Results and plans of the CRESST dark matter search

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dc.creatorAltmann, M.
dc.creatorAngloher, G.
dc.creatorBruckmayer, M.
dc.creatorBucci, C.
dc.creatorCooper, S.
dc.creatorCozzini, C.
dc.creatorDiStefano, P.
dc.creatorvon Feilitzsch, F.
dc.creatorFrank, T.
dc.creatorHauff, D.
dc.creatorJagemann, Th.
dc.creatorJochum, J.
dc.creatorKeeling, R.
dc.creatorKraus, H.
dc.creatorMacallister, J.
dc.creatorProebst, F.
dc.creatorRamachers, Y.
dc.creatorSchnagl, J.
dc.creatorSeidel, W.
dc.creatorSergeyev, I.
dc.creatorStark, M.
dc.creatorStodolsky, L.
dc.creatorWulandari, H.
dc.date2001-06-18
dc.date.accessioned2026-07-07T01:58:58Z
dc.date.available2026-07-07T01:58:58Z
dc.descriptionData taken by CRESST in 2000 with a cryogenic detector system based on 262 g sapphire crystals is used to place limits on WIMP dark matter in the Galactic Halo. The detector is especially sensitive for low-mass WIMPS with spin-dependent cross sections and improves on existing limits in this region. CRESST is now preparing for a second phase, which will use a 10 kg detector consisting of 300 g CaWO4 crystals with simultaneous detection of phonons and scintillation light to reduce background.
dc.description23 pages, 15 figures, Paper contributed to the X International Symposium on Lepton and Photon Interactions at High Energies, 23rd-28th July 2001, Rome, Italy
dc.identifierhttps://arxiv.org/abs/astro-ph/0106314
dc.identifierhttp://arxiv.org/abs/astro-ph/0106314
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2924
dc.subjectAstrophysics
dc.titleResults and plans of the CRESST dark matter search
dc.typetext

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