{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:ZRMTZXJ3THOUYICX52VGICNNC5","short_pith_number":"pith:ZRMTZXJ3","schema_version":"1.0","canonical_sha256":"cc593cdd3b99dd4c2057eeaa6409ad17587a2bfeeed0e83780b80b33b6487810","source":{"kind":"arxiv","id":"astro-ph/9605153","version":1},"attestation_state":"computed","paper":{"title":"Solar opacity, neutrino signals and helioseismology","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Ricci","submitted_at":"1996-05-24T20:03:01Z","abstract_excerpt":"In connection with the recent suggestion by Tsytovich et al. that opacity in the solar core could be overestimated, we consider the following questions: i) What would a 10\\% opacity reduction imply for the solar neutrino puzzle? ii) Is there any hope of solving the solar neutrino puzzle by changing opacity? iii) Is a 10\\% opacity reduction testable with helioseismological data?"},"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":"astro-ph/9605153","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-05-24T20:03:01Z","cross_cats_sorted":[],"title_canon_sha256":"53258736b08b8f2564d9590d6fc544fe3486d74175a2a6e1f93c984b0bb8fe72","abstract_canon_sha256":"b5300a8d41b7a9eb4cfcf882e138ec00980a706773e612b25b375e5c5aa83c2b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:21:40.653960Z","signature_b64":"D7japBuUGpT7iKjufJ/gDvo7Yy0Y//fCfYZkOGKfrpQBi9PGrec9Wo27nMq9k4r6n255SY5jE9W/sd1VO6J4DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc593cdd3b99dd4c2057eeaa6409ad17587a2bfeeed0e83780b80b33b6487810","last_reissued_at":"2026-05-18T04:21:40.653504Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:21:40.653504Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar opacity, neutrino signals and helioseismology","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Ricci","submitted_at":"1996-05-24T20:03:01Z","abstract_excerpt":"In connection with the recent suggestion by Tsytovich et al. that opacity in the solar core could be overestimated, we consider the following questions: i) What would a 10\\% opacity reduction imply for the solar neutrino puzzle? ii) Is there any hope of solving the solar neutrino puzzle by changing opacity? iii) Is a 10\\% opacity reduction testable with helioseismological data?"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9605153","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":""},"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":"astro-ph/9605153","created_at":"2026-05-18T04:21:40.653574+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9605153v1","created_at":"2026-05-18T04:21:40.653574+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9605153","created_at":"2026-05-18T04:21:40.653574+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZRMTZXJ3THOU","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZRMTZXJ3THOUYICX","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZRMTZXJ3","created_at":"2026-05-18T12:25:48.327863+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/ZRMTZXJ3THOUYICX52VGICNNC5","json":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5.json","graph_json":"https://pith.science/api/pith-number/ZRMTZXJ3THOUYICX52VGICNNC5/graph.json","events_json":"https://pith.science/api/pith-number/ZRMTZXJ3THOUYICX52VGICNNC5/events.json","paper":"https://pith.science/paper/ZRMTZXJ3"},"agent_actions":{"view_html":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5","download_json":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5.json","view_paper":"https://pith.science/paper/ZRMTZXJ3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9605153&json=true","fetch_graph":"https://pith.science/api/pith-number/ZRMTZXJ3THOUYICX52VGICNNC5/graph.json","fetch_events":"https://pith.science/api/pith-number/ZRMTZXJ3THOUYICX52VGICNNC5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5/action/storage_attestation","attest_author":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5/action/author_attestation","sign_citation":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5/action/citation_signature","submit_replication":"https://pith.science/pith/ZRMTZXJ3THOUYICX52VGICNNC5/action/replication_record"}},"created_at":"2026-05-18T04:21:40.653574+00:00","updated_at":"2026-05-18T04:21:40.653574+00:00"}