{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:QPY4IMIOSXKZEBBS56SGLOYZNA","short_pith_number":"pith:QPY4IMIO","schema_version":"1.0","canonical_sha256":"83f1c4310e95d5920432efa465bb196831d8d8baf8bca1ff6bc919dfa54e2961","source":{"kind":"arxiv","id":"1004.0284","version":3},"attestation_state":"computed","paper":{"title":"Constraining the mass of the graviton using coalescing black-hole binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Drew Keppel, P. Ajith","submitted_at":"2010-04-02T04:27:29Z","abstract_excerpt":"We study how well the mass of the graviton can be constrained from gravitational-wave (GW) observations of coalescing binary black holes. Whereas the previous investigations employed post-Newtonian (PN) templates describing only the inspiral part of the signal, the recent progress in analytical and numerical relativity has provided analytical waveform templates coherently describing the inspiral-merger-ringdown (IMR) signals. We show that a search for binary black holes employing IMR templates will be able to constrain the mass of the graviton much more accurately (about an order of magnitude)"},"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":"1004.0284","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-04-02T04:27:29Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"60bc4e5ff9a946a3db532d68723118f3055fd9ee8db101fbe619f30ab49761d3","abstract_canon_sha256":"034a311ac4949679a3ec7612f0197b61b06e72c85c221057af831a6b3150d1dd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:32:43.561585Z","signature_b64":"pSht12aazq0Ma2Fci4v5n6xhev0luvV0u/Qy09C3M/LiskLccbHDL2fHYxEM/p6yARWC2uUMKZsjedi70s0/AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"83f1c4310e95d5920432efa465bb196831d8d8baf8bca1ff6bc919dfa54e2961","last_reissued_at":"2026-05-18T04:32:43.560913Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:32:43.560913Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining the mass of the graviton using coalescing black-hole binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Drew Keppel, P. Ajith","submitted_at":"2010-04-02T04:27:29Z","abstract_excerpt":"We study how well the mass of the graviton can be constrained from gravitational-wave (GW) observations of coalescing binary black holes. Whereas the previous investigations employed post-Newtonian (PN) templates describing only the inspiral part of the signal, the recent progress in analytical and numerical relativity has provided analytical waveform templates coherently describing the inspiral-merger-ringdown (IMR) signals. We show that a search for binary black holes employing IMR templates will be able to constrain the mass of the graviton much more accurately (about an order of magnitude)"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.0284","kind":"arxiv","version":3},"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":"1004.0284","created_at":"2026-05-18T04:32:43.561016+00:00"},{"alias_kind":"arxiv_version","alias_value":"1004.0284v3","created_at":"2026-05-18T04:32:43.561016+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.0284","created_at":"2026-05-18T04:32:43.561016+00:00"},{"alias_kind":"pith_short_12","alias_value":"QPY4IMIOSXKZ","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"QPY4IMIOSXKZEBBS","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"QPY4IMIO","created_at":"2026-05-18T12:26:12.377268+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/QPY4IMIOSXKZEBBS56SGLOYZNA","json":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA.json","graph_json":"https://pith.science/api/pith-number/QPY4IMIOSXKZEBBS56SGLOYZNA/graph.json","events_json":"https://pith.science/api/pith-number/QPY4IMIOSXKZEBBS56SGLOYZNA/events.json","paper":"https://pith.science/paper/QPY4IMIO"},"agent_actions":{"view_html":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA","download_json":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA.json","view_paper":"https://pith.science/paper/QPY4IMIO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1004.0284&json=true","fetch_graph":"https://pith.science/api/pith-number/QPY4IMIOSXKZEBBS56SGLOYZNA/graph.json","fetch_events":"https://pith.science/api/pith-number/QPY4IMIOSXKZEBBS56SGLOYZNA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA/action/storage_attestation","attest_author":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA/action/author_attestation","sign_citation":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA/action/citation_signature","submit_replication":"https://pith.science/pith/QPY4IMIOSXKZEBBS56SGLOYZNA/action/replication_record"}},"created_at":"2026-05-18T04:32:43.561016+00:00","updated_at":"2026-05-18T04:32:43.561016+00:00"}