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

165 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

Fingerprint

ASJC Scopus subject areas

Astronomy and Astrophysics

Cite this

Angloher, G., Bruckmayer, M., Bucci, C., Bühler, M., Cooper, S., Cozzini, C., ... 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.

@article{cfea2cf21e4444498421a4e6ec36381a,

title = "Limits on WIMP dark matter using sapphire cryogenic detectors",

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",

year = "2002",

month = "7",

day = "5",

doi = "10.1016/S0927-6505(02)00111-1",

language = "English",

volume = "18",

pages = "43--55",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

number = "1",

}

TY - JOUR

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

N2 - 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.

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.

UR - http://www.scopus.com/inward/record.url?scp=0036080154&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0036080154&partnerID=8YFLogxK

U2 - 10.1016/S0927-6505(02)00111-1

DO - 10.1016/S0927-6505(02)00111-1

M3 - Article

AN - SCOPUS:0036080154

VL - 18

SP - 43

EP - 55

JO - Astroparticle Physics

JF - Astroparticle Physics

SN - 0927-6505

IS - 1

ER -

Access to Document

10.1016/S0927-6505(02)00111-1