{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:MJM7EXMF2TDUVHSBCZKJ7BP4CL","short_pith_number":"pith:MJM7EXMF","schema_version":"1.0","canonical_sha256":"6259f25d85d4c74a9e4116549f85fc12d6f4230bcb82f480703ca91953ce6521","source":{"kind":"arxiv","id":"1110.4423","version":1},"attestation_state":"computed","paper":{"title":"Relativistic Binaries in Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.SR","authors_text":"Jonathan M. B. Downing, Matthew J. Benacquista","submitted_at":"2011-10-20T02:06:38Z","abstract_excerpt":"Galactic globular clusters are old, dense star systems typically containing 10\\super{4}--10\\super{7} stars. As an old population of stars, globular clusters contain many collapsed and degenerate objects. As a dense population of stars, globular clusters are the scene of many interesting close dynamical interactions between stars. These dynamical interactions can alter the evolution of individual stars and can produce tight binary systems containing one or two compact objects. In this review, we discuss theoretical models of globular cluster evolution and binary evolution, techniques for simula"},"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":"1110.4423","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-10-20T02:06:38Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"ca893fe4f2059c5885535841a599066bad93b6d14e963bb08f60bcb04b779c48","abstract_canon_sha256":"3600e6ae08ed97584f92ad0251eaee20a3f6057c3f2b4c834203f69da4ca1b23"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:08.201985Z","signature_b64":"2zH0koFMG1G5ZqN/odFvyitmH384X9AbukeQbCIwOySv1lf7W1Bg+FNgUNMmVui0P4XjLremAyA+/hHxRjdYDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6259f25d85d4c74a9e4116549f85fc12d6f4230bcb82f480703ca91953ce6521","last_reissued_at":"2026-05-18T02:00:08.201300Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:08.201300Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relativistic Binaries in Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.SR","authors_text":"Jonathan M. B. Downing, Matthew J. Benacquista","submitted_at":"2011-10-20T02:06:38Z","abstract_excerpt":"Galactic globular clusters are old, dense star systems typically containing 10\\super{4}--10\\super{7} stars. As an old population of stars, globular clusters contain many collapsed and degenerate objects. As a dense population of stars, globular clusters are the scene of many interesting close dynamical interactions between stars. These dynamical interactions can alter the evolution of individual stars and can produce tight binary systems containing one or two compact objects. In this review, we discuss theoretical models of globular cluster evolution and binary evolution, techniques for simula"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1110.4423","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":"1110.4423","created_at":"2026-05-18T02:00:08.201434+00:00"},{"alias_kind":"arxiv_version","alias_value":"1110.4423v1","created_at":"2026-05-18T02:00:08.201434+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1110.4423","created_at":"2026-05-18T02:00:08.201434+00:00"},{"alias_kind":"pith_short_12","alias_value":"MJM7EXMF2TDU","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_16","alias_value":"MJM7EXMF2TDUVHSB","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_8","alias_value":"MJM7EXMF","created_at":"2026-05-18T12:26:34.985390+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.23663","citing_title":"Disentangling spinning and nonspinning binary black hole populations with spin sorting","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL","json":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL.json","graph_json":"https://pith.science/api/pith-number/MJM7EXMF2TDUVHSBCZKJ7BP4CL/graph.json","events_json":"https://pith.science/api/pith-number/MJM7EXMF2TDUVHSBCZKJ7BP4CL/events.json","paper":"https://pith.science/paper/MJM7EXMF"},"agent_actions":{"view_html":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL","download_json":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL.json","view_paper":"https://pith.science/paper/MJM7EXMF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1110.4423&json=true","fetch_graph":"https://pith.science/api/pith-number/MJM7EXMF2TDUVHSBCZKJ7BP4CL/graph.json","fetch_events":"https://pith.science/api/pith-number/MJM7EXMF2TDUVHSBCZKJ7BP4CL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL/action/storage_attestation","attest_author":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL/action/author_attestation","sign_citation":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL/action/citation_signature","submit_replication":"https://pith.science/pith/MJM7EXMF2TDUVHSBCZKJ7BP4CL/action/replication_record"}},"created_at":"2026-05-18T02:00:08.201434+00:00","updated_at":"2026-05-18T02:00:08.201434+00:00"}