Publikationsansicht

Limits on WIMP Dark Matter using Sapphire Cryogenic Detectors (2002)

Angloher,G.,
Bruckmayer,M.,
Bucci,C.,
Bühler,M.,
Cooper,S.,
Cozzini,C.,
Di Stefano,P.,
Von Feilitzsch,F.,
Frank,T.,
Hauff,D.,
Jagemann,Th.,
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.,
Stolsky,L.,
Wulandari,H.,
Zerle,L.

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.

Details der Publikation

Download	http://edoc.mpg.de/193926
Archiv	Max Planck Society - eDocument Server (Germany)
Typ	Article