{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:V3YX7MMBNJEHYEV2XKILRKECHW","short_pith_number":"pith:V3YX7MMB","schema_version":"1.0","canonical_sha256":"aef17fb1816a487c12baba90b8a8823da1a2a23faa6c73bb7abd129ed9d3c137","source":{"kind":"arxiv","id":"1911.06422","version":1},"attestation_state":"computed","paper":{"title":"Sensitivity of the COHERENT Experiment to Accelerator-Produced Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"hep-ex","authors_text":"A. Bolozdynya, A. Galindo-Uribarri, A. Khromov, A. Konovalov, A. Kumpan, A. Shakirov, B. Becker, B. Cabrera-Palmer, B. Suh, C. Awe, C.-H. Yu, C. J. Virtue, COHERENT Collaboration: D. Akimov, C. Wiseman, D. J. Salvat, D. M. Markoff, D. Pershey, D. Radford, D. Reyna, D. Rudik, D. S. Parno, E. Conley, E. Kozlova, G. C. Rich, G. Simakov, G. Sinev, G. Visser, H. Moreno, H. Ray, I. Tolstukhin, J. A. Detwiler, J. Daughhetee, J. Liu, J. M. Link, J. Newby, J. Raybern, J. Runge, J. T. Librande, J. Vanderwerp, J. Yang, J. Yoo, J. Zettlemoyer, K. Mann, K. Scholberg, K. S. Hansen, K. Tellez-Giron-Flores, L. Fabris, L. J. Kaufman, L. Li, M. A. Blackston, M. del Valle Coello, M. Febbraro, M. Kaemingk, M. P. Green, M. R. Durand, M. R. Heath, N. Chen, O. Razuvaeva, P. An, P. E. Mueller, P. S. Barbeau, R. L. Cooper, R. L. Varner, R. Rapp, R. Tayloe, R. T. Thornton, S. Hedges, S. Penttila, S. R. Elliott, T. Johnson, T. Wongjirad, V. Belov, V. Sosnovtsev, W. Fox, W. M. Snow, Y. Efremenko, Y.-R. Yen","submitted_at":"2019-11-15T00:10:27Z","abstract_excerpt":"The COHERENT experiment is well poised to test sub-GeV dark matter models using low-energy recoil detectors sensitive to coherent elastic neutrino-nucleus scattering (CEvNS) in the $\\pi$-DAR neutrino beam produced by the Spallation Neutron Source. We show how a planned 750-kg liquid argon scintillation detector would place leading limits on scalar light dark matter models, over two orders of magnitude of dark matter mass, for dark matter particles produced through vector and leptophobic portals in the absence of other effects beyond the standard model. The characteristic timing structure of a "},"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":"1911.06422","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2019-11-15T00:10:27Z","cross_cats_sorted":["physics.ins-det"],"title_canon_sha256":"6955b5dfff9f43b1d64b8e50e440fbfcc4f11225eeb4c1932dd5fbf413469251","abstract_canon_sha256":"e5ca7807f8788ea8439393849bb79061636612ab665690471a93471bab64e833"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:40:22.395018Z","signature_b64":"9wvdEhz5DK49NtNZ4puf4gBGXpk/UlEoPVh64JziKnhfEw8Kbvnz2+IHWvVx+Kyt8n6xzeE8nHBEg8+a9tT5BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aef17fb1816a487c12baba90b8a8823da1a2a23faa6c73bb7abd129ed9d3c137","last_reissued_at":"2026-07-05T01:40:22.394516Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:40:22.394516Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Sensitivity of the COHERENT Experiment to Accelerator-Produced Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"hep-ex","authors_text":"A. Bolozdynya, A. Galindo-Uribarri, A. Khromov, A. Konovalov, A. Kumpan, A. Shakirov, B. Becker, B. Cabrera-Palmer, B. Suh, C. Awe, C.-H. Yu, C. J. Virtue, COHERENT Collaboration: D. Akimov, C. Wiseman, D. J. Salvat, D. M. Markoff, D. Pershey, D. Radford, D. Reyna, D. Rudik, D. S. Parno, E. Conley, E. Kozlova, G. C. Rich, G. Simakov, G. Sinev, G. Visser, H. Moreno, H. Ray, I. Tolstukhin, J. A. Detwiler, J. Daughhetee, J. Liu, J. M. Link, J. Newby, J. Raybern, J. Runge, J. T. Librande, J. Vanderwerp, J. Yang, J. Yoo, J. Zettlemoyer, K. Mann, K. Scholberg, K. S. Hansen, K. Tellez-Giron-Flores, L. Fabris, L. J. Kaufman, L. Li, M. A. Blackston, M. del Valle Coello, M. Febbraro, M. Kaemingk, M. P. Green, M. R. Durand, M. R. Heath, N. Chen, O. Razuvaeva, P. An, P. E. Mueller, P. S. Barbeau, R. L. Cooper, R. L. Varner, R. Rapp, R. Tayloe, R. T. Thornton, S. Hedges, S. Penttila, S. R. Elliott, T. Johnson, T. Wongjirad, V. Belov, V. Sosnovtsev, W. Fox, W. M. Snow, Y. Efremenko, Y.-R. Yen","submitted_at":"2019-11-15T00:10:27Z","abstract_excerpt":"The COHERENT experiment is well poised to test sub-GeV dark matter models using low-energy recoil detectors sensitive to coherent elastic neutrino-nucleus scattering (CEvNS) in the $\\pi$-DAR neutrino beam produced by the Spallation Neutron Source. We show how a planned 750-kg liquid argon scintillation detector would place leading limits on scalar light dark matter models, over two orders of magnitude of dark matter mass, for dark matter particles produced through vector and leptophobic portals in the absence of other effects beyond the standard model. The characteristic timing structure of a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1911.06422","kind":"arxiv","version":1},"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/1911.06422/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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1911.06422","created_at":"2026-07-05T01:40:22.394580+00:00"},{"alias_kind":"arxiv_version","alias_value":"1911.06422v1","created_at":"2026-07-05T01:40:22.394580+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1911.06422","created_at":"2026-07-05T01:40:22.394580+00:00"},{"alias_kind":"pith_short_12","alias_value":"V3YX7MMBNJEH","created_at":"2026-07-05T01:40:22.394580+00:00"},{"alias_kind":"pith_short_16","alias_value":"V3YX7MMBNJEHYEV2","created_at":"2026-07-05T01:40:22.394580+00:00"},{"alias_kind":"pith_short_8","alias_value":"V3YX7MMB","created_at":"2026-07-05T01:40:22.394580+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.15306","citing_title":"New Physics Opportunities at Neutrino Facilities: BSM Physics at Accelerator, Atmospheric, and Reactor Neutrino Experiments","ref_index":240,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW","json":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW.json","graph_json":"https://pith.science/api/pith-number/V3YX7MMBNJEHYEV2XKILRKECHW/graph.json","events_json":"https://pith.science/api/pith-number/V3YX7MMBNJEHYEV2XKILRKECHW/events.json","paper":"https://pith.science/paper/V3YX7MMB"},"agent_actions":{"view_html":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW","download_json":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW.json","view_paper":"https://pith.science/paper/V3YX7MMB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1911.06422&json=true","fetch_graph":"https://pith.science/api/pith-number/V3YX7MMBNJEHYEV2XKILRKECHW/graph.json","fetch_events":"https://pith.science/api/pith-number/V3YX7MMBNJEHYEV2XKILRKECHW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW/action/storage_attestation","attest_author":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW/action/author_attestation","sign_citation":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW/action/citation_signature","submit_replication":"https://pith.science/pith/V3YX7MMBNJEHYEV2XKILRKECHW/action/replication_record"}},"created_at":"2026-07-05T01:40:22.394580+00:00","updated_at":"2026-07-05T01:40:22.394580+00:00"}