{"paper":{"title":"Low-Mass Dark Matter Search with CDMSlite","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","hep-ex","physics.ins-det"],"primary_cat":"astro-ph.CO","authors_text":"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. Mohanty, B. Sadoulet, B. Serfass, B. von Krosigk, B. Welliver, C. Cartaro, C. Jena, D.A. Bauer, D. Balakishiyeva, D. Barker, D.G. Cerdeno, D.H. Wright, D. Jardin, D. MacDonell, D.O. Caldwell, D. Speller, D. Toback, E. Fascione, E. Figueroa-Feliciano, E.H. Miller, E. Lopez Asamar, E.W. Hoppe, G. Gerbier, G.L. Godfrey, H.A. Tanaka, H. Chagani, H.E. Rogers, H. Qiu, H.R. Harris, I.J. Arnquist, J. Cooley, J.D. Morales Mendoza, J. Hall, J.J. Yen, J.L. Orrell, J. Nelson, J. Sander, J. Street, J.S. Wilson, K. Page, K. Schneck, K. Senapati, L. Esteban, L. Hsu, M.A. Bowles, M. Daal, M.E. Huber, M. Fritts, M. Ghaith, M.H. Kelsey, M.J Wilson, M. Penalver Martinez, 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.A. Moffatt, R. Basu Thakur, R. Bunker, R. Calkins, R. Mahapatra, R. Partridge, R. Underwood, R.W. Schnee, S.M. Oser, S. Poudel, S.R. Golwala, S. Scorza, SuperCDMS Collaboration: R. Agnese, S. Yellin, T. Aralis, T. Aramaki, T. Binder, T. Doughty, T. Reynolds, T. Saab, V. Iyer, V. Mandic, W.A. Page, W. Baker, W. Rau, X. Zhang, X. Zhao, Y. Chang, Y. Chen, Z. Hong","submitted_at":"2017-07-06T04:30:52Z","abstract_excerpt":"The SuperCDMS experiment is designed to directly detect weakly interacting massive particles (WIMPs) that may constitute the dark matter in our Galaxy. During its operation at the Soudan Underground Laboratory, germanium detectors were run in the CDMSlite mode to gather data sets with sensitivity specifically for WIMPs with masses ${<}$10 GeV/$c^2$. In this mode, a higher detector-bias voltage is applied to amplify the phonon signals produced by drifting charges. This paper presents studies of the experimental noise and its effect on the achievable energy threshold, which is demonstrated to be"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.01632","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":""},"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"}