Title of article
Installation of the cryogenic dark matter search (CDMS)
Author/Authors
Barnes Jr.، نويسنده , , P.D and Da Silva، نويسنده , , A and Akerib، نويسنده , , D.S. and Bauer، نويسنده , , D and Brink، نويسنده , , P and Cabrera، نويسنده , , B and Caldwell، نويسنده , , D.O and Chugg، نويسنده , , B and Clarke، نويسنده , , R.M and Cummings، نويسنده , , A and Davies، نويسنده , , A and Diaz، نويسنده , , R.C and Dougherty، نويسنده , , B.L and Emes، نويسنده , , Golwala، نويسنده , , S.R and Hale، نويسنده , , D and Haller، نويسنده , , E.E، نويسنده ,
Pages
4
From page
233
To page
236
Abstract
We discuss the status of a cryogenic dark matter search beginning operation in the Stanford Underground Facility. The detectors will be cooled in a specially designed cryostat connected to a modified side access Oxford 400 dilution refrigerator. We discuss two detector designs and performance, the cryostat construction and operation, and the multi-level shield surrounding the cryostat. Finally, we will examine the limits which we will be able to set on WIMP dark matter with this experiment.
Journal title
Astroparticle Physics
Record number
1997103
Link To Document