{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:N5PKHMDNELPLEZWEITAIR53N2Q","short_pith_number":"pith:N5PKHMDN","schema_version":"1.0","canonical_sha256":"6f5ea3b06d22deb266c444c088f76dd4011fbaf43cac845962072c7532dedb7b","source":{"kind":"arxiv","id":"2607.10834","version":1},"attestation_state":"computed","paper":{"title":"Asteroseismic forward modelling of 36 $\\beta$ Cep pulsators and inferences on their internal differential rotation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Conny Aerts, Dario J. Fritzewski, Mathijs Vanrespaille, Vincent Vanlaer","submitted_at":"2026-07-12T16:49:31Z","abstract_excerpt":"Asteroseismic observations of the interior rotation of main sequence stars have shown that angular momentum transport is much more efficient than expected. Which transport mechanisms are responsible for this is still unclear. Detections of radial differential rotation provide valuable constraints on these transport mechanisms. This has been detected in several massive main sequence $\\beta$ Cep pulsators, even though fewer than ten $\\beta$ Cep stars have been asteroseismically modelled in detail so far. We aim to expand the sample of asteroseismically forward modelled $\\beta$ Cep pulsators to m"},"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":"2607.10834","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-07-12T16:49:31Z","cross_cats_sorted":[],"title_canon_sha256":"601065f7a35f228d8e479bdd93570109deae773bf8048e64b5677df658f0d14a","abstract_canon_sha256":"e1d17d3da0d0d74f8718580be2bf77b4b3cede451218b4eccd1049aa523879f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-14T01:21:42.626885Z","signature_b64":"BHVlf4UdyyeFCMwNv2D0CaBKINC2Rv1nAArx8dCruOcQtDNBxHwCRBZVH6o3rKNgcUVUba7LVewkjysoHWuTDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6f5ea3b06d22deb266c444c088f76dd4011fbaf43cac845962072c7532dedb7b","last_reissued_at":"2026-07-14T01:21:42.625943Z","signature_status":"signed_v1","first_computed_at":"2026-07-14T01:21:42.625943Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Asteroseismic forward modelling of 36 $\\beta$ Cep pulsators and inferences on their internal differential rotation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Conny Aerts, Dario J. Fritzewski, Mathijs Vanrespaille, Vincent Vanlaer","submitted_at":"2026-07-12T16:49:31Z","abstract_excerpt":"Asteroseismic observations of the interior rotation of main sequence stars have shown that angular momentum transport is much more efficient than expected. Which transport mechanisms are responsible for this is still unclear. Detections of radial differential rotation provide valuable constraints on these transport mechanisms. This has been detected in several massive main sequence $\\beta$ Cep pulsators, even though fewer than ten $\\beta$ Cep stars have been asteroseismically modelled in detail so far. We aim to expand the sample of asteroseismically forward modelled $\\beta$ Cep pulsators to m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.10834","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/2607.10834/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":"2607.10834","created_at":"2026-07-14T01:21:42.626369+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.10834v1","created_at":"2026-07-14T01:21:42.626369+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.10834","created_at":"2026-07-14T01:21:42.626369+00:00"},{"alias_kind":"pith_short_12","alias_value":"N5PKHMDNELPL","created_at":"2026-07-14T01:21:42.626369+00:00"},{"alias_kind":"pith_short_16","alias_value":"N5PKHMDNELPLEZWE","created_at":"2026-07-14T01:21:42.626369+00:00"},{"alias_kind":"pith_short_8","alias_value":"N5PKHMDN","created_at":"2026-07-14T01:21:42.626369+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/N5PKHMDNELPLEZWEITAIR53N2Q","json":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q.json","graph_json":"https://pith.science/api/pith-number/N5PKHMDNELPLEZWEITAIR53N2Q/graph.json","events_json":"https://pith.science/api/pith-number/N5PKHMDNELPLEZWEITAIR53N2Q/events.json","paper":"https://pith.science/paper/N5PKHMDN"},"agent_actions":{"view_html":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q","download_json":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q.json","view_paper":"https://pith.science/paper/N5PKHMDN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.10834&json=true","fetch_graph":"https://pith.science/api/pith-number/N5PKHMDNELPLEZWEITAIR53N2Q/graph.json","fetch_events":"https://pith.science/api/pith-number/N5PKHMDNELPLEZWEITAIR53N2Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q/action/storage_attestation","attest_author":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q/action/author_attestation","sign_citation":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q/action/citation_signature","submit_replication":"https://pith.science/pith/N5PKHMDNELPLEZWEITAIR53N2Q/action/replication_record"}},"created_at":"2026-07-14T01:21:42.626369+00:00","updated_at":"2026-07-14T01:21:42.626369+00:00"}