{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:IWGYCYCRJR3VG53Q7HFGIAJU6M","short_pith_number":"pith:IWGYCYCR","schema_version":"1.0","canonical_sha256":"458d8160514c77537770f9ca640134f33e15419c21b2480a54fac22b93b46906","source":{"kind":"arxiv","id":"1805.10385","version":2},"attestation_state":"computed","paper":{"title":"Self-force and radiation reaction in general relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Adam Pound, Leor Barack","submitted_at":"2018-05-25T22:48:11Z","abstract_excerpt":"[Abridged] This review surveys the theory of gravitational self-force in curved spacetime and its application to the gravitational two-body problem in the extreme-mass-ratio regime. We first lay the relevant formal foundation, describing the rigorous derivation of the equation of self-forced motion using matched asymptotic expansions and other ideas. We then review the progress that has been achieved in numerically calculating the self-force and its physical effects in the astrophysical scenario of a compact object inspiralling into a (rotating) massive black hole. We highlight the way in whic"},"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":"1805.10385","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-05-25T22:48:11Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"2de0d3421ee15efd06de6bfc37dadb5c293610ec49548253b49f1d06de15374a","abstract_canon_sha256":"219fafdc84b3f91504e8b7c2772bc1d76df06e13aed63f24537d3c4bef8c0a9e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:57:41.281141Z","signature_b64":"FlCMdHugehb7aOG2RmjLmc9SBBvlrrpos55fXl2rh5Iid8TPqh1v5fW8W0IO079MOvcGH/cV0MrEV4gBIRLPAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"458d8160514c77537770f9ca640134f33e15419c21b2480a54fac22b93b46906","last_reissued_at":"2026-05-17T23:57:41.280487Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:57:41.280487Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Self-force and radiation reaction in general relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Adam Pound, Leor Barack","submitted_at":"2018-05-25T22:48:11Z","abstract_excerpt":"[Abridged] This review surveys the theory of gravitational self-force in curved spacetime and its application to the gravitational two-body problem in the extreme-mass-ratio regime. We first lay the relevant formal foundation, describing the rigorous derivation of the equation of self-forced motion using matched asymptotic expansions and other ideas. We then review the progress that has been achieved in numerically calculating the self-force and its physical effects in the astrophysical scenario of a compact object inspiralling into a (rotating) massive black hole. We highlight the way in whic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.10385","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":"1805.10385","created_at":"2026-05-17T23:57:41.280592+00:00"},{"alias_kind":"arxiv_version","alias_value":"1805.10385v2","created_at":"2026-05-17T23:57:41.280592+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1805.10385","created_at":"2026-05-17T23:57:41.280592+00:00"},{"alias_kind":"pith_short_12","alias_value":"IWGYCYCRJR3V","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_16","alias_value":"IWGYCYCRJR3VG53Q","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_8","alias_value":"IWGYCYCR","created_at":"2026-05-18T12:32:31.084164+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":22,"internal_anchor_count":9,"sample":[{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":98,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13847","citing_title":"Analytical Fluxes from Generic Schwarzschild Geodesics","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2411.11846","citing_title":"Emergence of Calabi-Yau manifolds in high-precision black hole scattering","ref_index":27,"is_internal_anchor":true},{"citing_arxiv_id":"2605.18544","citing_title":"The Classical Gravitational Impulse at High Energies","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2507.04471","citing_title":"A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2510.11793","citing_title":"Black hole mergers beyond general relativity: a self-force approach","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2510.16113","citing_title":"Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary","ref_index":120,"is_internal_anchor":true},{"citing_arxiv_id":"2601.11186","citing_title":"Analytic self-force effects on radial infalling particles in the Schwarzschild spacetime: the radiated energy","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13847","citing_title":"Analytical Fluxes from Generic Schwarzschild Geodesics","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2605.09250","citing_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11499","citing_title":"Black Hole Ringdown Seen in Photon Polarization Swings","ref_index":40,"is_internal_anchor":false},{"citing_arxiv_id":"2604.28140","citing_title":"Beyond the Separatrix: Analytic Continuation of Darwin Variables for Plunging Geodesics in Schwarzschild Spacetime","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2605.09250","citing_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2112.06861","citing_title":"Tests of General Relativity with GWTC-3","ref_index":40,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08798","citing_title":"Gravitational waveform from radial infall at the third-and-half Post-Newtonian order","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05362","citing_title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22009","citing_title":"Black Hole Response Theory and its Exact Shockwave Limit","ref_index":98,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05362","citing_title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06009","citing_title":"Are Black Holes Fuzzballs? Probing Horizon-Scale Structure with LISA","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06053","citing_title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","ref_index":102,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14112","citing_title":"Gravitational Sommerfeld Effects: Formalism, Renormalization, and Perturbation to $O(G^{10})$","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2503.12263","citing_title":"The Science of the Einstein Telescope","ref_index":216,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M","json":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M.json","graph_json":"https://pith.science/api/pith-number/IWGYCYCRJR3VG53Q7HFGIAJU6M/graph.json","events_json":"https://pith.science/api/pith-number/IWGYCYCRJR3VG53Q7HFGIAJU6M/events.json","paper":"https://pith.science/paper/IWGYCYCR"},"agent_actions":{"view_html":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M","download_json":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M.json","view_paper":"https://pith.science/paper/IWGYCYCR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1805.10385&json=true","fetch_graph":"https://pith.science/api/pith-number/IWGYCYCRJR3VG53Q7HFGIAJU6M/graph.json","fetch_events":"https://pith.science/api/pith-number/IWGYCYCRJR3VG53Q7HFGIAJU6M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M/action/storage_attestation","attest_author":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M/action/author_attestation","sign_citation":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M/action/citation_signature","submit_replication":"https://pith.science/pith/IWGYCYCRJR3VG53Q7HFGIAJU6M/action/replication_record"}},"created_at":"2026-05-17T23:57:41.280592+00:00","updated_at":"2026-05-17T23:57:41.280592+00:00"}