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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

Measurement of the gamma ray background in the Davis cavern at the Sanford Underground Research Facility

Astroparticle Physics Elsevier 116:March 2020 (2019) 102391

Authors:

Ds Akerib, Cw Akerlof, Sk Alsum, Ke Boast, C Carels, A Cottle, T Fruth

Abstract:

Deep underground environments are ideal for low background searches due to the attenuation of cosmic rays by passage through the earth. However, they are affected by backgrounds from γ-rays emitted by 40K and the 238U and 232Th decay chains in the surrounding rock. The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a liquid xenon TPC located within the Davis campus at the Sanford Underground Research Facility, Lead, South Dakota, at the 4850-foot level. In order to characterise the cavern background, in-situ γ-ray measurements were taken with a sodium iodide detector in various locations and with lead shielding. The integral count rates (0–3300 keV) varied from 596 Hz to 1355 Hz for unshielded measurements, corresponding to a total flux from the cavern walls of 1.9 ± 0.4 γ cm−2s−1. The resulting activity in the walls of the cavern can be characterised as 220 ± 60 Bq/kg of 40K, 29 ± 15 Bq/kg of 238U, and 13 ± 3 Bq/kg of 232Th.
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Low temperature scintillation properties of Ga2O3

Applied Physics Letters AIP Publishing 115:8 (2019) 081103

Authors:

VB Mykhaylyk, Hans Kraus, V Kapustianyk, M Rudko

Abstract:

Gallium oxide has recently been identified as a promising scintillator. To assess its potential as a detector material for ionizing radiation at low temperatures, we measured the luminescence and scintillation properties of an undoped Ga2O3 crystal over the 7–295 K temperature range. The emission of the crystal is due to the radiative decay of self-trapped excitons and donor-acceptor pairs and peaks at a wavelength of 380 nm. The scintillation light output of the undoped Ga2O3 increases with a decrease in temperature, reaching a maximum value of 19 300 ± 2200 ph/MeV at 50 K. The measured luminescence kinetics has a recombination character with specific decay time (τ0.1) increasing from 1 to 1.8 μs at cooling. Since radiative decay in the crystal competes with nonradiative processes, material optimization could lead to the scintillator achieving a yield of 40800 ph/MeV, a figure considered to be an upper limit.
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First results on sub-GeV spin-dependent dark matter interactions with 7Li

European Physical Journal C Springer Nature 79:7 (2019) 630

Authors:

AH Abdelhameed, G Angloher, P Bauer, A Bento, E Bertoldo, C Bucci, L Canonica, A D’Addabbo, X Defay, S Di Lorenzo, A Erb, FV Feilitzsch, N Ferreiro Iachellini, S Fichtinger, A Fuss, P Gorla, D Hauff, J Jochum, A Kinast, H Kluck, H Kraus, A Langenkämper, M Mancuso, V Mokina, E Mondragon, A Münster, M Olmi, T Ortmann, C Pagliarone, L Pattavina, F Petricca, W Potzel, F Pröbst, F Reindl, J Rothe, K Schäffner, J Schieck, V Schipperges, D Schmiedmayer, S Schönert, C Schwertner, M Stahlberg, L Stodolsky, C Strandhagen, R Strauss, C Türkoğlu, I Usherov, M Willers, V Zema, M Chapellier, A Giuliani, C Nones, DV Poda, VN Shlegel, M Velázquez, AS Zolotarova
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Bright and fast scintillation of organolead perovskite MAPbBr₃ at low temperatures

Materials Horizons Royal Society of Chemistry (2019)

Authors:

V Mykhaylyk, Hans Kraus, M Saliba

Abstract:

We report the excellent scintillation properties of MAPbBr3, an organic–inorganic trihalide perovskite (OTP). The characteristic scintillation time constants were determined using pulsed monochromatic 14 keV X-rays from a synchrotron. We find that between 50 and 130 K the MAPbBr3 crystal exhibits a very fast and intense scintillation response, with the fast (τf) and slow (τs) decay components reaching 0.1 and 1 ns, respectively. The light yield of MAPbBr3 is estimated to be 90 000 ± 18 000 ph MeV−1 at 77 K and 116 000 ± 23 000 ph MeV−1 at 8 K.
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Measurement of the Gamma Ray Background in the Davis Cavern at the Sanford Underground Research Facility

(2019)

Authors:

DS Akerib, CW Akerlof, SK Alsum, N Angelides, HM Araújo, JE Armstrong, M Arthurs, X Bai, J Balajthy, S Balashov, A Baxter, EP Bernard, A Biekert, TP Biesiadzinski, KE Boast, B Boxer, P Brás, JH Buckley, VV Bugaev, S Burdin, JK Busenitz, C Carels, DL Carlsmith, MC Carmona-Benitez, M Cascella, C Chan, A Cole, A Cottle, JE Cutter, CE Dahl, L de Viveiros, JEY Dobson, E Druszkiewicz, TK Edberg, A Fan, S Fiorucci, H Flaecher, T Fruth, RJ Gaitskell, J Genovesi, C Ghag, MGD Gilchriese, S Gokhale, MGD van der Grinten, CR Hall, S Hans, J Harrison, SJ Haselschwardt, SA Hertel, JY-K Hor, M Horn, DQ Huang, CM Ignarra, O Jahangir, W Ji, J Johnson, AC Kaboth, K Kamdin, D Khaitan, A Khazov, WT Kim, CD Kocher, L Korley, EV Korolkova, J Kras, H Kraus, SW Kravitz, L Kreczko, B Krikler, VA Kudryavtsev, EA Leason, J Lee, DS Leonard, KT Lesko, C Levy, J Li, J Liao, F-T Liao, J Lin, A Lindote, R Linehan, WH Lippincott, R Liu, X Liu, C Loniewski, MI Lopes, B López Paredes, W Lorenzon, S Luitz, JM Lyle, PA Majewski, A Manalaysay, L Manenti, RL Mannino, N Marangou, MF Marzioni, DN McKinsey, J McLaughlin, Y Meng, EH Miller, ME Monzani, JA Morad, E Morrison, BJ Mount, A St J Murphy, D Naim, A Naylor, C Nedlik, C Nehrkorn, HN Nelson, F Neves, J Nikoleyczik, A Nilima, I Olcina, KC Oliver-Mallory, S Pal, KJ Palladino, EK Pease, BP Penning, G Pereira, A Piepke, K Pushkin, J Reichenbacher, CA Rhyne, Q Riffard, GRC Rischbieter, JP Rodrigues, R Rosero, P Rossiter, G Rutherford, ABMR Sazzad, RW Schnee, M Schubnell, PR Scovell, D Seymour, S Shaw, TA Shutt, JJ Silk, C Silva, M Solmaz, VN Solovov, P Sorensen, I Stancu, A Stevens, TM Stiegler, K Stifter, M Szydagis, WC Taylor, R Taylor, D Temples, PA Terman, DR Tiedt, M Timalsina, A Tomás, M Tripathi, L Tvrznikova, U Utku, S Uvarov, A Vacheret, JJ Wang, JR Watson, RC Webb, RG White, TJ Whitis, FLH Wolfs, D Woodward, J Yin
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