Snowmass CF1 Summary: WIMP Dark Matter Direct Detection
By P. Cushman, C. Galbiati, D. McKinsey, H. Robertson, T. Tait, D. Bauer, A. Borgland, B. Cabrera, F. Calaprice, J. Cooley and 39 more. 2013
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Author(s): Cushman, P; Galbiati, C; McKinsey, DN; Robertson, H; Tait, TMP; Bauer, D; Borgland, A; Cabrera, B; Calaprice, F; Cooley, J; Empl, T; Essig, R; Figueroa-Feliciano, E; Gaitskell, R; Golwala, S; Hall, J; Hill, R; Hime, A; Hoppe, E; Hsu, L; Hungerford, E; Jacobsen, R; Kelsey, M; Lang, RF; Lippincott, WH; Loer, B; Luitz, S; Mandic, V; Mardon, J; Maricic, J; Maruyama, R; Mahapatra, R; Nelson, H; Orrell, J; Palladino, K; Pantic, E; Partridge, R; Ryd, A; Saab, T; Sadoulet, B; Schnee, R; Shepherd, W; Sonnenschein, A; Sorensen, P; Szydagis, M; Volansky, T; Witherell, M; Wright, D; Zurek, K | Abstract: As part of the Snowmass process, the Cosmic Frontier WIMP Direct Detection subgroup (CF1) has drawn on input from the Cosmic Frontier and the broader Particle Physics community to produce this document. The charge to CF1 was (a) to summarize the current status and projected sensitivity of WIMP direct detection experiments worldwide, (b) motivate WIMP dark matter searches over a broad parameter space by examining a spectrum of WIMP models, (c) establish a community consensus on the type of experimental program required to explore that parameter space, and (d) identify the common infrastructure required to practically meet those goals.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/2ab5584a05b674a0120cc033219948e2287c3909
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In Nuclear and High Energy Physics
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- Colloquium : Majorana fermions in nuclear, particle, and solid-state physics (2014, background): “The recent long-range planning process for high energy physics in the US has resulted in a number of nice reviews (Buckley et al., 2013; Cushman et al., 2013; Kusenko et al., 2013) detailing this program, and the review by Schumann (Schumann, 2013) ties the field together well in a short summary.”