{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:EIUZA55N3WITBUGSZCXXRETETA","short_pith_number":"pith:EIUZA55N","schema_version":"1.0","canonical_sha256":"22299077addd9130d0d2c8af789264980a7e4cdb62ef7058e073286a9d194264","source":{"kind":"arxiv","id":"gr-qc/0602078","version":2},"attestation_state":"computed","paper":{"title":"Evolution of 3D Boson Stars with Waveform Extraction","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Edward Seidel, F. Siddhartha Guzman, Gregory Daues, Jayashree Balakrishna, Ruxandra Bondarescu","submitted_at":"2006-02-20T20:48:11Z","abstract_excerpt":"Numerical results from a study of boson stars under nonspherical perturbations using a fully general relativistic 3D code are presented together with the analysis of emitted gravitational radiation. We have constructed a simulation code suitable for the study of scalar fields in space-times of general symmetry by bringing together components for addressing the initial value problem, the full evolution system and the detection and analysis of gravitational waves. Within a series of numerical simulations, we explicitly extract the Zerilli and Newman-Penrose scalar $\\Psi_4$ gravitational waveform"},"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/0602078","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2006-02-20T20:48:11Z","cross_cats_sorted":[],"title_canon_sha256":"253c00e13b6bd35901f42a09a4659b021900308764b325de44f2f39b0a00a128","abstract_canon_sha256":"455965270c67a2b5f2021230323c2bfd5240814014c6a4bebb109f5c8e7001f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:39:20.143638Z","signature_b64":"QACjNMKjt3lR9dtCEZxutfDt9GabHKS3MBygC3hOmqF6iE3aV3+unD8dEoKekFBpTU+dowsBbgzkCee8vhQvAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"22299077addd9130d0d2c8af789264980a7e4cdb62ef7058e073286a9d194264","last_reissued_at":"2026-05-18T01:39:20.142978Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:39:20.142978Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evolution of 3D Boson Stars with Waveform Extraction","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Edward Seidel, F. Siddhartha Guzman, Gregory Daues, Jayashree Balakrishna, Ruxandra Bondarescu","submitted_at":"2006-02-20T20:48:11Z","abstract_excerpt":"Numerical results from a study of boson stars under nonspherical perturbations using a fully general relativistic 3D code are presented together with the analysis of emitted gravitational radiation. We have constructed a simulation code suitable for the study of scalar fields in space-times of general symmetry by bringing together components for addressing the initial value problem, the full evolution system and the detection and analysis of gravitational waves. Within a series of numerical simulations, we explicitly extract the Zerilli and Newman-Penrose scalar $\\Psi_4$ gravitational waveform"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0602078","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":""},"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/0602078","created_at":"2026-05-18T01:39:20.143089+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0602078v2","created_at":"2026-05-18T01:39:20.143089+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0602078","created_at":"2026-05-18T01:39:20.143089+00:00"},{"alias_kind":"pith_short_12","alias_value":"EIUZA55N3WIT","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"EIUZA55N3WITBUGS","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"EIUZA55N","created_at":"2026-05-18T12:25:53.939244+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"1907.08193","citing_title":"The three dynamical fates of Boson Stars","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19572","citing_title":"Timing-Window Mechanism for Chain-Like Transients in Collisions of Radially Excited Boson Stars","ref_index":13,"is_internal_anchor":true},{"citing_arxiv_id":"2512.15242","citing_title":"Massive boson stars: Stability and GW emission in head-on mergers","ref_index":27,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA","json":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA.json","graph_json":"https://pith.science/api/pith-number/EIUZA55N3WITBUGSZCXXRETETA/graph.json","events_json":"https://pith.science/api/pith-number/EIUZA55N3WITBUGSZCXXRETETA/events.json","paper":"https://pith.science/paper/EIUZA55N"},"agent_actions":{"view_html":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA","download_json":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA.json","view_paper":"https://pith.science/paper/EIUZA55N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0602078&json=true","fetch_graph":"https://pith.science/api/pith-number/EIUZA55N3WITBUGSZCXXRETETA/graph.json","fetch_events":"https://pith.science/api/pith-number/EIUZA55N3WITBUGSZCXXRETETA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA/action/storage_attestation","attest_author":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA/action/author_attestation","sign_citation":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA/action/citation_signature","submit_replication":"https://pith.science/pith/EIUZA55N3WITBUGSZCXXRETETA/action/replication_record"}},"created_at":"2026-05-18T01:39:20.143089+00:00","updated_at":"2026-05-18T01:39:20.143089+00:00"}