Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group

D. S. Akerib (Co-chair , Case Western Reserve University) , E. Aprile (Co-chair , Columbia University) , E. A. Baltz (Kavli Institute for Particle Astrophysics , Cosmology , SLAC) , M. R. Dragowsky (Case Western Reserve University)

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R. J. Gaitskell (Brown University) P. Gondolo (University of Utah) A. Hime (Los Alamos National Laboratory) C. J. Martoff (Temple University) D.-M. Mei (Los Alamos National Laboratory) H. Nelson (University of California Santa Barbara) B. Sadoulet (University of California Berkeley) R. W. Schnee (Case Western Reserve University) A. H. Sonnenschein (Fermi National Accelerator Laboratory) L. E. Strigari (University of California Irvine)

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keywords darkmatterdetectioncontextdeepdirectengineeringlaboratory

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A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the U.S. The table of contents follows: 1. Overview 2. WIMP Dark Matter: Cosmology, Astrophysics, and Particle Physics 3. Direct Detection of WIMPs 4. Indirect Detection of WIMPs 5. Dark Matter Candidates and New Physics in the Laboratory 6. Synergies with Other Sub-Fields 7. Direct Detection Experiments: Status and Future Prospects 8. Infrastructure 9. International Context 10. Summary and Outlook 11. Acknowledgments

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Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group

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