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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

Signals induced by charge-trapping in EDELWEISS FID detectors: analytical modeling and applications

Journal of Instrumentation Institute of Physics 11:10 (2016) P10008

Authors:

Quentin Arnaud, Eric Armengaud, Corinne Augier, Alain Benoît, Laurent Bergé, Julien Billard, Johannes Blümer, Thibault de Boissière, Alex Broniatowski, Philippe Camus, Antoine Cazes, Maurice Chapellier, Florence Charlieux, Louis Dumoulin, Klaus Eitel, Nadine Foerster, Nicolas Fourches, Jules Gascon, Andrea Giuliani, Michel Gros, Lukas Hehn, Geertje Heuermann, Maryvonne de Jésus, JunSong Lin, Alex Juillard, Matthias Kleifges, Valentin Kozlov, Hans Kraus, Cecile Kéfélian, Vitaly A Kudryavtsev, Helène Le-Sueur, Stefanos Marnieros, Xavier-Francois Navick, Claudia Nones, Emiliano Olivieri, Patrick Pari, Bernard Paul, Marie-Cécile Piro, Denys Poda, Emiline Queguiner, Sergey Rozov, Véronique Sanglard, Benjamin Schmidt, Silvia Scorza, Bernhard Siebenborn, Denis Tcherniakhovski, Lionel Vagneron, Marc Weber, Evgeny Yakushev

Abstract:

The EDELWEISS-III experiment uses cryogenic HP-Ge detectors Fully covered with Inter-Digitized electrodes (FID). They are operated at low fields (< 1 V=cm), and as a consequence charge-carrier trapping significantly affects both the ionization and heat energy measurements. This paper describes an analytical model of the signals induced by trapped charges in FID detectors based on the Shockley-Ramo theorem. It is used to demonstrate that veto electrodes, initially designed for the sole purpose of surface event rejection, can be used to provide a sensitivity to the depth of the energy deposits, characterize the trapping in the crystals, perform heat and ionization energy corrections and improve the ionization baseline resolutions. These procedures are applied successfully to actual data.

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New limits on double electron capture of 40 Ca and 180 W

Journal of Physics G: Nuclear and Particle Physics Institute of Physics 43:9 (2016) 095202

Authors:

Godehard Angloher, Matthias Bauer, Philipp Bauer, Irina Bavykina, Antonio CSSM Bento, Carlo Bucci, Lucia Canonica, Christian Ciemniak, Xavier Defay, Gerhard Deuter, Andreas Erb, Franz von Feilitzsch, Nahuel Ferreiro Iachellini, Achim Gütlein, Christian Isaila, Margit Kiefer, Hans Kraus, Franz Pröbst, Sabine Roth, Christian Sailer, Anja Tanzke, Thi-Hieu Ho, Andreas Ulrich, Michael Willers, Mark Wüstrich

Abstract:

We analyzed low-background data from the CRESST-II experiment with a total net exposure of 730 kg days to extract limits on double electron capture processes. We established new limits for 40Ca with T1/22v2K > 9.9 × 1021 y and T1/20v2EC > 1.4 × 1022 y and for 180W T1/22v/2K > 3.1 × 1019 with y and T1/20v2ED > 9.4 × 1018 y at 90% CL. Depending on the process, these values improve the currently best limits by a factor of ∼1.4-30.
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The CRESST-III low-mass WIMP detector

Journal of Physics: Conference Series Institute of Physics 718:4 (2016) 042048

Authors:

Godehard Angloher, Antonio Bento, Carlo Bucci, Lucia Canonica, Xavier Defay, Andreas Erb, Franz von Feilitzsch, Nahuel Ferreiro Iachellini, Paolo Gorla, Achim Gütlein, Dieter Hauff, Josef Jochum, Margit Kiefer, Holger Kluck, Hans Kraus, Jean-Come Lanfranchi, Jurek Loebell, Andrea Münster, Carmine Pagliarone, Federica Petricca, Christian Strandhagen, Anja Tanzke, Hong H Trinh Thi, Cenk Türkoğlu, Martin Uffinger

Abstract:

The next generation direct dark matter experiment CRESST-III has a high potential to significantly increase the sensitivity to low-mass WIMPs (mx ≲10 GeV/c2). We present the new CRESST detector module: it consists of a 24 g CaWO4 crystal operated as a phonon detector and a 20x20 mm^2 silicon-on-sapphire light detector. The phonon energy threshold is lowered to ~100 eV and a light detector resolution of typically 5 eV is achieved. A fully-scintillating inner detector housing is realised which efficiently rejects events from surface alpha decays. The CaWO4 sticks holding the target crystal are also operated as calorimeters to discriminate all possible artefacts related to the support structure. A projection for the sensitivity to spin-independent WIMP-nucleon scattering is given for the first phase of CRESSTIII which will start beginning of 2016.
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Exploring Low-Mass Dark Matter with CRESST

Journal of Low Temperature Physics Springer Nature 184:3-4 (2016) 866-872

Authors:

R Strauss, G Angloher, A Bento, C Bucci, L Canonica, X Defay, A Erb, FV Feilitzsch, N Ferreiro Iachellini, P Gorla, A Gütlein, D Hauff, J Jochum, M Kiefer, H Kluck, H Kraus, JC Lanfranchi, J Loebell, A Münster, C Pagliarone, F Petricca, W Potzel, F Pröbst, F Reindl, K Schäffner, J Schieck, S Schönert, W Seidel, L Stodolsky, C Strandhagen, A Tanzke, HH Trinh Thi, C Türkoglu, M Uffinger, A Ulrich, I Usherov, S Wawoczny, M Willers, M Wüstrich, A Zöller
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Improved EDELWEISS-III sensitivity for low-mass WIMPs using a profile likelihood approach

(2016)

Authors:

EDELWEISS Collaboration, L Hehn, E Armengaud, Q Arnaud, C Augier, A Benoît, L Bergé, J Billard, J Blümer, T de Boissière, A Broniatowski, P Camus, A Cazes, M Chapellier, F Charlieux, M De Jésus, L Dumoulin, K Eitel, N Foerster, J Gascon, A Giuliani, M Gros, G Heuermann, Y Jin, A Juillard, C Kéfélian, M Kleifges, V Kozlov, H Kraus, VA Kudryavtsev, H Le-Sueur, S Marnieros, X-F Navick, C Nones, E Olivieri, P Pari, B Paul, M-C Piro, D Poda, E Queguiner, S Rozov, V Sanglard, B Schmidt, S Scorza, B Siebenborn, D Tcherniakhovski, L Vagneron, M Weber, E Yakushev
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