{"paper":{"title":"Production Rate Measurement of Tritium and Other Cosmogenic Isotopes in Germanium with CDMSlite","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM","hep-ex","nucl-ex"],"primary_cat":"physics.ins-det","authors_text":"A.E. Robinson, A. Jastram, A. Kennedy, A. Kubik, A.N. Villano, A. Reisetter, A. Roberts, A. Scarff, B.A. Young, B. Cabrera, B. Cornell, B. Loer, B. Mohanty, B. Sadoulet, B. Serfass, B. von Krosigk, C. Cartaro, C. Jena, C.W. Fink, D.A. Bauer, D. Barker, D.G. Cerde\\~no, D.H. Wright, D. Jardin, D. MacDonell, D. Speller, D. Toback, E. Azadbakht, E. Fascione, E. Figueroa-Feliciano, E. Lopez Asamar, E. Miller, E.W. Hoppe, F. Ponce, G. Gerbier, H.A. Tanaka, H.E. Rogers, H. Qiu, H.R. Harris, I.J. Arnquist, J. Cooley, J.D. Morales Mendoza, J.L. Orrell, J. Nelson, J. Sander, J. Street, J.S. Wilson, J. Winchell, K. Senapati, L. Hsu, M.A. Bowles, M.E. Huber, M. Fritts, M. Ghaith, M.H. Kelsey, M.J. Wilson, M. Pepin, M. Pyle, M. Stein, N.A. Kurinsky, N. Mast, N. Mirabolfathi, P. Cushman, P.L. Brink, P. Lukens, R. Bunker, R. Calkins, R.E. Lawrence, R. Germond, R. Mahapatra, R. Partridge, R. Ren, R. Underwood, R.W. Schnee, S. Banik, S.L. Watkins, S.M. Oser, S. Poudel, S.R. Golwal, 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.-Y. Chang, Z. Hong","submitted_at":"2018-06-19T05:14:25Z","abstract_excerpt":"Future direct searches for low-mass dark matter particles with germanium detectors, such as SuperCDMS SNOLAB, are expected to be limited by backgrounds from radioactive isotopes activated by cosmogenic radiation inside the germanium. There are limited experimental data available to constrain production rates and a large spread of theoretical predictions. We examine the calculation of expected production rates, and analyze data from the second run of the CDMS low ionization threshold experiment (CDMSlite) to estimate the rates for several isotopes. We model the measured CDMSlite spectrum and fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.07043","kind":"arxiv","version":5},"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/1806.07043/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"}