{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:GAIQK5NE7LUXLQIKGIINE6QV6L","short_pith_number":"pith:GAIQK5NE","schema_version":"1.0","canonical_sha256":"30110575a4fae975c10a3210d27a15f2d230d9188fb5aae59535bb4a0bbc24f5","source":{"kind":"arxiv","id":"1802.08654","version":1},"attestation_state":"computed","paper":{"title":"Black Hole Mergers from Globular Clusters Observable by LISA and LIGO: Results from post-Newtonian Binary-Single Scatterings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Abbas Askar, Daniel J. D'Orazio, Johan Samsing, Mirek Giersz","submitted_at":"2018-02-23T17:36:37Z","abstract_excerpt":"We study the gravitational wave (GW) frequency and chirp mass distribution of binary black hole (BBH) mergers assembled through three-body interactions in globular clusters (GCs), when GW emission at the 2.5 post-Newtonian (PN) level is included in the $N$-body equation-of-motion (EOM). From performing $\\sim 2.5\\times10^{6}$ PN binary-single interactions based on GC data from the `MOCCA-Survey Database I' project, and by the use of analytical methods, we find that $5-10\\%$ of all the three-body assembled GC BBH mergers have a GW frequency at formation that is $\\gtrsim 10^{-1}$ Hz, implying the"},"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":"1802.08654","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-02-23T17:36:37Z","cross_cats_sorted":[],"title_canon_sha256":"2ee10c5e8bee69c0347d6d2105b02a9c305ccd4767fb48b5b8ddb6d0473001bf","abstract_canon_sha256":"e4ceb6476cd881e279866d27596ec01063a05e3fb777afc01a624b1a27e06d3c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:40.907305Z","signature_b64":"B6A4mRJpEgMlTE7ynEUg/WmvDZEihjNxDwZ4k8DyyvoNoE8HsNXSmFOti70M/NXmWlzYorLqOScqvP6M86MtDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"30110575a4fae975c10a3210d27a15f2d230d9188fb5aae59535bb4a0bbc24f5","last_reissued_at":"2026-05-18T00:22:40.906658Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:40.906658Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black Hole Mergers from Globular Clusters Observable by LISA and LIGO: Results from post-Newtonian Binary-Single Scatterings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Abbas Askar, Daniel J. D'Orazio, Johan Samsing, Mirek Giersz","submitted_at":"2018-02-23T17:36:37Z","abstract_excerpt":"We study the gravitational wave (GW) frequency and chirp mass distribution of binary black hole (BBH) mergers assembled through three-body interactions in globular clusters (GCs), when GW emission at the 2.5 post-Newtonian (PN) level is included in the $N$-body equation-of-motion (EOM). From performing $\\sim 2.5\\times10^{6}$ PN binary-single interactions based on GC data from the `MOCCA-Survey Database I' project, and by the use of analytical methods, we find that $5-10\\%$ of all the three-body assembled GC BBH mergers have a GW frequency at formation that is $\\gtrsim 10^{-1}$ Hz, implying the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.08654","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":"1802.08654","created_at":"2026-05-18T00:22:40.906754+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.08654v1","created_at":"2026-05-18T00:22:40.906754+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.08654","created_at":"2026-05-18T00:22:40.906754+00:00"},{"alias_kind":"pith_short_12","alias_value":"GAIQK5NE7LUX","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_16","alias_value":"GAIQK5NE7LUXLQIK","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_8","alias_value":"GAIQK5NE","created_at":"2026-05-18T12:32:25.280505+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L","json":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L.json","graph_json":"https://pith.science/api/pith-number/GAIQK5NE7LUXLQIKGIINE6QV6L/graph.json","events_json":"https://pith.science/api/pith-number/GAIQK5NE7LUXLQIKGIINE6QV6L/events.json","paper":"https://pith.science/paper/GAIQK5NE"},"agent_actions":{"view_html":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L","download_json":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L.json","view_paper":"https://pith.science/paper/GAIQK5NE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.08654&json=true","fetch_graph":"https://pith.science/api/pith-number/GAIQK5NE7LUXLQIKGIINE6QV6L/graph.json","fetch_events":"https://pith.science/api/pith-number/GAIQK5NE7LUXLQIKGIINE6QV6L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L/action/storage_attestation","attest_author":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L/action/author_attestation","sign_citation":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L/action/citation_signature","submit_replication":"https://pith.science/pith/GAIQK5NE7LUXLQIKGIINE6QV6L/action/replication_record"}},"created_at":"2026-05-18T00:22:40.906754+00:00","updated_at":"2026-05-18T00:22:40.906754+00:00"}