized measurements, or to be integrated within assembly tooling, coordinate measurement machines or robotic machinery. Analysis and simulation show that AMS can be self-aligned to achieve a theoretical combined standard uncertainty for the independent uncertainties of an individual 1 m scale bar of approximately 0.49 µm. It is also shown that combined with a 1 µm m−1 standard uncertainty in the central reference system this could result in coordinate standard uncertainty magnitudes of 42 µm over a slender 1 m by 20 m network. This would be a sufficient step change in accuracy to enable next generation aerospace structures with natural laminar flow and part-topart interchangeability.
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Measurement of event-shape observables in Z→ℓ+ℓ− events in pp collisions at s√=7 TeV with the ATLAS detector at the LHC

European Physical Journal C Springer Berlin Heidelberg 76:7 (2016) 375

Authors:

K Motohashi, R Mount, E Mountricha, SV Mouraviev, EJW Moyse, S Muanza, RD Mudd, F Mueller, J Mueller, RSP Mueller, T Mueller, D Muenstermann, P Mullen, GA Mullier, FJ Munoz Sanchez, JA Murillo Quijada, WJ Murray, H Musheghyan, M Muskinja, AG Myagkov, M Myska, BP Nachman, O Nackenhorst, J Nadal, Koichi Nagai

Abstract:

Event-shape observables measured using charged particles in inclusive Z-boson events are presented, using the electron and muon decay modes of the Z bosons. The measurements are based on an integrated luminosity of 1.1 fb−1 of proton–proton collisions recorded by the ATLAS detector at the LHC at a centre-of-mass energy √s = 7 TeV. Chargedparticle distributions, excluding the lepton–antilepton pair from the Z-boson decay, are measured in different ranges of transverse momentum of the Z boson. Distributions include multiplicity, scalar sum of transverse momenta, beam thrust, transverse thrust, spherocity, and F-parameter, which are in particular sensitive to properties of the underlying event at small values of the Z-boson transverse momentum. The measured observables are compared with predictions from Pythia8, Sherpa, and Herwig7. Typically, all three Monte Carlo generators provide predictions that are in better agreement with the data at high Z-boson transverse momenta than at low Z-boson transverse momenta, and for the observables that are less sensitive to the number of charged particles in the event.
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Experimental and theoretical studies of the properties of coherent Smith-Purcell radiation

Proceedings of International Particle Accelerator Conference 8-13 May 2016, Busan, Korea Joint Accelerator Conferences Website (JACoW) (2016)

Authors:

Faissal Bakkali Taheri, Ivan V Konoplev, George Doucas, Armin Reichold, Riccardo Bartolini, N Delerue, J Barros, C Clarke

Abstract:

Recent advances in physics of particles accelerators and lasers have shifted dramatically the expectations of bunch length and capability to generate electron bunches with specific longitudinal profiles [1,2]. This has stimulated interest in analysis of spectrum of coherent radiation to enable the longitudinal bunch profile diagnostics at femtosecond-scale. Spectral analysis of coherent Smith- Purcell radiation (cSPr) is particularly relevant as it allows non-invasive and cost-effective monitoring of electron bunch profiles. In this paper, the recent results observed from the E203 experiment (FACET, SLAC) are presented. Consistency of the cSPr as diagnostic tool is discussed, as well as the properties of cSPr such as directionality and polarization.
Details from ORA

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.
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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 Vázquez-Jáuregui, 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
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