Author/Authors :
Wang، H. نويسنده , , Cline، D. نويسنده , , Curioni، A. نويسنده , , Lamarina، A. نويسنده , , Mannocchi، G. نويسنده , , Otwinowski، S. نويسنده , , Periale، L. نويسنده , , Periale، R. نويسنده , , Picchi، P. نويسنده , , Pietropaolo، F. نويسنده , , Woo، J. نويسنده ,
Abstract :
We describe an important new technique to search for WIMPs. This technique employs a method of background discrimination using double phase xenon as detector target. We describe the construction of a two-phase, I-kg xenon delector. The detector will be installed at the underground laboratory in the Mt. Blanc tunnel, which provides a low background rale. A comparison between the sensitivity curve of our detector and the theoretical events limit from SUSY calculations is presented.
Keywords :
Pulsars , Inverse CompTon scattering , Gamma-rays , Cherenkov telescopes: Pulsars , individual (PSR B1259 - 63, PSR J0045 - 73)