{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:XBASZAGC6VCNMZGXMWEBDOYCJI","short_pith_number":"pith:XBASZAGC","schema_version":"1.0","canonical_sha256":"b8412c80c2f544d664d7658811bb024a120030b5e6b588c6563c6629b6e34abd","source":{"kind":"arxiv","id":"1608.03041","version":1},"attestation_state":"computed","paper":{"title":"The Effect of Tides on the Population of PN from Interacting Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Eva Villaver, Niyas Madappatt, Orsola De Marco","submitted_at":"2016-08-10T04:29:21Z","abstract_excerpt":"We have used the tidal equations of Zahn to determine the maximum orbital distance at which companions are brought into Roche lobe contact with their giant primary, when the primary expands during the giant phases. This is a key step when determining the rates of interaction between giants and their companions. Our stellar structure calculations are presented as maximum radii reached during the red and asymptotic giant branch (RGB and AGB, respectively) stages of evolution for masses between 0.8 and 4.0 Mo (Z=0.001 - 0.04) and compared with other models to gauge the uncertainty on radii derivi"},"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":"1608.03041","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-08-10T04:29:21Z","cross_cats_sorted":[],"title_canon_sha256":"2726be384aef60b28740ec43fa28d70236c7e37f836b5374e8ce985c16965ee8","abstract_canon_sha256":"8fc81ddf98f6b4bba651cf380793caea01b2032f020512599687b1696bc76ff7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:08:37.420421Z","signature_b64":"swWXWRelCJqd2o9AVkQR/2ovn9qwMHOBqBiyz1eQbH44ZseQGsepxAgLZ2O2T+FVYPxgzMJxADFZ3cOyYPF1Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b8412c80c2f544d664d7658811bb024a120030b5e6b588c6563c6629b6e34abd","last_reissued_at":"2026-05-18T01:08:37.419720Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:08:37.419720Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Effect of Tides on the Population of PN from Interacting Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Eva Villaver, Niyas Madappatt, Orsola De Marco","submitted_at":"2016-08-10T04:29:21Z","abstract_excerpt":"We have used the tidal equations of Zahn to determine the maximum orbital distance at which companions are brought into Roche lobe contact with their giant primary, when the primary expands during the giant phases. This is a key step when determining the rates of interaction between giants and their companions. Our stellar structure calculations are presented as maximum radii reached during the red and asymptotic giant branch (RGB and AGB, respectively) stages of evolution for masses between 0.8 and 4.0 Mo (Z=0.001 - 0.04) and compared with other models to gauge the uncertainty on radii derivi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.03041","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":"1608.03041","created_at":"2026-05-18T01:08:37.419821+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.03041v1","created_at":"2026-05-18T01:08:37.419821+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.03041","created_at":"2026-05-18T01:08:37.419821+00:00"},{"alias_kind":"pith_short_12","alias_value":"XBASZAGC6VCN","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"XBASZAGC6VCNMZGX","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"XBASZAGC","created_at":"2026-05-18T12:30:51.357362+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/XBASZAGC6VCNMZGXMWEBDOYCJI","json":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI.json","graph_json":"https://pith.science/api/pith-number/XBASZAGC6VCNMZGXMWEBDOYCJI/graph.json","events_json":"https://pith.science/api/pith-number/XBASZAGC6VCNMZGXMWEBDOYCJI/events.json","paper":"https://pith.science/paper/XBASZAGC"},"agent_actions":{"view_html":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI","download_json":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI.json","view_paper":"https://pith.science/paper/XBASZAGC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.03041&json=true","fetch_graph":"https://pith.science/api/pith-number/XBASZAGC6VCNMZGXMWEBDOYCJI/graph.json","fetch_events":"https://pith.science/api/pith-number/XBASZAGC6VCNMZGXMWEBDOYCJI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI/action/storage_attestation","attest_author":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI/action/author_attestation","sign_citation":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI/action/citation_signature","submit_replication":"https://pith.science/pith/XBASZAGC6VCNMZGXMWEBDOYCJI/action/replication_record"}},"created_at":"2026-05-18T01:08:37.419821+00:00","updated_at":"2026-05-18T01:08:37.419821+00:00"}