{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1999:RZT2NR5ERIHEDGCAAF4YUY624W","short_pith_number":"pith:RZT2NR5E","schema_version":"1.0","canonical_sha256":"8e67a6c7a48a0e41984001798a63dae59cce443ac7a8b33485c5efc73a89aaba","source":{"kind":"arxiv","id":"gr-qc/9911034","version":1},"attestation_state":"computed","paper":{"title":"Gravitational wave astronomy","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bernard F Schutz","submitted_at":"1999-11-09T19:32:52Z","abstract_excerpt":"The first decade of the new millenium should see the first direct detections of gravitational waves. This will be a milestone for fundamental physics and it will open the new observational science of gravitational wave astronomy. But gravitational waves already play an important role in the modeling of astrophysical systems. I review here the present state of gravitational radiation theory in relativity and astrophysics, and I then look at the development of detector sensitivity over the next decade, both on the ground (such as LIGO) and in space (LISA). I review the sources of gravitational w"},"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":"gr-qc/9911034","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1999-11-09T19:32:52Z","cross_cats_sorted":[],"title_canon_sha256":"dabf65639744ea0468f39aa1d6e1f2938cd96787d32c8542185c24f2cce5c07b","abstract_canon_sha256":"0c5cc65607d7de6f261cd8061f769ab0199db84b7092ab07267947c2193bbc63"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:25:20.168161Z","signature_b64":"vI3OhSQ/QWaqfTpx3B0igzaxXEZr9qZYcrMCyoMWJFOIBdXkYfUrKSbAI8eT8orWCD+jZ0x6BNrRopDsBa0jBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8e67a6c7a48a0e41984001798a63dae59cce443ac7a8b33485c5efc73a89aaba","last_reissued_at":"2026-07-04T17:25:20.167718Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:25:20.167718Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational wave astronomy","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bernard F Schutz","submitted_at":"1999-11-09T19:32:52Z","abstract_excerpt":"The first decade of the new millenium should see the first direct detections of gravitational waves. This will be a milestone for fundamental physics and it will open the new observational science of gravitational wave astronomy. But gravitational waves already play an important role in the modeling of astrophysical systems. I review here the present state of gravitational radiation theory in relativity and astrophysics, and I then look at the development of detector sensitivity over the next decade, both on the ground (such as LIGO) and in space (LISA). I review the sources of gravitational w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9911034","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/gr-qc/9911034/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":"gr-qc/9911034","created_at":"2026-07-04T17:25:20.167785+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9911034v1","created_at":"2026-07-04T17:25:20.167785+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9911034","created_at":"2026-07-04T17:25:20.167785+00:00"},{"alias_kind":"pith_short_12","alias_value":"RZT2NR5ERIHE","created_at":"2026-07-04T17:25:20.167785+00:00"},{"alias_kind":"pith_short_16","alias_value":"RZT2NR5ERIHEDGCA","created_at":"2026-07-04T17:25:20.167785+00:00"},{"alias_kind":"pith_short_8","alias_value":"RZT2NR5E","created_at":"2026-07-04T17:25:20.167785+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2606.23021","citing_title":"Periodic Timelike Motion and Gravitational Wave Signatures around a Magnetically Charged Black Hole Surrounded by Quintessence","ref_index":26,"is_internal_anchor":true},{"citing_arxiv_id":"2606.11728","citing_title":"Periodic orbits as probes of charged loop quantum gravity black holes through gravitational waves","ref_index":83,"is_internal_anchor":true},{"citing_arxiv_id":"2601.00550","citing_title":"Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2605.07187","citing_title":"Probing Gravitational Wave Signatures from Periodic Orbits of Regular Black Holes in Asymptotically Safe Gravity","ref_index":10,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W","json":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W.json","graph_json":"https://pith.science/api/pith-number/RZT2NR5ERIHEDGCAAF4YUY624W/graph.json","events_json":"https://pith.science/api/pith-number/RZT2NR5ERIHEDGCAAF4YUY624W/events.json","paper":"https://pith.science/paper/RZT2NR5E"},"agent_actions":{"view_html":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W","download_json":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W.json","view_paper":"https://pith.science/paper/RZT2NR5E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/9911034&json=true","fetch_graph":"https://pith.science/api/pith-number/RZT2NR5ERIHEDGCAAF4YUY624W/graph.json","fetch_events":"https://pith.science/api/pith-number/RZT2NR5ERIHEDGCAAF4YUY624W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W/action/storage_attestation","attest_author":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W/action/author_attestation","sign_citation":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W/action/citation_signature","submit_replication":"https://pith.science/pith/RZT2NR5ERIHEDGCAAF4YUY624W/action/replication_record"}},"created_at":"2026-07-04T17:25:20.167785+00:00","updated_at":"2026-07-04T17:25:20.167785+00:00"}