{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:F3XVLF3XFOL5NFEMK4ZR27U4XG","short_pith_number":"pith:F3XVLF3X","schema_version":"1.0","canonical_sha256":"2eef5597772b97d6948c57331d7e9cb98e2c9ca01beb4ff9e3fe02db0c39ea40","source":{"kind":"arxiv","id":"1711.03138","version":2},"attestation_state":"computed","paper":{"title":"Planet Formation in Disks with Inclined Binary Companions: Can Primordial Spin-Orbit Misalignment be Produced?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Dong Lai, J. J. Zanazzi","submitted_at":"2017-11-08T20:04:01Z","abstract_excerpt":"Many hot Jupiter (HJ) systems have been observed to have their stellar spin axis misaligned with the planet's orbital angular momentum axis. The origin of this spin-orbit misalignment and the formation mechanism of HJs remain poorly understood. A number of recent works have suggested that gravitational interactions between host stars, protoplanetary disks, and inclined binary companions may tilt the stellar spin axis with respect to the disk's angular angular momentum axis, producing planetary systems with misaligned orbits. These previous works considered idealized disk evolution models and n"},"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":"1711.03138","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-11-08T20:04:01Z","cross_cats_sorted":[],"title_canon_sha256":"752d196320ea800b6962a0209bc2ef8769ca61e5e9cb56bcea6c16e5a9148568","abstract_canon_sha256":"dcdf2a04ce15179c9c43aff57b77dccb3a0466d0cefbf7ac4e849aab89c96c45"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:17:27.105067Z","signature_b64":"VH22DrELiBniE/ilD3GNAlBmteC5dSXNiV+LiGvTe9jtYIiL9vR6urFteZFIU3u8ppsPvqxSy9jnmMibwkjxAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2eef5597772b97d6948c57331d7e9cb98e2c9ca01beb4ff9e3fe02db0c39ea40","last_reissued_at":"2026-05-18T00:17:27.104535Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:17:27.104535Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planet Formation in Disks with Inclined Binary Companions: Can Primordial Spin-Orbit Misalignment be Produced?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Dong Lai, J. J. Zanazzi","submitted_at":"2017-11-08T20:04:01Z","abstract_excerpt":"Many hot Jupiter (HJ) systems have been observed to have their stellar spin axis misaligned with the planet's orbital angular momentum axis. The origin of this spin-orbit misalignment and the formation mechanism of HJs remain poorly understood. A number of recent works have suggested that gravitational interactions between host stars, protoplanetary disks, and inclined binary companions may tilt the stellar spin axis with respect to the disk's angular angular momentum axis, producing planetary systems with misaligned orbits. These previous works considered idealized disk evolution models and n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.03138","kind":"arxiv","version":2},"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":"1711.03138","created_at":"2026-05-18T00:17:27.104619+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.03138v2","created_at":"2026-05-18T00:17:27.104619+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.03138","created_at":"2026-05-18T00:17:27.104619+00:00"},{"alias_kind":"pith_short_12","alias_value":"F3XVLF3XFOL5","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"F3XVLF3XFOL5NFEM","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"F3XVLF3X","created_at":"2026-05-18T12:31:15.632608+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.20803","citing_title":"Planet-Planet Secular Migration Predicts a Stellar Obliquity-Period Anti-Correlation","ref_index":83,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG","json":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG.json","graph_json":"https://pith.science/api/pith-number/F3XVLF3XFOL5NFEMK4ZR27U4XG/graph.json","events_json":"https://pith.science/api/pith-number/F3XVLF3XFOL5NFEMK4ZR27U4XG/events.json","paper":"https://pith.science/paper/F3XVLF3X"},"agent_actions":{"view_html":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG","download_json":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG.json","view_paper":"https://pith.science/paper/F3XVLF3X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.03138&json=true","fetch_graph":"https://pith.science/api/pith-number/F3XVLF3XFOL5NFEMK4ZR27U4XG/graph.json","fetch_events":"https://pith.science/api/pith-number/F3XVLF3XFOL5NFEMK4ZR27U4XG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG/action/storage_attestation","attest_author":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG/action/author_attestation","sign_citation":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG/action/citation_signature","submit_replication":"https://pith.science/pith/F3XVLF3XFOL5NFEMK4ZR27U4XG/action/replication_record"}},"created_at":"2026-05-18T00:17:27.104619+00:00","updated_at":"2026-05-18T00:17:27.104619+00:00"}