{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:GOCLTZA5D2JDQOZTSVDVVSHGOK","short_pith_number":"pith:GOCLTZA5","schema_version":"1.0","canonical_sha256":"3384b9e41d1e92383b3395475ac8e672964dd48c567286eb0507bb1f15796faf","source":{"kind":"arxiv","id":"0807.2926","version":3},"attestation_state":"computed","paper":{"title":"Solar neutrino limit on axions and keV-mass bosons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Georg Raffelt, Paolo Gondolo","submitted_at":"2008-07-18T18:23:01Z","abstract_excerpt":"The all-flavor solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO) constrains nonstandard energy losses to less than about 10% of the Sun's photon luminosity, superseding a helioseismological argument and providing new limits on the interaction strength of low-mass particles. For the axion-photon coupling strength we find g_a\\gamma < 7E-10 1/GeV. We also derive explicit limits on the Yukawa coupling to electrons of pseudoscalar, scalar and vector bosons with keV-scale masses."},"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":"0807.2926","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-07-18T18:23:01Z","cross_cats_sorted":[],"title_canon_sha256":"53f8cd1991bb1d1d02f6070a2c1e2930a5ba677651e68487cbe0a27e572433cc","abstract_canon_sha256":"9a8472d7c813d59542a4de23f954d0d021b816c655eda6fcb9420e4f1bbadda7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:27:32.431894Z","signature_b64":"FLP30+h3q9NU31cRDcDb+w8VRGN87PcUQkVJLu3KMlaYJFW3pfuxsuoZp2+wjfpOzwYoaiWEiWT7kF/N0NlaDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3384b9e41d1e92383b3395475ac8e672964dd48c567286eb0507bb1f15796faf","last_reissued_at":"2026-07-04T17:27:32.431478Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:27:32.431478Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar neutrino limit on axions and keV-mass bosons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Georg Raffelt, Paolo Gondolo","submitted_at":"2008-07-18T18:23:01Z","abstract_excerpt":"The all-flavor solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO) constrains nonstandard energy losses to less than about 10% of the Sun's photon luminosity, superseding a helioseismological argument and providing new limits on the interaction strength of low-mass particles. For the axion-photon coupling strength we find g_a\\gamma < 7E-10 1/GeV. We also derive explicit limits on the Yukawa coupling to electrons of pseudoscalar, scalar and vector bosons with keV-scale masses."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0807.2926","kind":"arxiv","version":3},"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/0807.2926/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":"0807.2926","created_at":"2026-07-04T17:27:32.431539+00:00"},{"alias_kind":"arxiv_version","alias_value":"0807.2926v3","created_at":"2026-07-04T17:27:32.431539+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0807.2926","created_at":"2026-07-04T17:27:32.431539+00:00"},{"alias_kind":"pith_short_12","alias_value":"GOCLTZA5D2JD","created_at":"2026-07-04T17:27:32.431539+00:00"},{"alias_kind":"pith_short_16","alias_value":"GOCLTZA5D2JDQOZT","created_at":"2026-07-04T17:27:32.431539+00:00"},{"alias_kind":"pith_short_8","alias_value":"GOCLTZA5","created_at":"2026-07-04T17:27:32.431539+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.25779","citing_title":"Dark Photons from Red Dwarfs","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2606.20792","citing_title":"Minimal Proton-Mass Dark Matter","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2604.09283","citing_title":"Probing Solar Symmetrons with Direct Detection","ref_index":76,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK","json":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK.json","graph_json":"https://pith.science/api/pith-number/GOCLTZA5D2JDQOZTSVDVVSHGOK/graph.json","events_json":"https://pith.science/api/pith-number/GOCLTZA5D2JDQOZTSVDVVSHGOK/events.json","paper":"https://pith.science/paper/GOCLTZA5"},"agent_actions":{"view_html":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK","download_json":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK.json","view_paper":"https://pith.science/paper/GOCLTZA5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0807.2926&json=true","fetch_graph":"https://pith.science/api/pith-number/GOCLTZA5D2JDQOZTSVDVVSHGOK/graph.json","fetch_events":"https://pith.science/api/pith-number/GOCLTZA5D2JDQOZTSVDVVSHGOK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK/action/storage_attestation","attest_author":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK/action/author_attestation","sign_citation":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK/action/citation_signature","submit_replication":"https://pith.science/pith/GOCLTZA5D2JDQOZTSVDVVSHGOK/action/replication_record"}},"created_at":"2026-07-04T17:27:32.431539+00:00","updated_at":"2026-07-04T17:27:32.431539+00:00"}