{"paper":{"title":"A Strategy for Low-Mass Dark Matter Searches with Cryogenic Detectors in the SuperCDMS SNOLAB Facility","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.IM","hep-ex","nucl-ex"],"primary_cat":"physics.ins-det","authors_text":"A. E. Robinson, A. Jastram, A. J. Mayer, A. Kubik, A. Li, A. N. Villano, A. Pradeep, A. Roberts, A. Sattari, A. Zaytsev, B. A. Hines, B. A. Young, B. Cabrera, B. Loer, B. Mohanty, B. Sadoulet, B. Schmidt, B. Serfass, B. von Krosigk, B. Zatschler, C. Bathurst, C. Cartaro, C. Stanford, C. W. Fink, D. A. Bauer, D. B. MacFarlane, D. G. Cerdeno, D.J. Sincavage, D. S. Pedreros, D. Toback, D. W. P. Amaral, E. Azadbakht, E. Fascione, E. Figueroa-Feliciano, E. Michaud, E. Michielin, E. Reid, E. W. Hoppe, E. Zhang, F. De Brienne, F. K. Thasrawala, F. Ponce, G. Gerbier, H. Coombes, H. Meyer zu Theenhausen, H. Neog, H. Sun, I. Alkhatib, I. Ataee Langroudy, I. J. Arnquist, I. Saikia, J. Cooley, J. Corbett, J. Hall, J. Liu, J. L. Orrell, J. Nelson, J. Sander, J. Street, J. Winchell, K. Fouts, K. Wyko, L. Hsu, L. Zheng, M. Chaudhuri, M. D. Diamond, M.D. Osborne, M. E. Huber, M. Fritts, M. Ghaith, M. H. Kelsey, M. I. Hollister, M.J. Wilson, M. L. di Vacri, M. Lee, M. Pyle, N. A. Kurinsky, N. Chott, N. Hassan, N. Mast, N. Mirabolfathi, O. Wen, P. Cushman, P. L. Brink, P. Lukens, R. A. Cameron, R. Bhattacharyya, R. Bunker, R. Calkins, R. Chen, R. E. Lawrence, R. Germond, R. Mahapatra, R. Partridge, R. Podviianiuk, R. Ren, R. Underwood, R. W. Schnee, S. Banik, S. Dharani, S. L. Watkins, S. M. Oser, S. Nagorny, S. Poudel, S. R. Golwala, S. Scorza, S. S. Poudel, SuperCDMS Collaboration: M.F. Albakry, S. Verma, S. Yellin, S. Zatschler, S. Zuber, T. Aralis, T. Aramaki, T. C. Yu, T. Reynolds, T. Saab, V. Iyer, V. K. S. Kashyap, V. Mandic, V. Novati, W.A. Page, W. Rau, Y. Liu, Y. -Y. Chang, Z. Hong, Z. Williams","submitted_at":"2022-03-16T08:43:18Z","abstract_excerpt":"The SuperCDMS Collaboration is currently building SuperCDMS SNOLAB, a dark matter search focused on nucleon-coupled dark matter in the 1-5 GeV/c$^2$ mass range. Looking to the future, the Collaboration has developed a set of experience-based upgrade scenarios, as well as novel directions, to extend the search for dark matter using the SuperCDMS technology in the SNOLAB facility. The experienced-based scenarios are forecasted to probe many square decades of unexplored dark matter parameter space below 5 GeV/c$^2$, covering over 6 decades in mass: 1-100 eV/c$^2$ for dark photons and axion-like p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.08463","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2203.08463/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}