Limits on WIMP dark matter using scintillating CaWO4 cryogenic detectors with active background suppression

Astroparticle Physics

Volumn 23, Issue 3, 2005, Pages 325-339

  Angloher, G ^a   Bucci, C ^d   Christ, P ^a   Cozzini, C ^b   von Feilitzsch, F ^c   Hauff, D ^a   Henry, S ^b   Jagemann, Th ^c   Jochum, J ^e   Kraus, H ^b   Majorovits, B ^b   Ninkovic, J ^a   Petricca, F ^a   Potzel, W ^c   Probst F ^a   Ramachers, Y ^b,f   Razeti, M ^c   Rau, W ^c   Seidel, W ^a   Stark, M ^c   Stodolsky, L ^a   Tolhurst, A J B ^b   Westphal, W ^c   Wulandari, H ^c   more..

^a MAX PLANCK INSTITUT FÜR PHYSIK   (Germany)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c TECHNICAL UNIVERSITY OF MUNICH   (Germany)

^d LABORATORI NAZIONALI DEL GRAN SASSO   (Italy)

^e UNIVERSITY OF TÜBINGEN   (Germany)

^f UNIVERSITY OF WARWICK   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

CRYOGENICS; ELEMENTARY PARTICLES; EXTRATERRESTRIAL ATMOSPHERES; GALAXIES; HIGH ENERGY PHYSICS; PARTICLE DETECTORS; PHONONS; SCINTILLATION COUNTERS;

BACKGROUND DISCRIMINATION; DARK MATTER; LOW TEMPERATURE DETECTORS; WEAKLY INTERACTING MASSIVE PARTICLE (WIMP);

ASTROPHYSICS;

EID: 20144365141     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.astropartphys.2005.01.006     Document Type: Article

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