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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

Cresst-II: dark matter search with scintillating absorbers

NUCL INSTRUM METH A 520:1-3 (2004) 108-111

Authors:

G Angloher, C Bucci, C Cozzini, F von Feilitzsch, T Frank, D Hauff, S Henry, T Jagemann, J Jochum, H Kraus, B Majorovits, J Ninkovic, F Petricca, F Probst, Y Ramachers, W Rau, W Seidel, M Stark, S Uchaikin, L Stodolsky, H Wulandari

Abstract:

In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct weakly interacting massive particles (WIMP) detection. Nuclear recoils can be discriminated against electron recoils by measuring phonons and scintillation light simultaneously. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers. Results on the sensitivity of the phonon and the light channel, radiopurity, the scintillation properties of CaWO4, and on the WIMP sensitivity are presented. (C) 2003 Elsevier B.V. All rights reserved.

Multichannel SQUID readout for CRESST II

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 520 (2004) 588-591

Authors:

SA Henry, H. Kraus, B. Majorovits, Y. Ramachers

Direct WIMP detection with cryogenic detectors

PHILOS T ROY SOC A 361:1812 (2003) 2581-2590

Abstract:

Cryogenic detectors have been developed since the mid 1980s and have been applied successfully to dark-matter searches since the mid 1990s. Among the advantages of cryogenic detectors are their high sensitivity to nuclear recoil, their low detection thresholds, the wide choice of target materials and the possibility of implementing event type recognition on an event-by-event basis. I explain the basics of cryogenic detectors, review various implementations, discuss advantages and drawbacks and give an overview of current dark-matter-search experiments based upon cryogenic detectors.

Direct WIMP detection with cryogenic detectors.

Philos Trans A Math Phys Eng Sci 361:1812 (2003) 2581-2590

Abstract:

Cryogenic detectors have been developed since the mid 1980s and have been applied successfully to dark-matter searches since the mid 1990s. Among the advantages of cryogenic detectors are their high sensitivity to nuclear recoil, their low detection thresholds, the wide choice of target materials and the possibility of implementing event type recognition on an event-by-event basis. I explain the basics of cryogenic detectors, review various implementations, discuss advantages and drawbacks and give an overview of current dark-matter-search experiments based upon cryogenic detectors.

Limits on WIMP dark matter using sapphire cryogenic detectors

NUCL PHYS B-PROC SUP 124 (2003) 189-192

Authors:

J Jochum, G Angloher, C Bucci, S Cooper, C Cozzini, P DiStefano, F von Fellitzsch, T Frank, D Hauff, T Jagemann, R Keeling, H Kraus, M Loidl, O Meier, U Nagel, F Probst, Y Ramachers, A Rulofs, J Schnagl, W Seidel, I Sergeyev, M Sisti, M Stark, S Uchaikin, L Stodolsky, H Wulandari

Abstract:

Data taken by CRESST with a cryogenic detector system based on 262 g sapphire crystals has been used to place limits on WIMP dark matter. The experiment was especially sensitive for low-mass WIMPs with spin-dependent cross sections and improves on existing limits in this region.

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