{"paper":{"title":"Projected Sensitivity of the SuperCDMS SNOLAB experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"physics.ins-det","authors_text":"A. Borgland, A. E. Robinson, A. J. Anderson, A. Jastram, A. Kennedy, A. Kubik, A. Leder, A. N. Villano, A. Phipps, A. Reisetter, A. Roberts, B. A. Young, B. Cabrera, B. Cornell, B. Loer, B. Sadoulet, B. Serfass, B. von Krosigk, B. Welliver, C. Cartaro, D. A. Bauer, D. Barker, D. G. Cerde\\~no, D. Holmgren, D. H. Wright, D. Jardin, D. O. Caldwell, D. Speller, D. Toback, E. Figueroa-Feliciano, E. Hoppe, E. Lopez Asamar, G. Gerbier, G. L. Godfrey, H. A. Tanaka, H. Chagani, H. E. Rogers, H. Qiu, H. R. Harris, I. Arnquist, J. Cooley, J. D. Morales Mendoza, J. Hall, J. J. Yen, J. L. Orrell, J. Sander, J. Street, J. S. Wilson, K. Page, K. Schneck, L. Esteban, L. Hsu, M. A. Bowles, M. Daal, M. E. Huber, M. Fritts, M. Ghaith, M. H. Kelsey, M. Pepin, M. Pyle, M. Stein, N. A. Kurinsky, N. Mast, N. Mirabolfathi, P. C. F. Di Stefano, P. Cushman, P. L. Brink, P. Lukens, P. Redl, R. Agnese, R. A. Moffatt, R. Basu Thakur, R. Bunker, R. Calkins, R. Mahapatra, R. Partridge, R. Underwood, R. W. Schnee, S. Fallows, S. M. Oser, S. Poudel, S. R. Golwala, S. Yellin, T. Aramaki, T. Doughty, T. Hofer, T. Saab, V. Iyer, V. Mandic, W. A. Page, W. Baker, W. Rau, X. Zhang, X. Zhao, Y. Chen, Z. Hong","submitted_at":"2016-09-30T12:30:49Z","abstract_excerpt":"SuperCDMS SNOLAB will be a next-generation experiment aimed at directly detecting low-mass (< 10 GeV/c$^2$) particles that may constitute dark matter by using cryogenic detectors of two types (HV and iZIP) and two target materials (germanium and silicon). The experiment is being designed with an initial sensitivity to nuclear recoil cross sections ~ 1 x 10$^{-43}$ cm$^2$ for a dark matter particle mass of 1 GeV/c$^2$, and with capacity to continue exploration to both smaller masses and better sensitivities. The phonon sensitivity of the HV detectors will be sufficient to detect nuclear recoils"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.00006","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}