{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2003:CEAH7KW2N3CPCSFOI6FE6LRDO3","short_pith_number":"pith:CEAH7KW2","canonical_record":{"source":{"id":"astro-ph/0302313","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-02-16T17:56:50Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"6fa2a82535daa3d2f09f4cbf1eb3f311ae42429c15cb5d904bcb2880c5e21ac9","abstract_canon_sha256":"d1121f9c540fa401f3d3a4532fa624a2dee4a8699214c6de7ae471ee6c308c9d"},"schema_version":"1.0"},"canonical_sha256":"11007faada6ec4f148ae478a4f2e2376e21738a44500e6dccacaae0bf8387bcc","source":{"kind":"arxiv","id":"astro-ph/0302313","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0302313","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0302313v2","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0302313","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"pith_short_12","alias_value":"CEAH7KW2N3CP","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"pith_short_16","alias_value":"CEAH7KW2N3CPCSFO","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"pith_short_8","alias_value":"CEAH7KW2","created_at":"2026-07-04T16:36:30Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2003:CEAH7KW2N3CPCSFOI6FE6LRDO3","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0302313","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-02-16T17:56:50Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"6fa2a82535daa3d2f09f4cbf1eb3f311ae42429c15cb5d904bcb2880c5e21ac9","abstract_canon_sha256":"d1121f9c540fa401f3d3a4532fa624a2dee4a8699214c6de7ae471ee6c308c9d"},"schema_version":"1.0"},"canonical_sha256":"11007faada6ec4f148ae478a4f2e2376e21738a44500e6dccacaae0bf8387bcc","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:36:30.486585Z","signature_b64":"XN5/qLJ0gJrmA4OBV5PzVJtXyV16FwWU6z+IOZrssfeBSb04xN3DMVdjyduvydxVebcMIGGx4Y/7/eC/CwWfBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"11007faada6ec4f148ae478a4f2e2376e21738a44500e6dccacaae0bf8387bcc","last_reissued_at":"2026-07-04T16:36:30.486191Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:36:30.486191Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0302313","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:36:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"+b2juXNFYtZ2xzV2R+Tde9r1TsiUWygxKsFjJJg5q0+TVlssRwCCbUNXN0wWmNnuhc2EFXNP92rRIRAFrKZBCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T18:43:30.736424Z"},"content_sha256":"20eb2d15cd31045edef54f882f211612eebdbd85fbca5a6e77eca13c0e1c312f","schema_version":"1.0","event_id":"sha256:20eb2d15cd31045edef54f882f211612eebdbd85fbca5a6e77eca13c0e1c312f"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2003:CEAH7KW2N3CPCSFOI6FE6LRDO3","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Inertial modes of neutron stars with the superfluid core","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph","authors_text":"Shijun Yoshida, Umin Lee","submitted_at":"2003-02-16T17:56:50Z","abstract_excerpt":"We investigate the modal properties of inertial modes of rotating neutron stars with the core filled with neutron and proton superfluids, taking account of entrainment effects between the superfluids. In this paper, the entrainment effects are modeled by introducing a parameter $\\eta$ so that no entrainment state is realized at $\\eta=0$. We find that inertial modes of rotating neutron stars with the superfluid core are split into two families, which we call ordinary fluid inertial modes ($i^o$-mode) and superfluid inertial modes ($i^s$-mode). The two superfluids in the core counter-move for th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0302313","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0302313/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:36:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"nZHQT1K0OYZNitz7vXadln4Gug6mfGfZ35fYwgGo7+MZZbCdBvXPIHO5egB7jEJluKuRSSIM/+vaMXKPjK11CA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T18:43:30.737030Z"},"content_sha256":"f486bb447be1866a10abf710a9cc8dabe2f36b6e4cf83cfb3358ef576061a309","schema_version":"1.0","event_id":"sha256:f486bb447be1866a10abf710a9cc8dabe2f36b6e4cf83cfb3358ef576061a309"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/CEAH7KW2N3CPCSFOI6FE6LRDO3/bundle.json","state_url":"https://pith.science/pith/CEAH7KW2N3CPCSFOI6FE6LRDO3/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/CEAH7KW2N3CPCSFOI6FE6LRDO3/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-04T18:43:30Z","links":{"resolver":"https://pith.science/pith/CEAH7KW2N3CPCSFOI6FE6LRDO3","bundle":"https://pith.science/pith/CEAH7KW2N3CPCSFOI6FE6LRDO3/bundle.json","state":"https://pith.science/pith/CEAH7KW2N3CPCSFOI6FE6LRDO3/state.json","well_known_bundle":"https://pith.science/.well-known/pith/CEAH7KW2N3CPCSFOI6FE6LRDO3/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2003:CEAH7KW2N3CPCSFOI6FE6LRDO3","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"d1121f9c540fa401f3d3a4532fa624a2dee4a8699214c6de7ae471ee6c308c9d","cross_cats_sorted":["gr-qc"],"license":"","primary_cat":"astro-ph","submitted_at":"2003-02-16T17:56:50Z","title_canon_sha256":"6fa2a82535daa3d2f09f4cbf1eb3f311ae42429c15cb5d904bcb2880c5e21ac9"},"schema_version":"1.0","source":{"id":"astro-ph/0302313","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0302313","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0302313v2","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0302313","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"pith_short_12","alias_value":"CEAH7KW2N3CP","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"pith_short_16","alias_value":"CEAH7KW2N3CPCSFO","created_at":"2026-07-04T16:36:30Z"},{"alias_kind":"pith_short_8","alias_value":"CEAH7KW2","created_at":"2026-07-04T16:36:30Z"}],"graph_snapshots":[{"event_id":"sha256:f486bb447be1866a10abf710a9cc8dabe2f36b6e4cf83cfb3358ef576061a309","target":"graph","created_at":"2026-07-04T16:36:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/astro-ph/0302313/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We investigate the modal properties of inertial modes of rotating neutron stars with the core filled with neutron and proton superfluids, taking account of entrainment effects between the superfluids. In this paper, the entrainment effects are modeled by introducing a parameter $\\eta$ so that no entrainment state is realized at $\\eta=0$. We find that inertial modes of rotating neutron stars with the superfluid core are split into two families, which we call ordinary fluid inertial modes ($i^o$-mode) and superfluid inertial modes ($i^s$-mode). The two superfluids in the core counter-move for th","authors_text":"Shijun Yoshida, Umin Lee","cross_cats":["gr-qc"],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2003-02-16T17:56:50Z","title":"Inertial modes of neutron stars with the superfluid core"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0302313","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:20eb2d15cd31045edef54f882f211612eebdbd85fbca5a6e77eca13c0e1c312f","target":"record","created_at":"2026-07-04T16:36:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"d1121f9c540fa401f3d3a4532fa624a2dee4a8699214c6de7ae471ee6c308c9d","cross_cats_sorted":["gr-qc"],"license":"","primary_cat":"astro-ph","submitted_at":"2003-02-16T17:56:50Z","title_canon_sha256":"6fa2a82535daa3d2f09f4cbf1eb3f311ae42429c15cb5d904bcb2880c5e21ac9"},"schema_version":"1.0","source":{"id":"astro-ph/0302313","kind":"arxiv","version":2}},"canonical_sha256":"11007faada6ec4f148ae478a4f2e2376e21738a44500e6dccacaae0bf8387bcc","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"11007faada6ec4f148ae478a4f2e2376e21738a44500e6dccacaae0bf8387bcc","first_computed_at":"2026-07-04T16:36:30.486191Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T16:36:30.486191Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"XN5/qLJ0gJrmA4OBV5PzVJtXyV16FwWU6z+IOZrssfeBSb04xN3DMVdjyduvydxVebcMIGGx4Y/7/eC/CwWfBg==","signature_status":"signed_v1","signed_at":"2026-07-04T16:36:30.486585Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0302313","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:20eb2d15cd31045edef54f882f211612eebdbd85fbca5a6e77eca13c0e1c312f","sha256:f486bb447be1866a10abf710a9cc8dabe2f36b6e4cf83cfb3358ef576061a309"],"state_sha256":"57d11b30483c4decce080d5d1c040758677fe62d021fa65828a576495b78237d"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"z2bHUDHB/B0/AQZbRMPEI4BQIv/utG+khouApyWWkRgNMcytYD8rvAEoBPxbRVowjzGtDj4c36wuxufE6f+6CQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-04T18:43:30.769741Z","bundle_sha256":"1730b876b66fd041ff871a552e043aca8b55287d62bc9aa497204fc65552d0e4"}}