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

Dr Kevin Thieme

Postdoctoral Research Assistant

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Particle Physics

Research groups

  • LUX-ZEPLIN
kevin.thieme@physics.ox.ac.uk
Denys Wilkinson Building, room 504A
INSPIRE HEP
ORCID
  • About
  • CV
  • Publications

DarkSide-20k sensitivity to light dark matter particles

Communications Physics Springer Nature 7:1 (2024) 422

Authors:

F Acerbi, P Adhikari, P Agnes, I Ahmad, S Albergo, Ifm Albuquerque, T Alexander, Ak Alton, P Amaudruz, M Angiolilli, E Aprile, R Ardito, M Atzori Corona, Dj Auty, M Ave, Ic Avetisov, O Azzolini, Ho Back, Z Balmforth, A Barrado Olmedo, P Barrillon, G Batignani, P Bhowmick, S Blua, V Bocci, W Bonivento, B Bottino, Mg Boulay, A Buchowicz, S Bussino, J Busto, M Cadeddu, M Cadoni, R Calabrese, V Camillo, A Caminata, N Canci, A Capra, M Caravati, M Cárdenas-Montes, N Cargioli, M Carlini, A Castellani, P Castello, P Cavalcante, S Cebrian, JM Cela Ruiz, S Chashin, A Chepurnov, L Cifarelli

Abstract:

The dual-phase liquid argon time projection chamber is presently one of the leading technologies to search for dark matter particles with masses below 10 GeV c−2. This was demonstrated by the DarkSide-50 experiment with approximately 50 kg of low-radioactivity liquid argon as target material. The next generation experiment DarkSide-20k, currently under construction, will use 1,000 times more argon and is expected to start operation in 2027. Based on the DarkSide-50 experience, here we assess the DarkSide-20k sensitivity to models predicting light dark matter particles, including Weakly Interacting Massive Particles (WIMPs) and sub-GeV c−2 particles interacting with electrons in argon atoms. With one year of data, a sensitivity improvement to dark matter interaction cross-sections by at least one order of magnitude with respect to DarkSide-50 is expected for all these models. A sensitivity to WIMP–nucleon interaction cross-sections below 1 × 10−42 cm2 is achievable for WIMP masses above 800 MeV c−2. With 10 years exposure, the neutrino fog can be reached for WIMP masses around 5 GeV c−2.
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A new hybrid gadolinium nanoparticles-loaded polymeric material for neutron detection in rare event searches

Journal of Instrumentation IOP Publishing 19:09 (2024) P09021

Authors:

F Acerbi, P Adhikari, P Agnes, I Ahmad, S Albergo, IF Albuquerque, T Alexander, AK Alton, P Amaudruz, M Angiolilli, E Aprile, R Ardito, M Atzori Corona, DJ Auty, M Ave, IC Avetisov, O Azzolini, HO Back, Z Balmforth, A Barrado Olmedo, P Barrillon, G Batignani, P Bhowmick, V Bocci

Abstract:

Experiments aimed at direct searches for WIMP dark matter require highly effective reduction of backgrounds and control of any residual radioactive contamination. In particular, neutrons interacting with atomic nuclei represent an important class of backgrounds due to the expected similarity of a WIMP-nucleon interaction, so that such experiments often feature a dedicated neutron detector surrounding the active target volume. In the context of the development of DarkSide-20k detector at INFN Gran Sasso National Laboratory (LNGS), several R&D projects were conceived and developed for the creation of a new hybrid material rich in both hydrogen and gadolinium nuclei to be employed as an essential element of the neutron detector. Thanks to its very high cross-section for neutron capture, gadolinium is one of the most widely used elements in neutron detectors, while the hydrogen-rich material is instrumental in efficiently moderating the neutrons. In this paper results from one of the R&Ds are presented. In this effort the new hybrid material was obtained as a poly(methyl methacrylate) (PMMA) matrix, loaded with gadolinium oxide in the form of nanoparticles. We describe its realization, including all phases of design, purification, construction, characterization, and determination of mechanical properties of the new material.
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Constraints on directionality effect of nuclear recoils in a liquid argon time projection chamber

The European Physical Journal C SpringerOpen 84:1 (2024) 24

Authors:

P Agnes, I Ahmad, S Albergo, IFM Albuquerque, T Alexander, AK Alton, P Amaudruz, M Atzori Corona, M Ave, I Ch Avetisov, O Azzolini, HO Back, Z Balmforth, A Barrado-Olmedo, P Barrillon, A Basco, G Batignani, V Bocci, WM Bonivento, B Bottino, MG Boulay, J Busto, M Cadeddu, A Caminata, N Canci, G Cappello, A Capra, S Caprioli, M Caravati, N Cargioli, M Carlini, P Castello, V Cataudella, P Cavalcante, S Cavuoti, S Cebrian, JM Cela Ruiz, S Chashin, A Chepurnov, E Chyhyrynets, L Cifarelli, D Cintas, M Citterio, B Cleveland, V Cocco, E Conde Vilda, L Consiglio, S Copello, G Covone, M Czubak

Abstract:

Ph.D
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Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136Xe

European Physical Journal C Springer Nature 83:11 (2023) 996

Authors:

F Agostini, SEM Ahmed Maouloud, L Althueser, F Amaro, B Antunovic, E Aprile, L Baudis, D Baur, Y Biondi, A Bismark, PA Breur, A Brown, G Bruno, R Budnik, C Capelli, J Cardoso, D Cichon, M Clark, AP Colijn, JJ Cuenca-García, JP Cussonneau, MP Decowski, A Depoian, J Dierle, P Di Gangi, A Di Giovanni, S Diglio, JMF dos Santos, G Drexlin, K Eitel, R Engel, AD Ferella, H Fischer, M Galloway, F Gao, F Girard, F Glück, L Grandi, R Größle, R Gumbsheimer, S Hansmann-Menzemer, F Jörg, G Khundzakishvili, A Kopec, F Kuger, LM Krauss, H Landsman, RF Lang, S Lindemann, M Lindner, JAM Lopes, A Loya Villalpando, C Macolino, A Manfredini, T Marrodán Undagoitia, J Masbou, E Masson, P Meinhardt, S Milutinovic, A Molinario, CMB Monteiro, M Murra, UG Oberlack, M Pandurovic, R Peres, J Pienaar, M Pierre, V Pizzella, J Qin, D Ramírez García, S Reichard, N Rupp, P Sanchez-Lucas, G Sartorelli, D Schulte, M Schumann, L Scotto Lavina, M Selvi, M Silva, H Simgen, M Steidl, A Terliuk, C Therreau, D Thers, K Thieme, R Trotta, CD Tunnell, K Valerius, G Volta, D Vorkapic, C Weinheimer, C Wittweg, J Wolf, JP Zopounidis, K Zuber
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Study of cosmogenic activation above ground for the DarkSide-20k experiment

Astroparticle Physics Elsevier 152 (2023) 102878

Authors:

A Elersich, P Agnes, I Ahmad, S Albergo, IFM Albuquerque, T Alexander, AK Alton, P Amaudruz, M Atzori Corona, M Ave, I Ch Avetisov, O Azzolini, HO Back, Z Balmforth, A Barrado-Olmedo, P Barrillon, A Basco, G Batignani, V Bocci, WM Bonivento, B Bottino, MG Boulay, J Busto, M Cadeddu, A Caminata, N Canci, A Capra, S Caprioli, M Caravati, N Cargioli, M Carlini, P Castello, P Cavalcante, S Cavuoti, S Cebrian, JM Cela Ruiz, S Chashin, A Chepurnov, E Chyhyrynets, L Cifarelli, D Cintas, M Citterio, B Cleveland, V Cocco, D Colaiuda, E Conde Vilda, L Consiglio, S Copello, G Covone, M Czubak, M D’Aniello, S D’Auria, MD Da Rocha Rolo, S Davini, S De Cecco, D De Gruttola, S De Pasquale, G De Rosa, G Dellacasa, AV Derbin, A Devoto, F Di Capua, L Di Noto, P Di Stefano, G Dolganov, F Dordei, E Ellingwood, T Erjavec, M Fernandez Diaz, G Fiorillo, P Franchini, D Franco, N Funicello, F Gabriele, D Gahan, C Galbiati, G Gallina, G Gallus, M Garbini, P Garcia Abia, A Gendotti, C Ghiano, C Giganti, GK Giovanetti, V Goicoechea Casanueva, A Gola, G Grauso, G Grilli di Cortona, A Grobov, M Gromov, M Guan, M Guerzoni, M Gulino, C Guo, BR Hackett, AL Hallin, A Hamer, M Haranczyk, T Hessel, S Hill, S Horikawa, F Hubaut, J Hucker, T Hugues, An Ianni, V Ippolito, C Jillings, S Jois, P Kachru, AA Kemp, CL Kendziora, M Kimura, I Kochanek, K Kondo, G Korga, S Koulosousas, A Kubankin, M Kuss, M Kuzniak, M La Commara, M Lai, E Le Guirriec, E Leason, A Leoni, L Lidey, M Lissia, L Luzzi, O Lychagina, O Macfadyen, IN Machulin, S Manecki, I Manthos, L Mapelli, A Margotti, SM Mari, C Mariani, J Maricic, A Marini, M Martínez, CJ Martoff, G Matteucci, K Mavrokoridis, AB McDonald, A Messina, R Milincic, A Mitra, A Moharana, J Monroe, E Moretti, M Morrocchi, T Mróz, VN Muratova, C Muscas, P Musico, R Nania, M Nessi, G Nieradka, K Nikolopoulos, J Nowak, K Olchansky, A Oleinik, V Oleynikov, P Organtini, A Ortiz de Solórzano, L Pagani, M Pallavicini, L Pandola, E Pantic, E Paoloni, G Paternoster, PA Pegoraro, K Pelczar, C Pellegrino, V Pesudo, S Piacentini, L Pietrofaccia, N Pino, A Pocar, DM Poehlmann, S Pordes, P Pralavorio, D Price, F Ragusa, Y Ramachers, M Razeti, AL Renshaw, M Rescigno, F Retiere, LP Rignanese, C Ripoli, A Rivetti, A Roberts, C Roberts, J Rode, G Rogers, L Romero, M Rossi, A Rubbia, MA Sabia, P Salomone, E Sandford, S Sanfilippo, D Santone, R Santorelli, C Savarese, E Scapparone, G Schillaci, FG Schuckman, G Scioli, M Simeone, P Skensved, MD Skorokhvatov, O Smirnov, T Smirnova, B Smith, F Spadoni, M Spangenberg, R Stefanizzi, A Steri, V Stornelli, S Stracka, M Stringer, S Sulis, A Sung, Y Suvorov, AM Szelc, R Tartaglia, A Taylor, J Taylor, S Tedesco, G Testera, K Thieme, TN Thorpe, A Tonazzo, A Tricomi, EV Unzhakov, T Vallivilayil John, M Van Uffelen, T Viant, S Viel, RB Vogelaar, J Vossebeld, M Wada, MB Walczak, H Wang, Y Wang, S Westerdale, L Williams, I Wingerter-Seez, R Wojaczynski, Ma M Wojcik, T Wright, Y Xie, C Yang, A Zabihi, P Zakhary, A Zani, A Zichichi, G Zuzel, MP Zykova, The DarkSide-20k Collaboration
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