{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:ZDATVGJNSWEZONP4OWXWKC5ZLF","short_pith_number":"pith:ZDATVGJN","schema_version":"1.0","canonical_sha256":"c8c13a992d95899735fc75af650bb9596abe35706c7e2a4767c6a1261101d281","source":{"kind":"arxiv","id":"1501.04956","version":3},"attestation_state":"computed","paper":{"title":"Spinning gravitating objects in the effective field theory in the post-Newtonian scheme","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Jan Steinhoff, Michele Levi","submitted_at":"2015-01-20T20:54:00Z","abstract_excerpt":"We introduce a formulation for spinning gravitating objects in the effective field theory in the post-Newtonian scheme in the context of the binary inspiral problem. We aim at an effective action, where all field modes below the orbital scale are integrated out. We spell out the relevant degrees of freedom, in particular the rotational ones, and the associated symmetries. Building on these symmetries, we introduce the minimal coupling part of the point particle action in terms of gauge rotational variables, and construct the spin-induced nonminimal couplings, where we obtain the leading order "},"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":"1501.04956","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-01-20T20:54:00Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"89be47370b466d60bc3b98ee4f158fad56646dca87134cb756432c4bb50011c7","abstract_canon_sha256":"d61e6b3471e36f8c3e992fc2b5513ee65f6c12cadfa1e8f6d7a7a3e6a6d8938e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:31:03.397472Z","signature_b64":"MKnOYJ8QuGnzte+wN/3h4FiylY/QrvubhOKNANWwBIDv7NA/zx//kC/sgNkP1i3qqqNd86lmfbl5T/44ZaRdCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c8c13a992d95899735fc75af650bb9596abe35706c7e2a4767c6a1261101d281","last_reissued_at":"2026-05-18T01:31:03.396972Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:31:03.396972Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spinning gravitating objects in the effective field theory in the post-Newtonian scheme","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Jan Steinhoff, Michele Levi","submitted_at":"2015-01-20T20:54:00Z","abstract_excerpt":"We introduce a formulation for spinning gravitating objects in the effective field theory in the post-Newtonian scheme in the context of the binary inspiral problem. We aim at an effective action, where all field modes below the orbital scale are integrated out. We spell out the relevant degrees of freedom, in particular the rotational ones, and the associated symmetries. Building on these symmetries, we introduce the minimal coupling part of the point particle action in terms of gauge rotational variables, and construct the spin-induced nonminimal couplings, where we obtain the leading order "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.04956","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":"1501.04956","created_at":"2026-05-18T01:31:03.397061+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.04956v3","created_at":"2026-05-18T01:31:03.397061+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.04956","created_at":"2026-05-18T01:31:03.397061+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZDATVGJNSWEZ","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZDATVGJNSWEZONP4","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZDATVGJN","created_at":"2026-05-18T12:29:52.810259+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2504.07862","citing_title":"Resummation of Universal Tails in Gravitational Waveforms","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2602.18790","citing_title":"Generalized Carter & R\\\"udiger Constants of $\\sqrt{\\text{Kerr}}$","ref_index":45,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15160","citing_title":"N-body next-to-leading order gravitational spin-orbit interaction via effective field theory","ref_index":64,"is_internal_anchor":true},{"citing_arxiv_id":"2603.27353","citing_title":"Universality in Relativistic Spinning Particle Models","ref_index":96,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12214","citing_title":"A Runway to Dissipation of Angular Momentum via Worldline Quantum Field Theory","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14134","citing_title":"All-order structure of static gravitational interactions and the seventh post-Newtonian potential","ref_index":105,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09828","citing_title":"Testing the Kerr hypothesis beyond the quadrupole with GW241011","ref_index":59,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08653","citing_title":"Love numbers of black holes and compact objects","ref_index":143,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF","json":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF.json","graph_json":"https://pith.science/api/pith-number/ZDATVGJNSWEZONP4OWXWKC5ZLF/graph.json","events_json":"https://pith.science/api/pith-number/ZDATVGJNSWEZONP4OWXWKC5ZLF/events.json","paper":"https://pith.science/paper/ZDATVGJN"},"agent_actions":{"view_html":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF","download_json":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF.json","view_paper":"https://pith.science/paper/ZDATVGJN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.04956&json=true","fetch_graph":"https://pith.science/api/pith-number/ZDATVGJNSWEZONP4OWXWKC5ZLF/graph.json","fetch_events":"https://pith.science/api/pith-number/ZDATVGJNSWEZONP4OWXWKC5ZLF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF/action/storage_attestation","attest_author":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF/action/author_attestation","sign_citation":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF/action/citation_signature","submit_replication":"https://pith.science/pith/ZDATVGJNSWEZONP4OWXWKC5ZLF/action/replication_record"}},"created_at":"2026-05-18T01:31:03.397061+00:00","updated_at":"2026-05-18T01:31:03.397061+00:00"}