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 | |
| Publication status | Published - 5 Jul 2002 |
| Externally published | Yes |
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ASJC Scopus subject areas
- Astronomy and Astrophysics
Cite this
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
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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
VL - 18
SP - 43
EP - 55
JO - Astroparticle Physics
JF - Astroparticle Physics
SN - 0927-6505
IS - 1
ER -