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91Ě˝»¨
Bullet cluster image
Credit: Credit: X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.; Lensing Map: NASA/STScI

Professor Jocelyn Monroe

Professor of Particle Physics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Particle Physics
jocelyn.monroe@physics.ox.ac.uk
Telephone: 273317
  • About
  • Publications

Characterization of germanium detectors for the first underground laboratory in Mexico

Journal of Instrumentation 15:11 (2020)

Authors:

A Aguilar-Arevalo, S Alvarado-Mijangos, X Bertou, C Canet, MA Cruz-Pérez, A Deisting, A Dias, JC D’Olivo, F Favela-Pérez, EA Garcés, A González Muñoz, JO Guerra-Pulido, J Mancera-Alejandrez, DJ Marín-Lámbarri, M Martinez Montero, J Monroe, C Iván Ortega-Hernández, S Paling, S Peeters, D Ruíz Esparza Rodríguez, PR Scovell, C Türkoğlu, E Vázquez-Jáuregui, J Walding

Abstract:

This article reports the characterization of two High Purity Germanium detectors performed by extracting and comparing their efficiencies using experimental data and Monte Carlo simulations. The efficiencies were calculated for pointlike -ray sources as well as for extended calibration sources. Characteristics of the detectors such as energy linearity, energy resolution and full energy peak efficiencies are reported from measurements performed on surface laboratories. The detectors will be deployed in a γ-ray assay facility that will be located in the first underground laboratory in Mexico, Laboratorio Subterráneo de Mineral del Chico (LABChico), in the Comarca Minera UNESCO Global Geopark [1].

Constraints on dark matter-nucleon effective couplings in the presence of kinematically distinct halo substructures using the DEAP-3600 detector

Physical Review D American Physical Society (APS) 102:8 (2020) 082001

Authors:

P Adhikari, R Ajaj, DJ Auty, CE Bina, W Bonivento, MG Boulay, M Cadeddu, B Cai, M Cárdenas-Montes, S Cavuoti, Y Chen, BT Cleveland, JM Corning, S Daugherty, P DelGobbo, P Di Stefano, L Doria, M Dunford, A Erlandson, SS Farahani, N Fatemighomi, G Fiorillo, D Gallacher, EA Garcés, P García Abia, S Garg, P Giampa, D Goeldi, P Gorel, K Graham, A Grobov, AL Hallin, M Hamstra, T Hugues, A Ilyasov, A Joy, B Jigmeddorj, CJ Jillings, O Kamaev, G Kaur, A Kemp, I Kochanek, M Kuźniak, M Lai, S Langrock, B Lehnert, N Levashko, X Li, O Litvinov, J Lock, G Longo, I Machulin, AB McDonald, T McElroy, JB McLaughlin, C Mielnichuk, J Monroe, G Oliviéro, S Pal, SJM Peeters, V Pesudo, M-C Piro, TR Pollmann, ET Rand, C Rethmeier, F Retière, I Rodríguez-García, L Roszkowski, E Sanchez García, T Sánchez-Pastor, R Santorelli, D Sinclair, P Skensved, B Smith, NJT Smith, T Sonley, R Stainforth, M Stringer, B Sur, E Vázquez-Jáuregui, S Viel, AC Vincent, J Walding, M Waqar, M Ward, S Westerdale, J Willis, A Zuñiga-Reyes

Dosimetry and Calorimetry Performance of a Scientific CMOS Camera for Environmental Monitoring.

Sensors (Basel, Switzerland) 20:20 (2020) E5746

Authors:

Alexis Aguilar-Arevalo, Xavier Bertou, Carles Canet, Miguel Angel Cruz-Pérez, Alexander Deisting, Adriana Dias, Juan Carlos D'Olivo, Francisco Favela-Pérez, Estela A Garcés, Adiv González Muñoz, Jaime Octavio Guerra-Pulido, Javier Mancera-Alejandrez, Daniel José Marín-Lámbarri, Mauricio Martinez Montero, Jocelyn Monroe, Sean Paling, Simon JM Peeters, Paul Scovell, Cenk Türkoğlu, Eric Vázquez-Jáuregui, Joseph Walding

Abstract:

This paper explores the prospect of CMOS devices to assay lead in drinking water, using calorimetry. Lead occurs together with traces of radioisotopes, e.g., 210Pb, producing g-emissions with energies ranging from 10 keV to several 100 keV when they decay; this range is detectable in silicon sensors. In this paper we test a CMOS camera (OXFORD INSTRUMENTS Neo 5.5) for its general performance as a detector of X-rays and low energy g-rays and assess its sensitivity relative to the World Health Organization upper limit on lead in drinking water. Energies from 6 keV to 60 keV are examined. The CMOS camera has a linear energy response over this range and its energy resolution is for the most part slightly better than 2%. The Neo sCMOS is not sensitive to X-rays with energies below ~10 keV. The smallest detectable rate is 40 ± 3 mHz, corresponding to an incident activity on the chip of 7 ± 4 Bq. The estimation of the incident activity sensitivity from the detected activity relies on geometric acceptance and the measured efficiency vs. energy. We report the efficiency measurement, which is 0.08(2)% (0.0011(2)%) at 26.3 keV (59.5 keV). Taking calorimetric information into account we measure a minimal detectable rate of 4 ± 1 mHz (1.5 ± 0.1 mHz) for 26.3 keV (59.5 keV) g-rays, which corresponds to an incident activity of 1.0 ± 0.6 Bq (57 ± 33 Bq). Toy Monte Carlo and Geant4 simulations agree with these results. These results show this CMOS sensor is well-suited as a g- and X-ray detector with sensitivity at the few to 100 ppb level for 210Pb in a sample.

Search for hep solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory

Physical Review D American Physical Society (APS) 102:6 (2020) 062006

Authors:

B Aharmim, SN Ahmed, AE Anthony, N Barros, EW Beier, A Bellerive, B Beltran, M Bergevin, SD Biller, E Blucher, R Bonventre, K Boudjemline, MG Boulay, B Cai, EJ Callaghan, J Caravaca, YD Chan, D Chauhan, M Chen, BT Cleveland, GA Cox, X Dai, H Deng, FB Descamps, JA Detwiler, PJ Doe, G Doucas, P-L Drouin, M Dunford, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, F Fleurot, RJ Ford, JA Formaggio, N Gagnon, K Gilje, J TM Goon, K Graham, E Guillian, S Habib, RL Hahn, AL Hallin, ED Hallman, PJ Harvey, R Hazama, WJ Heintzelman, J Heise, RL Helmer, A Hime, C Howard, M Huang, P Jagam, B Jamieson, NA Jelley, M Jerkins, KJ Keeter, JR Klein, LL Kormos, M Kos, C Kraus, CB Krauss, A Krüger, T Kutter, CCM Kyba, K Labe, BJ Land, R Lange, A LaTorre, J Law, IT Lawson, KT Lesko, JR Leslie, I Levine, JC Loach, R MacLellan, S Majerus, HB Mak, J Maneira, RD Martin, A Mastbaum, N McCauley, AB McDonald, SR McGee, ML Miller, B Monreal, J Monroe, BG Nickel, AJ Noble, HM O’Keeffe, NS Oblath, CE Okada, RW Ollerhead, GD Orebi Gann, SM Oser, RA Ott, SJM Peeters, AWP Poon, G Prior, SD Reitzner, K Rielage, BC Robertson, RGH Robertson, MH Schwendener, JA Secrest, SR Seibert, O Simard, D Sinclair, P Skensved, TJ Sonley, LC Stonehill, G Tešić, N Tolich, T Tsui, R Van Berg, BA VanDevender, CJ Virtue, BL Wall, D Waller, H Wan Chan Tseung, DL Wark, J Wendland, N West, JF Wilkerson, JR Wilson, T Winchester, A Wright, M Yeh, F Zhang, K Zuber

Off-Axis Characterisation of the CERN T10 Beam for low Momentum Proton Measurements with a High Pressure Gas Time Projection Chamber

Instruments MDPI 4:3 (2020) 21

Authors:

SB Jones, TS Nonnenmacher, E Atkin, GJ Barker, A Basharina-Freshville, C Betancourt, SB Boyd, D Brailsford, Z Chen-Wishart, L Cremonesi, A Deisting, A Dias, P Dunne, J Haigh, P Hamacher-Baumann, A Kaboth, A Korzenev, W Ma, P Mermod, M Mironova, J Monroe, R Nichol, J Nowak, W Parker, H Ritchie-Yates, S Roth, R Saakyan, N Serra, Y Shitov, J Steinmann, A Tarrant, MA Uchida, S Valder, AV Waldron, M Ward, MO Wascko

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