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

Hans Kraus

Professor of Physics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Particle Physics

Research groups

  • LUX-ZEPLIN
Hans.Kraus@physics.ox.ac.uk
Telephone: 01865 (2)73361
Denys Wilkinson Building, room 623
  • About
  • Publications

Towards an automated data cleaning with deep learning in CRESST

The European Physical Journal Plus Springer Nature 138:1 (2023) 100

Authors:

G Angloher, S Banik, D Bartolot, G Benato, A Bento, A Bertolini, R Breier, C Bucci, J Burkhart, L Canonica, A D’Addabbo, S Di Lorenzo, L Einfalt, A Erb, FV Feilitzsch, N Ferreiro Iachellini, S Fichtinger, D Fuchs, A Fuss, A Garai, VM Ghete, S Gerster, P Gorla, PV Guillaumon, S Gupta, D Hauff, M Ješkovský, J Jochum, M Kaznacheeva, A Kinast, H Kluck, H Kraus, M Lackner, A Langenkämper, M Mancuso, L Marini, L Meyer, V Mokina, A Nilima, M Olmi, T Ortmann, C Pagliarone, L Pattavina, F Petricca, W Potzel, P Povinec, F Pröbst, F Pucci, F Reindl, D Rizvanovic, J Rothe, K Schäffner, J Schieck, D Schmiedmayer, S Schönert, C Schwertner, M Stahlberg, L Stodolsky, C Strandhagen, R Strauss, I Usherov, F Wagner, M Willers, V Zema, W Waltenberger
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A next-generation liquid xenon observatory for dark matter and neutrino physics

Journal of Physics G Nuclear and Particle Physics IOP Publishing 50:1 (2022) 13001

Authors:

J Aalbers, Ss AbdusSalam, K Abe, V Aerne, F Agostini, S Ahmed Maouloud, Ds Akerib, Dy Akimov, J Akshat, Ak Al Musalhi, F Alder, Sk Alsum, L Althueser, Cs Amarasinghe, Fd Amaro, A Ames, Tj Anderson, B Andrieu, N Angelides, E Angelino, J Angevaare, Vc Antochi, D Antón Martin, B Antunovic, E Aprile, Hm Araújo, Je Armstrong, F Arneodo, M Arthurs, P Asadi, S Baek, X Bai, D Bajpai, A Baker, J Balajthy, S Balashov, M Balzer, A Bandyopadhyay, J Bang, E Barberio, Jw Bargemann, L Baudis, D Bauer, D Baur, A Baxter, Al Baxter, M Bazyk, K Beattie, J Behrens, Nf Bell

Abstract:

The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.
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Ultra-fast low temperature scintillation and X-ray luminescence of CsPbCl3 crystals

Journal of Materials Chemistry C Royal Society of Chemistry 11 (2022) 656-665

Authors:

Vb Mykhaylyk, M Rudko, H Kraus, V Kapustianyk, V Kolomiets, N Vitoratou, Y Chornodolskyy, As Voloshinovskii, L Vasylechko

Abstract:

Halide perovskites recently emerged as promising materials for the detection of ionising radiation. Single crystals of halide perovskites exhibit very fast and bright scintillation when cooled and may outperform the best modern scintillators at temperatures below 100 K. In this work we report on low-temperature scintillation properties of CsPbCl3 single crystals, grown using the Bridgeman method. The temperature dependences of the luminescence and decay kinetics were studied using X-ray excitation. At low temperatures, the crystal exhibits an intense narrow-band emission at about 420 nm with very fast decay kinetics. This emission, of which a characteristic feature is the strong thermal quenching, is attributed to the radiative decays of bound and trapped excitons. The fast, middle, and slow decay time constants obtained from a fit of a sum of exponential functions to the decay curve at 10 K are 0.1, 1 and 11 ns, respectively. The scintillation light yield of CsPbCl3 at 7 K measured at excitation with α-particles from an 241Am source is estimated to be 140 ± 15% of a reference LYSO-Ce crystal and 19000 ± 2000 ph per MeV under 14 keV X-ray excitation at 10 K. It is concluded that owing to a reduced amplitude of the slow decay component, CsPbCl3 exhibits an ultra-fast scintillation response that is superior to that of other halide perovskites. The combination of sub-nanosecond response time and the encouraging light yield has the potential of establishing this material as first choice for scintillation applications that rely on prompt detector response at cryogenic temperatures.

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Improving the Quality of CaWO4 Target Crystals for CRESST

Journal of Low Temperature Physics Springer Nature 209:5-6 (2022) 1128-1134

Authors:

A Kinast, G Angloher, G Benato, A Bento, A Bertolini, R Breier, C Bucci, L Canonica, A D’Addabbo, S Di Lorenzo, L Einfalt, A Erb, FV Feilitzsch, N Ferreiro Iachellini, S Fichtinger, D Fuchs, A Fuss, A Garai, V-M Ghete, P Gorla, S Gupta, F Hamilton, D Hauff, M Ješkovský, J Jochum, M Kaznacheeva, H Kluck, H Kraus, A Langenkämper, M Mancuso, L Marini, V Mokina, A Nilima, M Olmi, T Ortmann, C Pagliarone, V Palušová, L Pattavina, F Petricca, W Potzel, P Povinec, F Pröbst, F Pucci, F Reindl, J Rothe, K Schäffner, J Schieck, D Schmiedmayer, S Schönert, C Schwertner, M Stahlberg, L Stodolsky, C Strandhagen, R Strauss, I Usherov, F Wagner, M Willers, V Zema
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Background Determination for the LUX-ZEPLIN (LZ) Dark Matter Experiment

(2022)

Authors:

J Aalbers, DS Akerib, AK Al Musalhi, F Alder, SK Alsum, CS Amarasinghe, A Ames, TJ Anderson, N Angelides, HM Araújo, JE Armstrong, M Arthurs, A Baker, J Bang, JW Bargemann, A Baxter, K Beattie, P Beltrame, EP Bernard, A Bhatti, A Biekert, TP Biesiadzinski, HJ Birch, GM Blockinger, B Boxer, CAJ Brew, P Brás, S Burdin, M Buuck, R Cabrita, MC Carmona-Benitez, C Chan, A Chawla, H Chen, APS Chiang, NI Chott, MV Converse, A Cottle, G Cox, O Creaner, CE Dahl, A David, S Dey, L de Viveiros, C Ding, JEY Dobson, E Druszkiewicz, SR Eriksen, A Fan, NM Fearon, S Fiorucci, H Flaecher, ED Fraser, T Fruth, RJ Gaitskell, J Genovesi, C Ghag, R Gibbons, MGD Gilchriese, S Gokhale, J Green, MGD van der Grinten, CB Gwilliam, CR Hall, S Han, E Hartigan-O'Connor, SJ Haselschwardt, SA Hertel, G Heuermann, M Horn, DQ Huang, D Hunt, CM Ignarra, RG Jacobsen, O Jahangir, RS James, J Johnson, AC Kaboth, AC Kamaha, D Khaitan, I Khurana, R Kirk, D Kodroff, L Korley, EV Korolkova, H Kraus, S Kravitz, L Kreczko, B Krikler, VA Kudryavtsev, EA Leason, J Lee, DS Leonard, KT Lesko, C Levy, J Lin, A Lindote, R Linehan, WH Lippincott, X Liu, MI Lopes, E Lopez Asamar, B López Paredes, W Lorenzon, C Lu, S Luitz, PA Majewski, A Manalaysay, RL Mannino, N Marangou, ME McCarthy, DN McKinsey, J McLaughlin, EH Miller, E Mizrachi, A Monte, ME Monzani, JD Morales Mendoza, E Morrison, BJ Mount, M Murdy, A St J Murphy, D Naim, A Naylor, C Nedlik, HN Nelson, F Neves, A Nguyen, JA Nikoleyczik, I Olcina, KC Oliver-Mallory, J Orpwood, KJ Palladino, J Palmer, N Parveen, SJ Patton, B Penning, G Pereira, E Perry, T Pershing, A Piepke, D Porzio, S Poudel, Y Qie, J Reichenbacher, CA Rhyne, Q Riffard, GRC Rischbieter, HS Riyat, R Rosero, P Rossiter, T Rushton, D Santone, ABMR Sazzad, RW Schnee, S Shaw, T Shutt, JJ Silk, C Silva, G Sinev, R Smith, M Solmaz, VN Solovov, P Sorensen, J Soria, I Stancu, A Stevens, K Stifter, B Suerfu, TJ Sumner, N Swanson, M Szydagis, R Taylor, WC Taylor, DJ Temples, PA Terman, DR Tiedt, M Timalsina, Z Tong, DR Tovey, J Tranter, M Trask, M Tripathi, DR Tronstad, W Turner, U Utku, AC Vaitkus, A Wang, JJ Wang, W Wang, Y Wang, JR Watson, RC Webb, TJ Whitis, M Williams, FLH Wolfs, S Woodford, D Woodward, CJ Wright, Q Xia, X Xiang, J Xu, M Yeh
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