{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:1997:BJLU3QYL57K3XQB4WRX3R5HVR5","short_pith_number":"pith:BJLU3QYL","canonical_record":{"source":{"id":"gr-qc/9710121","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1997-10-28T14:53:38Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"c46f2b3d431fd3942d44639ab2410bf6352d8e8c3ae65b465f13817a0235cf7a","abstract_canon_sha256":"28e03fb5f4715634882627844acae559be7fa5b76e055423b837679ee2de7cc9"},"schema_version":"1.0"},"canonical_sha256":"0a574dc30befd5bbc03cb46fb8f4f58f70671c2f057ae54935ae35e2412f6891","source":{"kind":"arxiv","id":"gr-qc/9710121","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"gr-qc/9710121","created_at":"2026-05-18T04:21:31Z"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9710121v1","created_at":"2026-05-18T04:21:31Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9710121","created_at":"2026-05-18T04:21:31Z"},{"alias_kind":"pith_short_12","alias_value":"BJLU3QYL57K3","created_at":"2026-05-18T12:25:48Z"},{"alias_kind":"pith_short_16","alias_value":"BJLU3QYL57K3XQB4","created_at":"2026-05-18T12:25:48Z"},{"alias_kind":"pith_short_8","alias_value":"BJLU3QYL","created_at":"2026-05-18T12:25:48Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:1997:BJLU3QYL57K3XQB4WRX3R5HVR5","target":"record","payload":{"canonical_record":{"source":{"id":"gr-qc/9710121","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1997-10-28T14:53:38Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"c46f2b3d431fd3942d44639ab2410bf6352d8e8c3ae65b465f13817a0235cf7a","abstract_canon_sha256":"28e03fb5f4715634882627844acae559be7fa5b76e055423b837679ee2de7cc9"},"schema_version":"1.0"},"canonical_sha256":"0a574dc30befd5bbc03cb46fb8f4f58f70671c2f057ae54935ae35e2412f6891","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:21:31.864583Z","signature_b64":"0l3EmgedjO7ENSWDUAJdP4SGb5V1pg2QgL/xAuzX3e81ywQ1tuPowupqxNPzkDg+ZlA7Pixj2rIRq70CbiWuDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0a574dc30befd5bbc03cb46fb8f4f58f70671c2f057ae54935ae35e2412f6891","last_reissued_at":"2026-05-18T04:21:31.864160Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:21:31.864160Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"gr-qc/9710121","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:21:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Q7UzVIVNuxN5L0V89naNevg4NyLkl5UMeM9qfR+3I2JP0i33Wmvs8kF95FMNDGA7V3huFxv/SZDjcwqS3s3yAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T18:44:08.404530Z"},"content_sha256":"e1d254896d7fe0b147558db0463c95e9c3e29109883aaeb0f706780505a0b2fa","schema_version":"1.0","event_id":"sha256:e1d254896d7fe0b147558db0463c95e9c3e29109883aaeb0f706780505a0b2fa"},{"event_type":"graph_snapshot","subject_pith_number":"pith:1997:BJLU3QYL57K3XQB4WRX3R5HVR5","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Spontaneous symmetry breaking of rapidly rotating stars in general relativity: influence of the 3D-shift vector","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"gr-qc","authors_text":"CNRS, E. Gourgoulhon (DARC, France), J. Frieben, Observatoire de Paris, S. Bonazzola","submitted_at":"1997-10-28T14:53:38Z","abstract_excerpt":"An analytical scheme and a numerical method in order to study the effects of general relativity on the viscosity driven secular bar mode instability of rapidly rotating stars are presented. The approach consists in perturbing an axisymmetric and stationary configuration and studying its evolution by constructing a series of triaxial quasi-equilibrium configurations. These are obtained by solution of an approximate set of field equations where only the dominant non-axisymmetric terms are taken into account. The progress with respect to our former investigation consists in a higher relativistic "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9710121","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:21:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2n48+dv7wElZM1rH5C0zuGJBQLTwsLNrqHYtEkcS07WOi8N0xDX9VS1XKcw/5C4NhHYALuxBPTcE3ze6+ZrRCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T18:44:08.405225Z"},"content_sha256":"f16416265504ae0bcfa89be1de6777e81833e4c4b9331045652b74c43ee5fef6","schema_version":"1.0","event_id":"sha256:f16416265504ae0bcfa89be1de6777e81833e4c4b9331045652b74c43ee5fef6"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/BJLU3QYL57K3XQB4WRX3R5HVR5/bundle.json","state_url":"https://pith.science/pith/BJLU3QYL57K3XQB4WRX3R5HVR5/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/BJLU3QYL57K3XQB4WRX3R5HVR5/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":"2026-05-25T18:44:08Z","links":{"resolver":"https://pith.science/pith/BJLU3QYL57K3XQB4WRX3R5HVR5","bundle":"https://pith.science/pith/BJLU3QYL57K3XQB4WRX3R5HVR5/bundle.json","state":"https://pith.science/pith/BJLU3QYL57K3XQB4WRX3R5HVR5/state.json","well_known_bundle":"https://pith.science/.well-known/pith/BJLU3QYL57K3XQB4WRX3R5HVR5/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:1997:BJLU3QYL57K3XQB4WRX3R5HVR5","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":"28e03fb5f4715634882627844acae559be7fa5b76e055423b837679ee2de7cc9","cross_cats_sorted":["astro-ph"],"license":"","primary_cat":"gr-qc","submitted_at":"1997-10-28T14:53:38Z","title_canon_sha256":"c46f2b3d431fd3942d44639ab2410bf6352d8e8c3ae65b465f13817a0235cf7a"},"schema_version":"1.0","source":{"id":"gr-qc/9710121","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"gr-qc/9710121","created_at":"2026-05-18T04:21:31Z"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9710121v1","created_at":"2026-05-18T04:21:31Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9710121","created_at":"2026-05-18T04:21:31Z"},{"alias_kind":"pith_short_12","alias_value":"BJLU3QYL57K3","created_at":"2026-05-18T12:25:48Z"},{"alias_kind":"pith_short_16","alias_value":"BJLU3QYL57K3XQB4","created_at":"2026-05-18T12:25:48Z"},{"alias_kind":"pith_short_8","alias_value":"BJLU3QYL","created_at":"2026-05-18T12:25:48Z"}],"graph_snapshots":[{"event_id":"sha256:f16416265504ae0bcfa89be1de6777e81833e4c4b9331045652b74c43ee5fef6","target":"graph","created_at":"2026-05-18T04:21:31Z","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"},"paper":{"abstract_excerpt":"An analytical scheme and a numerical method in order to study the effects of general relativity on the viscosity driven secular bar mode instability of rapidly rotating stars are presented. The approach consists in perturbing an axisymmetric and stationary configuration and studying its evolution by constructing a series of triaxial quasi-equilibrium configurations. These are obtained by solution of an approximate set of field equations where only the dominant non-axisymmetric terms are taken into account. The progress with respect to our former investigation consists in a higher relativistic ","authors_text":"CNRS, E. Gourgoulhon (DARC, France), J. Frieben, Observatoire de Paris, S. Bonazzola","cross_cats":["astro-ph"],"headline":"","license":"","primary_cat":"gr-qc","submitted_at":"1997-10-28T14:53:38Z","title":"Spontaneous symmetry breaking of rapidly rotating stars in general relativity: influence of the 3D-shift vector"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9710121","kind":"arxiv","version":1},"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:e1d254896d7fe0b147558db0463c95e9c3e29109883aaeb0f706780505a0b2fa","target":"record","created_at":"2026-05-18T04:21:31Z","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":"28e03fb5f4715634882627844acae559be7fa5b76e055423b837679ee2de7cc9","cross_cats_sorted":["astro-ph"],"license":"","primary_cat":"gr-qc","submitted_at":"1997-10-28T14:53:38Z","title_canon_sha256":"c46f2b3d431fd3942d44639ab2410bf6352d8e8c3ae65b465f13817a0235cf7a"},"schema_version":"1.0","source":{"id":"gr-qc/9710121","kind":"arxiv","version":1}},"canonical_sha256":"0a574dc30befd5bbc03cb46fb8f4f58f70671c2f057ae54935ae35e2412f6891","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"0a574dc30befd5bbc03cb46fb8f4f58f70671c2f057ae54935ae35e2412f6891","first_computed_at":"2026-05-18T04:21:31.864160Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:21:31.864160Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"0l3EmgedjO7ENSWDUAJdP4SGb5V1pg2QgL/xAuzX3e81ywQ1tuPowupqxNPzkDg+ZlA7Pixj2rIRq70CbiWuDw==","signature_status":"signed_v1","signed_at":"2026-05-18T04:21:31.864583Z","signed_message":"canonical_sha256_bytes"},"source_id":"gr-qc/9710121","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:e1d254896d7fe0b147558db0463c95e9c3e29109883aaeb0f706780505a0b2fa","sha256:f16416265504ae0bcfa89be1de6777e81833e4c4b9331045652b74c43ee5fef6"],"state_sha256":"0d06ca4335733124f9840135d78b25c7b34e753ff94357dc28784662072d3228"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7j4TnJRf2i30FEqLrQjQeMIrr0B0uw2AlRZbNQVC8dRvoxYCzKHPvhO1FQ3lty7q013EXaGsAGrY0WkLmHSuBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T18:44:08.409128Z","bundle_sha256":"eeb02f9b98569aeb0ffd767bdcdd0c3d9872efa7ee99571e35cbf9ed4154d168"}}