Author/Authors :
Barnabé-Heider، نويسنده , , M. and Di Marco، نويسنده , , M. and Doane، نويسنده , , P. and Genest، نويسنده , , M.-H. and Gornea، نويسنده , , R. and Guénette، نويسنده , , Wayne R. and LeRoy، نويسنده , , Juan C. and Lessard، نويسنده , , L. and Martin، نويسنده , , J.-P. and Wichoski، نويسنده , , U. and Zacek، نويسنده , , V. and Clark، نويسنده , , K. W. Krauss، نويسنده , , C.B. and Noble، نويسنده , , A.J. and Behnke، نويسنده , , E. and Feighery، نويسنده ,
Abstract :
We present results of systematic studies of the radiation response of superheated liquid droplet detectors, which are used in the PICASSO dark matter search experiment. This detection technique is based on the phase transitions of superheated liquid Freon droplets dispersed and trapped in a polymerized gel. Phase transitions can be induced by nuclear recoils following particle interactions and, in particular, interactions with Weakly Interacting Massive Particles (WIMPs). These detectors are threshold devices since a minimal energy deposition is necessary to induce a phase transition and their sensitivity to various types of radiation depends strongly on the operating temperature and pressure. The sensitivity to neutrons, α-particles and γ-rays was determined as a function of these operating parameters and the results are compared with simulations. In particular, we present a complete characterization of the response of detector modules already in use for a dark matter search at the SNO site to detect WIMPs and discuss possible background sources.
Keywords :
alpha particles , Detectors , Superheated droplet detectors , Cold dark matter , neutrons