Hans Kraus: Publications

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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CRESST DARK MATTER SEARCH

World Scientific Publishing (2003) 314-319

Authors:

C BUCCI, G ANGLOHER, C COZZINI, J DONCEV, T FRANK, D HAUFF, F PETRICCA, F PROEBST, W SEIDEL, L STODOLSKI, FV FEILITZSCH, T JAGEMANN, J JOCHUM, M STARK, H WULANDARI, N BAZIN, S HENRY, R KEELING, H KRAUS, Y RAMACHERS

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Dark matter search with CRESST cryogenic detectors

PHYS ATOM NUCL+ 66:3 (2003) 494-496

Authors:

G Angloher, M Altmann, M Bruckmayer, C Bucci, S Cooper, C Cozzini, P Di Stefano, F von Feilitzsch, T Frank, D Hauff, T Jagemann, J Jochum, R Keeling, H Kraus, J Macallister, F Probst, Y Ramachers, J Schnagl, W Seidel, I Sergeyev, M Stark, L Stodolsky, H Wulandari

Abstract:

Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire defectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. (C) 2003 MAIK "Nauka/Interperiodica".

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Limits on WIMP dark matter using sapphire cryogenic detectors

Astroparticle Physics 18 (2002) 43-55

Authors:

S Cooper, M Sisti, F Proebst, W Seidel

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Results of CRESST phase I

NUCL PHYS B-PROC SUP 110 (2002) 67-69

Authors:

F Probst, G Angloher, M Bruckmayer, C Bucci, S Cooper, P Di Stefano, F von Feilitzsch, T Frank, D Hauff, T Jagemann, J Jochum, R Keeling, H Kraus, J Marchese, Y Ramachers, J Schnagl, W Seidel, I Sergeyev, M Stark, L Stodolsky, H Wulandari

Abstract:

Results of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the galactic halo. The sapphire detectors are especially sensitive for low-mass WIMPS with spin-dependent interaction and improve on existing limits in this region.

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Hans Kraus

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Limits on WIMP dark matter using sapphire cryogenic detectors

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CRESST DARK MATTER SEARCH

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Dark matter search with CRESST cryogenic detectors

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Limits on WIMP dark matter using sapphire cryogenic detectors

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Results of CRESST phase I

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Hans Kraus

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Limits on WIMP dark matter using sapphire cryogenic detectors

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CRESST DARK MATTER SEARCH

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Dark matter search with CRESST cryogenic detectors

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Limits on WIMP dark matter using sapphire cryogenic detectors

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Results of CRESST phase I

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