{"paper":{"title":"Tests of Lorentz invariance at the Sudbury Neutrino Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"hep-ex","authors_text":"A. Bellerive, A. B. McDonald, A. E. Anthony, A. Hime, A. J. Noble, A. Kruger, A. Latorre, A. L. Hallin, A. Mastbaum, A. W. P. Poon, A. Wright, B. A. VanDevender, B. Beltran, B. Cai, B. C. Robertson, B. G. Nickel, B. Jamieson, B. J. Land, B. L. Wall, B. Monreal, B. T. Cleveland, C. B. Krauss, C. C. M. Kyba, C. E. Okada, C. Howard, C. J. Virtue, C. Kefelian, C. Kraus, D. Chauhan, D. L. Wark, D. Sinclair, D. Waller, E. Blucher, E. D. Hallman, E. Guillian, E. J. Callaghan, E. W. Beier, F. B. Descamps, F. Fleurot, F. Zhang, G. A. Cox, G. D. Orebi Gann, G. Doucas, G. Prior, G. Tesic, G. T. Ewan, H. B. Mak, H. C. Evans, H. Deng, H. Fergani, H. M. O'Keeffe, H. Wan Chan Tseung, I. Levine, I. T. Lawson, J. A. Detwiler, J. A. Formaggio, J. A. Secrest, J. Caravaca, J. C. Loach, J. Farine, J. F. Wilkerson, J. Heise, J. Law, J. Maneira, J. Monroe, J. R. Klein, J. R. Leslie, J. R. Wilson, J. TM. Goon, J. Wendland, K. Boudjemline, K. Gilje, K. Graham, K. J. Keeter, K. Labe, K. Rielage, K. T. Lesko, K. Zuber, L. C. Stonehill, L. L. Kormos, M. Bergevin, M. Chen, M. Dunford, M. G. Boulay, M. H. Schwendener, M. Huang, M. Jerkins, M. Kos, M. L. Miller, M. Yeh, N. A. Jelley, N. Barros, N. Gagnon, N. McCauley, N. S. Oblath, N. Tolich, N. West, O. Simard, P. Jagam, P. J. Doe, P. J. Harvey, P.-L. Drouin, P. Skensved, R. A. Ott, R. Bonventre, R. D. Martin, R. G. H. Robertson, R. Hazama, R. J. Ford, R. Lange, R. L. Hahn, R. L. Helmer, R. MacLellan, R. Van Berg, R. W. Ollerhead, S. D. Biller, S. D. Reitzner, S. Habib, S. J. M. Peeters, S. Majerus, S. M. Oser, S. N. Ahmed, SNO Collaboration: B. Aharmim, S. R. Elliott, S. R. McGee, S. R. Seibert, T. J. Sonley, T. Kutter, T. Tsui, T. Winchester, W. J. Heintzelman, X. Dai, Y. D. Chan","submitted_at":"2018-11-01T00:14:45Z","abstract_excerpt":"Experimental tests of Lorentz symmetry in systems of all types are critical for ensuring that the basic assumptions of physics are well-founded. Data from all phases of the Sudbury Neutrino Observatory, a kiloton-scale heavy water Cherenkov detector, are analyzed for possible violations of Lorentz symmetry in the neutrino sector. Such violations would appear as one of eight possible signal types in the detector: six seasonal variations in the solar electron neutrino survival probability differing in energy and time dependence, and two shape changes to the oscillated solar neutrino energy spect"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.00166","kind":"arxiv","version":2},"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"}