{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:RBS64ISSLS27NUSJ6623AROILD","short_pith_number":"pith:RBS64ISS","schema_version":"1.0","canonical_sha256":"8865ee22525cb5f6d249f7b5b045c858c43b2fbae1db6177dc9e5b32e27fb430","source":{"kind":"arxiv","id":"1109.4897","version":4},"attestation_state":"computed","paper":{"title":"Measurement of the neutrino velocity with the OPERA detector in the CNGS beam","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-ex","authors_text":"A. Aleksandrov, A. Anokhina, A. Ariga, A. Badertscher, A. Ben Dhahbi, A. Bertolin, A. Cazes, A. Chukanov, A. Di Crescenzo, A. Ereditato, A. Garfagnini, A. Hollnagel, A. Ljubicic, A. Longhin, A. Malgin, A. Mazzoni, A. Meregaglia, A. M. Guler, A. Olchevsky, A. Paoloni, A. Pastore, A. Rubbia, A. Russo, A. Schembri, A. Sheshukov, A. Zghiche, B. Carlus, B. D. Park, B. Klicek, B. Wonsak, C. Bozza, C. Girerd, C. Gollnitz, C. Guerin, C. Gustavino, C. Hagner, C. Jollet, C. Lazzaro, C. Pistillo, C. Sirignano, C. S. Yoon, D. Autiero, D. Di Ferdinando, D. Duchesneau, D. Golubkov, D. Missiaen, D. Naumov, E. Gschwendtner, E. Kiritsis, E. Medinaceli, E. Pennacchio, F. Brunet, F. Cavanna, F. Di Capua, F. Grianti, F. Juget, F. Meisel, F. Nitti, F. Pupilli, F. Riguzzi, F. Terranova, G. Brunetti, G. Colosimo, G. De Lellis, G. Giacomelli, G. Grella, G. Mandrioli, G. Rosa, G. Shoziyoev, G. Sirri, G. Wilquet, H. Ishida, H. Pessard, H. Rokujo, H. Shibuya, I. Efthymiopoulos, I. G. Park, I. Kreslo, I. Rostovtseva, I. Shakiryanova, I. Tezuka, J. Ebert, J. Favier, J. Goldberg, J. Kawada, J. Knuesel, J. Lenkeit, J.-L. Vuilleumier, J. Marteau, J. Schuler, J. Serrano, J. S. Song, J. Wurtz, J. Yoshida, K. Hamada, K. Ishiguro, K. Jakovcic, K. Kodama, K. Morishima, K. Pretzl, L. Chaussard, L. Goncharova, L. Patrizii, L. Scotto Lavina, L. S. Esposito, L. Stanco, L. Votano, M. Chernyavsky, M. Crespi, M. De Serio, M. Dracos, M. Giorgini, M. Giovannozzi, M. Hierholzer, M. Ieva, M. Jones, M. Kamiscioglu, M. Kimura, M. Komatsu, M. Nakamura, M. Pozzato, M. Sioli, M. Spinetti, M. Stipcevic, M. Tenti, M. T. Muciaccia, M. Vladimirov, N. Agafonova, N. D'Ambrosio, N. Di Marco, N. Kitagawa, N. Mauri, N. Naganawa, N. Okateva, N. Polukhina, N. Starkov, N. T. Tran, O. Altinok, O. Egorov, O. Palamara, O. Ryazhskaya, O. Sato, P. Alvarez Sanchez, P. Del Amo Sanchez, P. Migliozzi, P. Monacelli, P. Tolun, P. Vilain, R. A. Fini, R. Brugnera, R. Enikeev, R. Rescigno, S. Aoki, S. Buontempo, S. Dmitrievsky, S. Dusini, S. H. Kim, S. Mikado, S. Ogawa, S. Simone, S. Stellacci, S. Takahashi, S. Tufanli, S. Zemskova, T. Ariga, T. Brugiere, T. Dzhatdoev, T. Ferber, T. Fukuda, T. Hara, The OPERA Collaboration: T. Adam, T. Matsuo, T. Naka, T. Nakano, T. Roganova, T. Strauss, U. Kose, U. Moser, V. Chiarella, V. Matveev, V. Nikitina, V. Ryasny, V. Tioukov, V. Yakushev, Y. Declais, Y. Gornushkin, Y. Nakatsuka, Y. Sato, Y. Zaitsev, Z. Sahnoun","submitted_at":"2011-09-22T17:59:33Z","abstract_excerpt":"The OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km. The measurement is based on data taken by OPERA in the years 2009, 2010 and 2011. Dedicated upgrades of the CNGS timing system and of the OPERA detector, as well as a high precision geodesy campaign for the measurement of the neutrino baseline, allowed reaching comparable systematic and statistical accuracies. An arrival time of CNGS muon neutrinos with respect to the one computed assuming the speed of light in vacuum of (6.5 +/-"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1109.4897","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2011-09-22T17:59:33Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"0025bf22ddc42f8c05ca031581166051872d72f75bb8bd0851df99f5dadde8e5","abstract_canon_sha256":"9a2f76201fa69377d2d949025cbca7f508ea99dca1de01bd003c62ecaf2c804d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:26.419235Z","signature_b64":"RYjeghvSh+e14EhHFp/7SoUvKOR+lP0ouIfsqLmR7tC3fHBdR74kIw2jrPARkftnoK+ehIzhsT9qd1YTvzH4Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8865ee22525cb5f6d249f7b5b045c858c43b2fbae1db6177dc9e5b32e27fb430","last_reissued_at":"2026-05-18T02:00:26.418578Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:26.418578Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measurement of the neutrino velocity with the OPERA detector in the CNGS beam","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-ex","authors_text":"A. Aleksandrov, A. Anokhina, A. Ariga, A. Badertscher, A. Ben Dhahbi, A. Bertolin, A. Cazes, A. Chukanov, A. Di Crescenzo, A. Ereditato, A. Garfagnini, A. Hollnagel, A. Ljubicic, A. Longhin, A. Malgin, A. Mazzoni, A. Meregaglia, A. M. Guler, A. Olchevsky, A. Paoloni, A. Pastore, A. Rubbia, A. Russo, A. Schembri, A. Sheshukov, A. Zghiche, B. Carlus, B. D. Park, B. Klicek, B. Wonsak, C. Bozza, C. Girerd, C. Gollnitz, C. Guerin, C. Gustavino, C. Hagner, C. Jollet, C. Lazzaro, C. Pistillo, C. Sirignano, C. S. Yoon, D. Autiero, D. Di Ferdinando, D. Duchesneau, D. Golubkov, D. Missiaen, D. Naumov, E. Gschwendtner, E. Kiritsis, E. Medinaceli, E. Pennacchio, F. Brunet, F. Cavanna, F. Di Capua, F. Grianti, F. Juget, F. Meisel, F. Nitti, F. Pupilli, F. Riguzzi, F. Terranova, G. Brunetti, G. Colosimo, G. De Lellis, G. Giacomelli, G. Grella, G. Mandrioli, G. Rosa, G. Shoziyoev, G. Sirri, G. Wilquet, H. Ishida, H. Pessard, H. Rokujo, H. Shibuya, I. Efthymiopoulos, I. G. Park, I. Kreslo, I. Rostovtseva, I. Shakiryanova, I. Tezuka, J. Ebert, J. Favier, J. Goldberg, J. Kawada, J. Knuesel, J. Lenkeit, J.-L. Vuilleumier, J. Marteau, J. Schuler, J. Serrano, J. S. Song, J. Wurtz, J. Yoshida, K. Hamada, K. Ishiguro, K. Jakovcic, K. Kodama, K. Morishima, K. Pretzl, L. Chaussard, L. Goncharova, L. Patrizii, L. Scotto Lavina, L. S. Esposito, L. Stanco, L. Votano, M. Chernyavsky, M. Crespi, M. De Serio, M. Dracos, M. Giorgini, M. Giovannozzi, M. Hierholzer, M. Ieva, M. Jones, M. Kamiscioglu, M. Kimura, M. Komatsu, M. Nakamura, M. Pozzato, M. Sioli, M. Spinetti, M. Stipcevic, M. Tenti, M. T. Muciaccia, M. Vladimirov, N. Agafonova, N. D'Ambrosio, N. Di Marco, N. Kitagawa, N. Mauri, N. Naganawa, N. Okateva, N. Polukhina, N. Starkov, N. T. Tran, O. Altinok, O. Egorov, O. Palamara, O. Ryazhskaya, O. Sato, P. Alvarez Sanchez, P. Del Amo Sanchez, P. Migliozzi, P. Monacelli, P. Tolun, P. Vilain, R. A. Fini, R. Brugnera, R. Enikeev, R. Rescigno, S. Aoki, S. Buontempo, S. Dmitrievsky, S. Dusini, S. H. Kim, S. Mikado, S. Ogawa, S. Simone, S. Stellacci, S. Takahashi, S. Tufanli, S. Zemskova, T. Ariga, T. Brugiere, T. Dzhatdoev, T. Ferber, T. Fukuda, T. Hara, The OPERA Collaboration: T. Adam, T. Matsuo, T. Naka, T. Nakano, T. Roganova, T. Strauss, U. Kose, U. Moser, V. Chiarella, V. Matveev, V. Nikitina, V. Ryasny, V. Tioukov, V. Yakushev, Y. Declais, Y. Gornushkin, Y. Nakatsuka, Y. Sato, Y. Zaitsev, Z. Sahnoun","submitted_at":"2011-09-22T17:59:33Z","abstract_excerpt":"The OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km. The measurement is based on data taken by OPERA in the years 2009, 2010 and 2011. Dedicated upgrades of the CNGS timing system and of the OPERA detector, as well as a high precision geodesy campaign for the measurement of the neutrino baseline, allowed reaching comparable systematic and statistical accuracies. An arrival time of CNGS muon neutrinos with respect to the one computed assuming the speed of light in vacuum of (6.5 +/-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.4897","kind":"arxiv","version":4},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1109.4897","created_at":"2026-05-18T02:00:26.418675+00:00"},{"alias_kind":"arxiv_version","alias_value":"1109.4897v4","created_at":"2026-05-18T02:00:26.418675+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.4897","created_at":"2026-05-18T02:00:26.418675+00:00"},{"alias_kind":"pith_short_12","alias_value":"RBS64ISSLS27","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"RBS64ISSLS27NUSJ","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"RBS64ISS","created_at":"2026-05-18T12:26:41.206345+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD","json":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD.json","graph_json":"https://pith.science/api/pith-number/RBS64ISSLS27NUSJ6623AROILD/graph.json","events_json":"https://pith.science/api/pith-number/RBS64ISSLS27NUSJ6623AROILD/events.json","paper":"https://pith.science/paper/RBS64ISS"},"agent_actions":{"view_html":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD","download_json":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD.json","view_paper":"https://pith.science/paper/RBS64ISS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1109.4897&json=true","fetch_graph":"https://pith.science/api/pith-number/RBS64ISSLS27NUSJ6623AROILD/graph.json","fetch_events":"https://pith.science/api/pith-number/RBS64ISSLS27NUSJ6623AROILD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD/action/storage_attestation","attest_author":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD/action/author_attestation","sign_citation":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD/action/citation_signature","submit_replication":"https://pith.science/pith/RBS64ISSLS27NUSJ6623AROILD/action/replication_record"}},"created_at":"2026-05-18T02:00:26.418675+00:00","updated_at":"2026-05-18T02:00:26.418675+00:00"}