{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:NUAGQ4ZXH35ZMQZZCACBYTHTOR","short_pith_number":"pith:NUAGQ4ZX","schema_version":"1.0","canonical_sha256":"6d006873373efb96433910041c4cf374593b1ad8c951c8fab4103d10e6b3b4ff","source":{"kind":"arxiv","id":"1703.08075","version":1},"attestation_state":"computed","paper":{"title":"Domains of pulsational instability of low-frequency modes in rotating upper main-sequence stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jadwiga Daszy\\'nska-Daszkiewicz, Wojciech Szewczuk","submitted_at":"2017-03-23T13:57:32Z","abstract_excerpt":"We determine instability domains on the Hertzsprung-Russel diagram for rotating main sequence stars with masses 2-20 $\\mathrm M_\\odot$. The effects of the Coriolis force are treated in the framework of the traditional approximation. High-order g-modes with the harmonic degrees, $\\ell$, up to 4 and mixed gravity-Rossby modes with $|m|$ up to 4 are considered. Including the effects of rotation results in wider instability strips for a given $\\ell$ comparing to the non-rotating case and in an extension of the pulsational instability to hotter and more massive models. We present results for the fi"},"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":"1703.08075","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-03-23T13:57:32Z","cross_cats_sorted":[],"title_canon_sha256":"7f534c6a19e645f953c3e65f7f0ab76c0dfe8f75279de6f05d0648696b4c62ea","abstract_canon_sha256":"0b72f279f6881f279004646ec6d10f921bb8ff32f9e9cb378a5f281fed672b5a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:43:26.154184Z","signature_b64":"wGlBI/nAnOIuT9iY4L+G0/fZ68KKPACKy5tcrWPOEiCdWjyOJT84SaYGq3F6qCqmxSWg03QyI8YBfbTW4PzpAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6d006873373efb96433910041c4cf374593b1ad8c951c8fab4103d10e6b3b4ff","last_reissued_at":"2026-05-18T00:43:26.153373Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:43:26.153373Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Domains of pulsational instability of low-frequency modes in rotating upper main-sequence stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jadwiga Daszy\\'nska-Daszkiewicz, Wojciech Szewczuk","submitted_at":"2017-03-23T13:57:32Z","abstract_excerpt":"We determine instability domains on the Hertzsprung-Russel diagram for rotating main sequence stars with masses 2-20 $\\mathrm M_\\odot$. The effects of the Coriolis force are treated in the framework of the traditional approximation. High-order g-modes with the harmonic degrees, $\\ell$, up to 4 and mixed gravity-Rossby modes with $|m|$ up to 4 are considered. Including the effects of rotation results in wider instability strips for a given $\\ell$ comparing to the non-rotating case and in an extension of the pulsational instability to hotter and more massive models. We present results for the fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.08075","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":"1703.08075","created_at":"2026-05-18T00:43:26.153513+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.08075v1","created_at":"2026-05-18T00:43:26.153513+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.08075","created_at":"2026-05-18T00:43:26.153513+00:00"},{"alias_kind":"pith_short_12","alias_value":"NUAGQ4ZXH35Z","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"NUAGQ4ZXH35ZMQZZ","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"NUAGQ4ZX","created_at":"2026-05-18T12:31:34.259226+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/NUAGQ4ZXH35ZMQZZCACBYTHTOR","json":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR.json","graph_json":"https://pith.science/api/pith-number/NUAGQ4ZXH35ZMQZZCACBYTHTOR/graph.json","events_json":"https://pith.science/api/pith-number/NUAGQ4ZXH35ZMQZZCACBYTHTOR/events.json","paper":"https://pith.science/paper/NUAGQ4ZX"},"agent_actions":{"view_html":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR","download_json":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR.json","view_paper":"https://pith.science/paper/NUAGQ4ZX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.08075&json=true","fetch_graph":"https://pith.science/api/pith-number/NUAGQ4ZXH35ZMQZZCACBYTHTOR/graph.json","fetch_events":"https://pith.science/api/pith-number/NUAGQ4ZXH35ZMQZZCACBYTHTOR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR/action/storage_attestation","attest_author":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR/action/author_attestation","sign_citation":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR/action/citation_signature","submit_replication":"https://pith.science/pith/NUAGQ4ZXH35ZMQZZCACBYTHTOR/action/replication_record"}},"created_at":"2026-05-18T00:43:26.153513+00:00","updated_at":"2026-05-18T00:43:26.153513+00:00"}