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Beyond the CDMS-II Dark Matter Search: SuperCDMS

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arxiv astro-ph/0503583 v1 pith:2AGNB42W submitted 2005-03-28 astro-ph

P.L. Brink , B. Cabrera , C.L. Chang , J. Cooley , R.W. Ogburn , D.S. Akerib , C.N. Bailey , P.P. Brusov
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M.R. Dragowsky D.R. Grant R. Hennings-Yeomans R.W. Schnee M.J. Attisha R.J. Gaitskell J-P.F. Thompson L. Baudis T. Saab D.A. Bauer M.B. Crisler D. Holmgren E. Ramberg J. Yoo R. Bunker D.O. Caldwell R. Mahapatra H. Nelson J. Sander S. Yellin P. Cushman L. Duong A. Reisetter P. Denes A. Lu B. Sadoulet J. Filippini P. Meunier N. Mirabolfathi D.N. Seitz B. Serfass K.M. Sundqvist S.R. Golwala M.E. Huber K.D. Irwin B.A. Young
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keywords supercdmscdms-iidarkmattersearchsitewimpadvantage
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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 $10^{-46} - 10^{-44}$cm$^2$, 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 plan, identify primary issues, and set the goals that need to be met prior to embarking upon each phase of SuperCDMS.

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