Limits on WIMP dark matter using sapphire cryogenic detectors

G. Angloher, M. Bruckmayer, C. Bucci, M. Bühler, S. Cooper, C. Cozzini, P. DiStefano, F. Von Feilitzsch, T. Frank, D. Hauff, T. Jagemann, J. Jochum, V. Jörgens, R. Keeling, H. Kraus, M. Loidl, J. Marchese, O. Meier, U. Nagel, F. PröbstY. Ramachers, A. Rulofs, J. Schnagl, W. Seidel, I. Sergeyev, M. Sisti, M. Stark, S. Uchaikin, L. Stodolsky, H. Wulandari, L. Zerle

Research output: Contribution to journal › Article

166 Citations (Scopus)

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 in the Galactic Halo. The experiment was especially sensitive for low-mass WIMPs with spin-dependent cross sections and improves on existing limits in this region.

Original language	English
Pages (from-to)	43-55
Number of pages	13
Journal	Astroparticle Physics
Volume	18
Issue number	1
DOIs	https://doi.org/10.1016/S0927-6505(02)00111-1
Publication status	Published - 5 Jul 2002
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics

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10.1016/S0927-6505(02)00111-1

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Angloher, G., Bruckmayer, M., Bucci, C., Bühler, M., Cooper, S., Cozzini, C., DiStefano, P., Von Feilitzsch, F., Frank, T., Hauff, D., Jagemann, T., Jochum, J., Jörgens, V., Keeling, R., Kraus, H., Loidl, M., Marchese, J., Meier, O., Nagel, U., ... Zerle, L. (2002). Limits on WIMP dark matter using sapphire cryogenic detectors. Astroparticle Physics, 18(1), 43-55. https://doi.org/10.1016/S0927-6505(02)00111-1

Limits on WIMP dark matter using sapphire cryogenic detectors. / Angloher, G.; Bruckmayer, M.; Bucci, C.; Bühler, M.; Cooper, S.; Cozzini, C.; DiStefano, P.; Von Feilitzsch, F.; Frank, T.; Hauff, D.; Jagemann, T.; Jochum, J.; Jörgens, V.; Keeling, R.; Kraus, H.; Loidl, M.; Marchese, J.; Meier, O.; Nagel, U.; Pröbst, F.; Ramachers, Y.; Rulofs, A.; Schnagl, J.; Seidel, W.; Sergeyev, I.; Sisti, M.; Stark, M.; Uchaikin, S.; Stodolsky, L.; Wulandari, H.; Zerle, L.

In: Astroparticle Physics, Vol. 18, No. 1, 05.07.2002, p. 43-55.

Research output: Contribution to journal › Article

Angloher, G, Bruckmayer, M, Bucci, C, Bühler, M, Cooper, S, Cozzini, C, DiStefano, P, Von Feilitzsch, F, Frank, T, Hauff, D, Jagemann, T, Jochum, J, Jörgens, V, Keeling, R, Kraus, H, Loidl, M, Marchese, J, Meier, O, Nagel, U, Pröbst, F, Ramachers, Y, Rulofs, A, Schnagl, J, Seidel, W, Sergeyev, I, Sisti, M, Stark, M, Uchaikin, S, Stodolsky, L, Wulandari, H & Zerle, L 2002, 'Limits on WIMP dark matter using sapphire cryogenic detectors', Astroparticle Physics, vol. 18, no. 1, pp. 43-55. https://doi.org/10.1016/S0927-6505(02)00111-1

Angloher, G. ; Bruckmayer, M. ; Bucci, C. ; Bühler, M. ; Cooper, S. ; Cozzini, C. ; DiStefano, P. ; Von Feilitzsch, F. ; Frank, T. ; Hauff, D. ; Jagemann, T. ; Jochum, J. ; Jörgens, V. ; Keeling, R. ; Kraus, H. ; Loidl, M. ; Marchese, J. ; Meier, O. ; Nagel, U. ; Pröbst, F. ; Ramachers, Y. ; Rulofs, A. ; Schnagl, J. ; Seidel, W. ; Sergeyev, I. ; Sisti, M. ; Stark, M. ; Uchaikin, S. ; Stodolsky, L. ; Wulandari, H. ; Zerle, L. / Limits on WIMP dark matter using sapphire cryogenic detectors. In: Astroparticle Physics. 2002 ; Vol. 18, No. 1. pp. 43-55.

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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 in the Galactic Halo. 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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AU - Angloher, G.

AU - Bruckmayer, M.

AU - Bucci, C.

AU - Bühler, M.

AU - Cooper, S.

AU - Cozzini, C.

AU - DiStefano, P.

AU - Von Feilitzsch, F.

AU - Frank, T.

AU - Hauff, D.

AU - Jagemann, T.

AU - Jochum, J.

AU - Jörgens, V.

AU - Keeling, R.

AU - Kraus, H.

AU - Loidl, M.

AU - Marchese, J.

AU - Meier, O.

AU - Nagel, U.

AU - Pröbst, F.

AU - Ramachers, Y.

AU - Rulofs, A.

AU - Schnagl, J.

AU - Seidel, W.

AU - Sergeyev, I.

AU - Sisti, M.

AU - Stark, M.

AU - Uchaikin, S.

AU - Stodolsky, L.

AU - Wulandari, H.

AU - Zerle, L.

PY - 2002/7/5

Y1 - 2002/7/5

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