Measurement of the Forward-Backward Charge Asymmetry from W --> e nu Production in p anti-p Collisions at s**(1/2) = 1.96 TeV
ArXiv hep-ex/0501023 (2005)
Search for ZZ and ZW Production in ppbar Collisions at sqrt(s) = 1.96 TeV
ArXiv hep-ex/0501021 (2005)
CRESST cryogenic dark matter search
New Astronomy Reviews 49:2-6 SPEC. ISS. (2005) 255-258
Abstract:
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorbers for direct WIMP (weakly interactive massive particles) detection. The phonon signal in the CaWO4 crystal is registered in coincidence with the light signal, which is measured with a separate cryogenic light detector. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers (W-SPTs). As a result an active discrimination of the electron recoils against nuclear recoils is achieved. Results on the properties of the detector modules and on the WIMP sensitivity are presented. © 2005 Published by Elsevier B.V.Detector concepts
LCWS 2005 - 2005 International Linear Collider Workshop (2005)
Experimental determination of parton distributions
HERA and the LHC: A Workshop on the Implications of HERA for LHC Physics, HERA-LHC 2005 - Proceedings (2005) 78-118