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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
en.wikipedia.org/wiki/Jocelyn_Monroe
  • About
  • Publications

Characterisation of silicon photomultipliers in a dilution refrigerator down to 9.4 mK towards a cryogenic cosmic-ray muon veto system

Journal of Instrumentation 21:05 (2026)

Authors:

A Kemp, S Autti, E Bloomfield, A Casey, N Darvishi, D Doling, N Eng, P Franchini, RP Haley, PJ Heikkinen, A Jennings, S Koulosousas, E Leason, LV Levitin, J March-Russell, A Mayer, J Monroe, D Münstermann, MT Noble, JR Prance, X Rojas, T Salmon, J Saunders, J Smirnov, R Smith, MD Thompson, A Thomson, A Ting, V Tsepelin, SM West, L Whitehead, DE Zmeev, The QUEST-DMC collaboration

Abstract:

We report the characterisation of a FBK NUV-HD-cryo silicon photomultiplier (SiPM) sensor operated in a 9.4 ± 0.2 mK environment inside a dilution refrigerator, towards the development of a cryogenic cosmic-ray muon veto system to be operated internal to a dilution refrigerator required for low background experiments such as the QUEST-DMC dark matter search experiment. We characterise the single photon response and the gain (the charge produced per detected photon), the dark count noise rate, and correlated noise contributions as a function of operating voltage. This paper also reports first proof-of-concept measurements of using a SiPM coupled to scintillator internal to a dilution refrigerator, towards detecting high-energy events consistent with candidate cosmic-ray muon signals.
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Development of Superfluid Helium-3 Bolometry Using Nanowire Resonators with SQUID Readout for the QUEST-DMC Experiment

Journal of Low Temperature Physics Springer 222:2 (2026) 39

Authors:

E Leason, LV Levitin, S Autti, E Bloomfield, A Casey, N Darvishi, N Eng, P Franchini, RP Haley, PJ Heikkinen, A Jennings, A Kemp, J March-Russell, A Mayer, J Monroe, D Muenstermann, MT Noble, JR Prance, X Rojas, T Salmon, J Saunders, J Smirnov, R Smith, MD Thompson

Abstract:

Superfluid helium-3 bolometers can be utilised for dark matter direct detection searches. The extremely low heat capacity of the B phase of the superfluid helium-3 at ultra-low temperatures offers the potential to reach world leading sensitivity to spin-dependent interactions of dark matter in the sub-GeV/c2 mass range. Here, we describe the development of bolometry using both micron scale and sub-micron diameter vibrating wire resonators, with a SQUID amplifier-based readout scheme. Characterisation of the resonators and bolometer measurements are shown, including the use of nonlinear operation and the corresponding corrections. The bolometer contains two vibrating wire resonators, enabling heat injection calibration and simultaneous bolometer tracking measurements. Coincident events measured on both vibrating wire resonators verify their response. We also demonstrate proof of concept frequency multiplexed readout. Development of these measurement techniques lays the foundations for the use of superfluid helium-3 bolometers, instrumented with vibrating nanomechanical resonators, for future low-threshold dark matter searches.
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Dark matter EFT landscape probed by QUEST-DMC

Journal of Cosmology and Astroparticle Physics IOP Publishing 2025:10 (2025) 44

Authors:

N Darvishi, S Autti, L Bloomfield, A Casey, N Eng, Paolo Franchini, Rp Haley, Pj Heikkinen, A Jennings, A Kemp, Elizabeth Leason, John March-Russell, A Mayer, Jocelyn Monroe, D Münstermann, Mt Noble, Jr Prance, X Rojas, T Salmon, J Saunders, J Smirnov, R Smith, Md Thompson, A Thomson, A Ting, V Tsepelin, Sm West, L Whitehead, De Zmeev

Abstract:

We present the projected sensitivity to non-relativistic Effective Field Theory (EFT) operators for dark matter (DM) direct detection using the QUEST-DMC experiment. QUEST-DMC employs superfluid Helium-3 as a target medium and measures energy deposition via nanomechanical resonators with SQUID-based readout to probe DM interactions. The experiment aims to explore new parameter space in the sub-GeV mass range, probing light DM and a broad range of interaction models. We analyse the sensitivity to a complete set of fourteen independent non-relativistic EFT operators, each parameterised by a Wilson coefficient that quantifies the strength of DM interactions with Standard Model particles. For each interaction channel, we determine the corresponding sensitivity ceiling due to attenuation of the DM flux incident on the detector, caused by DM scattering in the Earth and atmosphere. As a key component of this analysis, we provide the mapping between the non-relativistic EFT operators and the relativistic bilinear DM-nucleon interactions, and assess the interaction sensitivity to sub-GeV DM in the QUEST-DMC detector. Our findings demonstrate that QUEST-DMC provides a unique probe of DM interactions, particularly in previously unexplored parameter space for momentum- and velocity-dependent interactions, thereby expanding the search for viable DM candidates beyond traditional weakly interacting massive particles.
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Direct measurement of the 39 Ar half-life from 3.4 years of data with the DEAP-3600 detector

The European Physical Journal C SpringerOpen 85:7 (2025) 728

Authors:

P Adhikari, R Ajaj, M Alpízar-Venegas, P-A Amaudruz, J Anstey, DJ Auty, M Batygov, B Beltran, MA Bigentini, CE Bina, WM Bonivento, MG Boulay, JF Bueno, M Cadeddu, B Cai, M Cárdenas-Montes, S Cavuoti, Y Chen, S Choudhary, BT Cleveland, R Crampton, S Daugherty, P DelGobbo, P Di Stefano

Abstract:

The half-life of 39Ar is measured using the DEAP-3600 detector located 2 km underground at SNOLAB. Between 2016 and 2020, DEAP-3600 used a target mass of (3269 ± 24) kg of liquid argon distilled from the atmosphere in a direct-detection dark matter search. Such an argon mass also enables direct measurements of argon isotope properties. The decay of 39Ar in DEAP-3600 is the dominant source of triggers by two orders of magnitude, ensuring high statistics and making DEAP-3600 well-suited for measuring this isotope’s half-life. Use of the pulse-shape discrimination technique in DEAP-3600 allows powerful discrimination between nuclear recoils and electron recoils, resulting in the selection of a clean sample of 39Ar decays. Observing over a period of 3.4 years, the 39Ar half-life is measured to be (302±8stat±6sys) years. This new direct measurement suggests that the half-life of 39Ar is significantly longer than the accepted value, with potential implications for measurements using this isotope’s half-life as input.
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Position reconstruction in the DEAP-3600 dark matter search experiment

Journal of Instrumentation 20:07 (2025)

Authors:

P Adhikari, R Ajaj, M Alpízar-Venegas, P-A Amaudruz, J Anstey, GR Araujo, DJ Auty, M Baldwin, M Batygov, B Beltran, H Benmansour, MA Bigentini, CE Bina, J Bonatt, WM Bonivento, MG Boulay, B Broerman, JF Bueno, PM Burghardt, A Butcher, M Cadeddu, B Cai, M Cárdenas-Montes, S Cavuoti, M Chen, Y Chen, S Choudhary, BT Cleveland, JM Corning, R Crampton, D Cranshaw, S Daugherty, P DelGobbo, K Dering, P Di Stefano, J DiGioseffo, G Dolganov, L Doria, FA Duncan, M Dunford, E Ellingwood, A Erlandson, SS Farahani, N Fatemighomi, G Fiorillo, S Florian, A Flower, RJ Ford, R Gagnon, D Gahan, D Gallacher, A Garai, P García Abia, S Garg, P Giampa, A Giménez-Alcázar, D Goeldi, VV Golovko, P Gorel, K Graham, DR Grant, A Grobov, AL Hallin, M Hamstra, PJ Harvey, S Haskins, C Hearns, J Hu, J Hucker, T Hugues, A Ilyasov, B Jigmeddorj, CJ Jillings, A Joy, O Kamaev, G Kaur, A Kemp, M Khoshraftar Yazdi, M Kuźniak, F La Zia, M Lai, S Langrock, B Lehnert, A Leonhardt, J LePage-Bourbonnais, N Levashko, J Lidgard, T Lindner, M Lissia, J Lock, L Luzzi, I Machulin, P Majewski, A Maru, J Mason, AB McDonald, T McElroy, T McGinn, JB McLaughlin, R Mehdiyev, C Mielnichuk, L Mirasola, A Moharana, J Monroe, A Murray, P Nadeau, C Nantais, C Ng, AJ Noble, E O'Dwyer, G Oliviéro, M Olszewski, C Ouellet, S Pal, D Papi, B Park, P Pasuthip, SJM Peeters, M Perry, V Pesudo, E Picciau, M-C Piro, TR Pollmann, F Rad, ET Rand, C Rethmeier, F Retière, I Rodríguez García, L Roszkowski, JB Ruhland, R Santorelli, FG Schuckman, N Seeburn, S Seth, V Shalamova, K Singhrao, P Skensved, T Smirnova, NJT Smith, B Smith, K Sobotkiewich, T Sonley, J Sosiak, J Soukup, R Stainforth, G Stanic, C Stone, V Strickland, M Stringer, B Sur, J Tang, R Turcotte-Tardif, E Vázquez-Jáuregui, L Veloce, S Viel, B Vyas, M Walczak, J Walding, M Waqar, M Ward, S Westerdale, J Willis, R Wormington, A Zuñiga-Reyes, The DEAP collaboration

Abstract:

In the DEAP-3600 dark matter search experiment, precise reconstruction of the positions of scattering events in liquid argon is key for background rejection and defining a fiducial volume that enhances dark matter candidate events identification. This paper describes three distinct position reconstruction algorithms employed by DEAP-3600, leveraging the spatial and temporal information provided by photomultipliers surrounding a spherical liquid argon vessel. Two of these methods are maximum-likelihood algorithms: the first uses the spatial distribution of detected photoelectrons, while the second incorporates timing information from the detected scintillation light. Additionally, a machine learning approach based on the pattern of photoelectron counts across the photomultipliers is explored.
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