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A longer candidate (10.1088/1748-0221/11/05/P05016.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1088/1748-0221/11/05/P05016.arXiv","detected_arxiv_id":null,"ref_index":69,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1088/1748-0221/14/02/P02021.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1088/1748-0221/14/02/P02021.arXiv","detected_arxiv_id":null,"ref_index":105,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/physrevlett.134.131801.url:https://link.aps.org/doi/10) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1103/physrevlett.134.131801.url:https://link.aps.org/doi/10","detected_arxiv_id":null,"ref_index":54,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/PhysRevD.110.122003.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1103/PhysRevD.110.122003.arXiv","detected_arxiv_id":null,"ref_index":116,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1145/279232.279236.url:https://doi.org/10.1145/279232.279236) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1145/279232.279236.url:https://doi.org/10.1145/279232.279236","detected_arxiv_id":null,"ref_index":86,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.nima.2003.11.423.url:https://www) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1016/j.nima.2003.11.423.url:https://www","detected_arxiv_id":null,"ref_index":100,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.nima.2004.07.248.url:http://dx.doi.org/10.1016/j.nima.2004.07.248) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1016/j.nima.2004.07.248.url:http://dx.doi.org/10.1016/j.nima.2004.07.248","detected_arxiv_id":null,"ref_index":110,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.physletb.2015.12.037.url:https://www.sciencedirect.com/) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1016/j.physletb.2015.12.037.url:https://www.sciencedirect.com/","detected_arxiv_id":null,"ref_index":145,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/physrevlett.98.050402.url:https://link.aps.org/doi/10.1103/PhysRevLett.98.050402) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1103/physrevlett.98.050402.url:https://link.aps.org/doi/10.1103/PhysRevLett.98.050402","detected_arxiv_id":null,"ref_index":151,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.nima.2018.06.018.url:https://www.sciencedirect.com/) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1016/j.nima.2018.06.018.url:https://www.sciencedirect.com/","detected_arxiv_id":null,"ref_index":46,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1088/1748-0221/17/11/P11003.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1088/1748-0221/17/11/P11003.arXiv","detected_arxiv_id":null,"ref_index":131,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/PhysRevLett.102.101802.url) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1103/PhysRevLett.102.101802.url","detected_arxiv_id":null,"ref_index":14,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/physrevlett.98.131802.url:https://link.aps.org/doi/10.1103/PhysRevLett) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1103/physrevlett.98.131802.url:https://link.aps.org/doi/10.1103/PhysRevLett","detected_arxiv_id":null,"ref_index":150,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1051/0004-6361/201833910.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1051/0004-6361/201833910.arXiv","detected_arxiv_id":null,"ref_index":25,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1140/s10052-018-5807-z.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1140/s10052-018-5807-z.arXiv","detected_arxiv_id":null,"ref_index":51,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/physreva.43.6089.url:https://link.aps.org/doi/10.1103/PhysRevA) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1103/physreva.43.6089.url:https://link.aps.org/doi/10.1103/PhysRevA","detected_arxiv_id":null,"ref_index":66,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.nds.2015.07.002.url:https://www.sciencedirect.com/science/article/pii/S0090375215000253) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1016/j.nds.2015.07.002.url:https://www.sciencedirect.com/science/article/pii/S0090375215000253","detected_arxiv_id":null,"ref_index":81,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/s0168-9002(96)00740-1.url:https://www.sciencedirect.com/science/article/) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1016/s0168-9002(96)00740-1.url:https://www.sciencedirect.com/science/article/","detected_arxiv_id":null,"ref_index":95,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.nima.2010.03.102.url:http://dx.doi.org/10.1016/j) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1016/j.nima.2010.03.102.url:http://dx.doi.org/10.1016/j","detected_arxiv_id":null,"ref_index":109,"audited_at":"2026-07-09T09:57:57.628720Z"},{"detector":"doi_compliance","finding_type":"recoverable_identifier","severity":"advisory","verdict_class":"incontrovertible","note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1088/1748-0221/16/10/P10021.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","detected_doi":"10.1088/1748-0221/16/10/P10021.arXiv","detected_arxiv_id":null,"ref_index":130,"audited_at":"2026-07-09T09:57:57.628720Z"}],"snapshot_sha256":"c22809c8a70796a2e879729b6ef332c5c70eed38093d887c50b4514ad8f25183"},"events":[{"event_id":8306,"event_type":"pith.integrity.v1","payload_sha256":"3d56e9fe72a20b522ab83c4b0c87ffdc173a0b0af44cef84ac31eafe6e10c987","signature_b64":"8b/v6RKLDJjhK+tXriL3+h7aOR5FHKnt3QggpvQMb4NEvsYnIJ3mF3XyrSm3Mpn4iRP4n6OMc8hLh1tZeRSwCw==","signing_key_id":"pith-v1-2026-05","created_at":"2026-07-09T10:02:33.459657+00:00","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1088/1748-0221/16/10/P10021.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"M. R. Anderson et al. “Optical calibration of the SNO+ detector in the water phase with deployed sources.”JINST,16(10), 2021, P10021.doi: 10.1088/1748-0221/16/10/ P10021. arXiv: 2106.03951[physics.ins-det]","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":130,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"M. R. 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A longer candidate (10.1103/PhysRevD.110.122003.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"A. Allega et al. “Measurement of the B8 solar neutrino flux using the full SNO+ water phase dataset.”Phys. Rev. D,110(12), 2024, p. 122003.doi: 10.1103/PhysRevD.110. 122003. arXiv: 2407.17595[hep-ex]","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":116,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"A. Allega et al. “Measurement of the B8 solar neutrino flux using the full SNO+ water phase dataset.”Phys. Rev. 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A longer candidate (10.1016/j.nima.2004.07.248.url:http://dx.doi.org/10.1016/j.nima.2004.07.248) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"A. Brigatti, A. Ianni, P. Lombardi, G. Ranucci, and O. Smirnov. “The photomultiplier tube testing facility for the Borexino experiment at LNGS.”Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Dete","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":110,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"A. Brigatti, A. Ianni, P. Lombardi, G. Ranucci, and O. 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A longer candidate (10.1016/j.nima.2010.03.102.url:http://dx.doi.org/10.1016/j) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"R. Abbasi et al. “Calibration and characterization of the IceCube photomultiplier tube.”Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment,618(1–3), June 2010, pp. ","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":109,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"R. 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A longer candidate (10.1088/1748-0221/14/02/P02021.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"J. Asaadi, B. J. P. Jones, A. Tripathi, I. Parmaksiz, H. Sullivan, and Z. G. R. Williams. “Emanation and bulk fluorescence in liquid argon from tetraphenyl butadiene wavelength shifting coatings.”JINST,14(02), 2019, P02021.doi: 10.1088/1748","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":105,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"J. Asaadi, B. J. P. Jones, A. Tripathi, I. Parmaksiz, H. Sullivan, and Z. G. R. 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A longer candidate (10.1016/j.nima.2003.11.423.url:https://www) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"S. Amoruso et al. “Study of electron recombination in liquid argon with the ICARUS TPC.”Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment,523(3), 2004, pp. 275–286","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":100,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"S. 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A longer candidate (10.1016/s0168-9002(96)00740-1.url:https://www.sciencedirect.com/science/article/) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"N. Ishida et al. “Attenuation length measurements of scintillation light in liquid rare gases and their mixtures using an improved reflection suppresser.”Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrome","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":95,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"N. 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A longer candidate (10.1145/279232.279236.url:https://doi.org/10.1145/279232.279236) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"C. Zhu, R. H. Byrd, P. Lu, and J. Nocedal. “Algorithm 778: L-BFGS-B: Fortran subroutines for large-scale bound-constrained optimization.”ACM Trans. Math. Softw., 23(4), Dec. 1997, pp. 550–560.issn: 0098-3500.doi: 10.1145/279232.279236.url: ","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":86,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"C. Zhu, R. H. Byrd, P. Lu, and J. Nocedal. “Algorithm 778: L-BFGS-B: Fortran subroutines for large-scale bound-constrained optimization.”ACM Trans. Math. 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A longer candidate (10.1016/j.nds.2015.07.002.url:https://www.sciencedirect.com/science/article/pii/S0090375215000253) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"M. S. Basunia. “Nuclear Data Sheets for A = 22.”Nuclear Data Sheets,127, 2015, pp. 69–190.issn: 0090-3752.doi: https://doi.org/10.1016/j.nds.2015.07.002.url: https://www.sciencedirect.com/science/article/pii/S0090375215000253","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":81,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"M. S. 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A longer candidate (10.1088/1748-0221/11/05/P05016.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"D. Whittington, S. Mufson, and B. Howard. “Scintillation Light from Cosmic-Ray Muons in Liquid Argon.”JINST,11(05), 2016, P05016.doi: 10.1088/1748-0221/11/ 05/P05016. arXiv: 1408.1763[physics.ins-det]","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":69,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"D. Whittington, S. Mufson, and B. 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A longer candidate (10.1103/physreva.43.6089.url:https://link.aps.org/doi/10.1103/PhysRevA) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"W. Krötz, A. Ulrich, B. Busch, G. Ribitzki, and J. Wieser. “Third excimer continuum of argon excited by a heavy-ion beam.”Phys. Rev. A,43, 11, June 1991, pp. 6089–6094. doi: 10.1103/PhysRevA.43.6089.url: https://link.aps.org/doi/10.1103/Phy","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":66,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"W. Krötz, A. Ulrich, B. Busch, G. Ribitzki, and J. Wieser. “Third excimer continuum of argon excited by a heavy-ion beam.”Phys. Rev. A,43, 11, June 1991, pp. 6089–6094. doi: 10.1103/PhysRevA.43.6089.url: https://link.aps.org/doi/10.1103/Phy","reconstructed_doi":"10.1103/physreva.43.6089.url:https://link.aps.org/doi/10.1103/PhysRevA"},"severity":"advisory","ref_index":66,"audited_at":"2026-07-09T09:57:57.628720Z","event_type":"pith.integrity.v1","detected_doi":"10.1103/physreva.43.6089.url:https://link.aps.org/doi/10.1103/PhysRevA","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"1543e9c3505c5a1ddf4077db7d4a8ff13db32264fd54396c672809783c319045","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null}},{"event_id":8295,"event_type":"pith.integrity.v1","payload_sha256":"a29a6ec225dcedc2f1b1c049075fc647d50dd2946ddd71b3145763596b8091e5","signature_b64":"+ZHHwkebloT6W7KBs6xP8olRQpCpQo8659S7vFJFYcvNx/mY0rc9+GBYJ+plMBBGMrFqG4hiaJcHvgQD+Z5uAQ==","signing_key_id":"pith-v1-2026-05","created_at":"2026-07-09T10:02:33.446830+00:00","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/physrevlett.134.131801.url:https://link.aps.org/doi/10) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"M. A. Hernandez-Morquecho et al. “Measurements of Pion and Muon Nuclear Capture at Rest on Argon in the LArIAT Experiment.”Phys. Rev. Lett.,134, 13, Apr. 2025, p. 131801.doi: 10.1103/PhysRevLett.134.131801.url: https://link.aps.org/doi/10. ","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":54,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"M. A. Hernandez-Morquecho et al. “Measurements of Pion and Muon Nuclear Capture at Rest on Argon in the LArIAT Experiment.”Phys. Rev. Lett.,134, 13, Apr. 2025, p. 131801.doi: 10.1103/PhysRevLett.134.131801.url: https://link.aps.org/doi/10. 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A longer candidate (10.1140/s10052-018-5807-z.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"C. Benson, G. Orebi Gann, and V. Gehman. “Measurements of the intrinsic quantum efficiency and absorption length of tetraphenyl butadiene thin films in the vacuum ultraviolet regime.”Eur. Phys. J. C,78(4), 2018, p. 329.doi: 10.1140/s10052-0","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":51,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"C. Benson, G. Orebi Gann, and V. Gehman. “Measurements of the intrinsic quantum efficiency and absorption length of tetraphenyl butadiene thin films in the vacuum ultraviolet regime.”Eur. Phys. J. C,78(4), 2018, p. 329.doi: 10.1140/s10052-0","reconstructed_doi":"10.1140/s10052-018-5807-z.arXiv"},"severity":"advisory","ref_index":51,"audited_at":"2026-07-09T09:57:57.628720Z","event_type":"pith.integrity.v1","detected_doi":"10.1140/s10052-018-5807-z.arXiv","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"1223d063cdc5fd5ee122b286ff3b24106051d6c997ebedd15e1bfc74ff806832","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null}},{"event_id":8293,"event_type":"pith.integrity.v1","payload_sha256":"daea6fb039dea2043b67a189cd91f5d06fe17271b90aca3ed45fb58aeb4fe15f","signature_b64":"CwlUdwW8s39cixsAcHy5b6ukdmaLwWUyE+35khzMBu8SckzEXpaJVRPlgMMvxpIY/JCGuuCPQw8OBaB3ZzYMBg==","signing_key_id":"pith-v1-2026-05","created_at":"2026-07-09T10:02:33.444100+00:00","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.nima.2018.06.018.url:https://www.sciencedirect.com/) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"L. Zavorka, M. J. Mocko, and P. E. Koehler. “Physics design of the next-generation spallation neutron target-moderator-reflector-shield assembly at LANSCE.”Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectro","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":46,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"L. Zavorka, M. J. Mocko, and P. E. 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A longer candidate (10.1016/0370-2693(81) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"M. Dine, W. Fischler, and M. Srednicki. “A Simple Solution to the Strong CP Problem with a Harmless Axion.”Phys. Lett. B,104, 1981, pp. 199–202.doi: 10.1016/0370- 2693(81)90590-6","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":37,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"M. Dine, W. Fischler, and M. Srednicki. “A Simple Solution to the Strong CP Problem with a Harmless Axion.”Phys. Lett. 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A longer candidate (10.1051/0004-6361/201833910.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"N. Aghanim et al. “Planck 2018 results. VI. Cosmological parameters.”Astron. Astro- phys.,641, 2020. [Erratum: Astron.Astrophys. 652, C4 (2021)], A6.doi: 10.1051/0004- 6361/201833910. arXiv: 1807.06209[astro-ph.CO]","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":25,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"N. Aghanim et al. “Planck 2018 results. VI. Cosmological parameters.”Astron. Astro- phys.,641, 2020. 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A longer candidate (10.1103/physrevlett.121.221801.url:https://link.aps.org/doi/10) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"A. A. Aguilar-Arevalo et al. “Significant Excess of Electronlike Events in the Mini- BooNE Short-Baseline Neutrino Experiment.”Phys. Rev. Lett.,121, 22, Nov. 2018, p. 221801.doi: 10.1103/PhysRevLett.121.221801.url: https://link.aps.org/doi/","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":15,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"A. A. Aguilar-Arevalo et al. “Significant Excess of Electronlike Events in the Mini- BooNE Short-Baseline Neutrino Experiment.”Phys. Rev. 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A longer candidate (10.1103/PhysRevD.64.112007.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"A. Aguilar et al. “Evidence for neutrino oscillations from the observation of¯νe appear- ance in a¯νµ beam.”Phys. Rev. D,64, 2001, p. 112007.doi: 10.1103/PhysRevD.64. 112007. arXiv: hep-ex/0104049","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":12,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"A. Aguilar et al. “Evidence for neutrino oscillations from the observation of¯νe appear- ance in a¯νµ beam.”Phys. Rev. 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A longer candidate (10.1103/physrevlett.98.050402.url:https://link.aps.org/doi/10.1103/PhysRevLett.98.050402) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"R. N. Mohapatra and S. Nasri. “Reconciling the CAST and PVLAS Results.”Phys. Rev. Lett.,98, 5, Jan. 2007, p. 050402.doi: 10.1103/PhysRevLett.98.050402.url: https://link.aps.org/doi/10.1103/PhysRevLett.98.050402","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":151,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"R. N. Mohapatra and S. Nasri. “Reconciling the CAST and PVLAS Results.”Phys. Rev. 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A longer candidate (10.1103/physrevlett.98.131802.url:https://link.aps.org/doi/10.1103/PhysRevLett) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"A. Dupays, E. Massó, J. Redondo, and C. Rizzo. “Light Scalars Coupled to Photons and Non-Newtonian Forces.”Phys. Rev. Lett.,98, 13, Mar. 2007, p. 131802.doi: 10.1103/PhysRevLett.98.131802.url: https://link.aps.org/doi/10.1103/PhysRevLett. 9","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":150,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"A. Dupays, E. Massó, J. Redondo, and C. Rizzo. “Light Scalars Coupled to Photons and Non-Newtonian Forces.”Phys. Rev. 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A longer candidate (10.1103/PhysRevLett.97.151802.url) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"E. Massó and J. Redondo. “Compatibility of Cast Search with Axionlike Interpretation of PVLAS Results.”Phys. Rev. Lett.,97, 15, Oct. 2006, p. 151802.doi: 10.1103/ PhysRevLett.97.151802.url: https://link.aps.org/doi/10.1103/PhysRevLett.97. 1","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":149,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"E. Massó and J. Redondo. “Compatibility of Cast Search with Axionlike Interpretation of PVLAS Results.”Phys. Rev. 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A longer candidate (10.1103/physrevd.75.013004.url:https://link.aps.org/doi/10.1103/PhysRevD) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"J. Jaeckel, E. Massó, J. Redondo, A. Ringwald, and F. Takahashi. “Need for purely laboratory-based axionlike particle searches.”Phys. Rev. D,75, 1, Jan. 2007, p. 013004. doi: 10.1103/PhysRevD.75.013004.url: https://link.aps.org/doi/10.1103/","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":147,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"J. Jaeckel, E. Massó, J. Redondo, A. Ringwald, and F. Takahashi. “Need for purely laboratory-based axionlike particle searches.”Phys. Rev. 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A longer candidate (10.1016/j.physletb.2015.12.037.url:https://www.sciencedirect.com/) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"J. Jaeckel and M. Spannowsky. “Probing MeV to 90 GeV axion-like particles with LEP and LHC.”Physics Letters B,753, 2016, pp. 482–487.issn: 0370-2693.doi: https://doi.org/10.1016/j.physletb.2015.12.037.url: https://www.sciencedirect.com/ sci","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":145,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"J. Jaeckel and M. 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A longer candidate (10.1140/epjp/i2018-11973-4.arXiv) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"C. E. Aalseth et al. “DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS.”Eur. Phys. J. Plus,133, 2018, p. 131.doi: 10.1140/epjp/ i2018-11973-4. arXiv: 1707.08145[physics.ins-det]","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":144,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"C. E. Aalseth et al. “DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS.”Eur. Phys. J. 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A longer candidate (10.1016/j.nuclphysbps.2004.10.091.url:https) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"G. Fiorillo. “The liquid argon technology for neutrino and astroparticle detectors.” Nuclear Physics B - Proceedings Supplements,150, 2006. Proceedings of the 9th Topical Seminar on Innovative Particle and Radiation Detectors, pp. 372–376.i","arxiv_id":"2607.07476","detector":"doi_compliance","evidence":{"ref_index":142,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"G. Fiorillo. “The liquid argon technology for neutrino and astroparticle detectors.” Nuclear Physics B - Proceedings Supplements,150, 2006. 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