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 › peer-review

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 › peer-review

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.",

author = "G. Angloher and M. Bruckmayer and C. Bucci and M. B{\"u}hler and S. Cooper and C. Cozzini and P. DiStefano and {Von Feilitzsch}, F. and T. Frank and D. Hauff and T. Jagemann and J. Jochum and V. J{\"o}rgens and R. Keeling and H. Kraus and M. Loidl and J. Marchese and O. Meier and U. Nagel and F. Pr{\"o}bst and Y. Ramachers and A. Rulofs and J. Schnagl and W. Seidel and I. Sergeyev and M. Sisti and M. Stark and S. Uchaikin and L. Stodolsky and H. Wulandari and L. Zerle",

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T1 - Limits on WIMP dark matter using sapphire cryogenic detectors

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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AB - 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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Limits on WIMP dark matter using sapphire cryogenic detectors

Abstract

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