Abstract
Presently the CDMS-II collaboration's Weakly Interacting Massive Particle (WIMP) search at the Soudan Underground Laboratory sets the most stringent exclusion limits of any WIMP cold dark matter direct-detection experiment. To extend our reach further, to WIMP-nucleon cross-sections in the range 10- 46 - 10- 44 cm2, we propose SuperCDMS, which would take advantage of a very deep site. One promising site is the recently approved SNOLab facility in Canada. In this paper we will present our overall program and focus on phase A of SuperCDMS.
Original language | English |
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Pages (from-to) | 411-413 |
Number of pages | 3 |
Journal | Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |
Volume | 559 |
Issue number | 2 |
DOIs | |
Publication status | Published - Apr 14 2006 |
Externally published | Yes |
Bibliographical note
Funding Information:This work is supported by the National Science Foundation (NSF) under Grant no. AST-9978911, by the Department of Energy under contracts DE-AC03-76SF00098, DE-FG03-90ER40569, DE-FG03-91ER40618, and by Fermilab, operated by the Universities Research Association, Inc., under Contract no. DE-AC02-76CH03000 with the Department of Energy. The ZIP detectors are fabricated in the Stanford Nanofabrication Facility (which is a member of the National Nanofabrication Infrastructure Network sponsored by NSF under Grant ECS-0335765). In addition, seed funding for SuperCDMS detector development has been provided at Stanford by the KIPAC Enterprise Fund, the Dean of Research, and a Center for Integrated Systems Internal Grant.
ASJC Scopus Subject Areas
- Nuclear and High Energy Physics
- Instrumentation
Keywords
- Cold dark matter
- Underground astrophysics