{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:T3PAY6BIDRXN7FEFILW4MZFG33","short_pith_number":"pith:T3PAY6BI","schema_version":"1.0","canonical_sha256":"9ede0c78281c6edf948542edc664a6deca2254b8fee77e351088439f6ca2b05d","source":{"kind":"arxiv","id":"1508.03044","version":4},"attestation_state":"computed","paper":{"title":"Slowly rotating black hole solutions in Horndeski gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Emanuele Berti, Hector O. Silva, Masato Minamitsuji","submitted_at":"2015-08-12T20:06:48Z","abstract_excerpt":"We study black hole solutions at first order in the Hartle-Thorne slow-rotation approximation in Horndeski gravity theories. We derive the equations of motion including also cases where the scalar depends linearly on time. In the Hartle-Thorne formalism, all first-order rotational corrections are described by a single frame-dragging function. We show that the frame-dragging function is exactly the same as in general relativity for all known black hole solutions in shift symmetric Horndeski theories, with the exception of theories with a linear coupling to the Gauss-Bonnet invariant. Our result"},"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":"1508.03044","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-08-12T20:06:48Z","cross_cats_sorted":["astro-ph.CO","hep-ph","hep-th"],"title_canon_sha256":"23e1ea2820814363aa516cfd8f6b803a540532811ae6ee7edb5ee53c1bb39d2e","abstract_canon_sha256":"9e7530af3a4076b0fd764a4e32fc4cabf681c53202e3c5d4f72b2e452880e741"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:25:31.430156Z","signature_b64":"gGdg1GMho2PsP5KWpIeQoDzjUwkeqrEqeg+hqdcJOoHOiG9+JXzZDLz0ZY1IrPLX9VDb9w82VpWESS/hqwABCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9ede0c78281c6edf948542edc664a6deca2254b8fee77e351088439f6ca2b05d","last_reissued_at":"2026-05-18T01:25:31.429624Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:25:31.429624Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Slowly rotating black hole solutions in Horndeski gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Emanuele Berti, Hector O. Silva, Masato Minamitsuji","submitted_at":"2015-08-12T20:06:48Z","abstract_excerpt":"We study black hole solutions at first order in the Hartle-Thorne slow-rotation approximation in Horndeski gravity theories. We derive the equations of motion including also cases where the scalar depends linearly on time. In the Hartle-Thorne formalism, all first-order rotational corrections are described by a single frame-dragging function. We show that the frame-dragging function is exactly the same as in general relativity for all known black hole solutions in shift symmetric Horndeski theories, with the exception of theories with a linear coupling to the Gauss-Bonnet invariant. Our result"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.03044","kind":"arxiv","version":4},"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":"1508.03044","created_at":"2026-05-18T01:25:31.429705+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.03044v4","created_at":"2026-05-18T01:25:31.429705+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.03044","created_at":"2026-05-18T01:25:31.429705+00:00"},{"alias_kind":"pith_short_12","alias_value":"T3PAY6BIDRXN","created_at":"2026-05-18T12:29:42.218222+00:00"},{"alias_kind":"pith_short_16","alias_value":"T3PAY6BIDRXN7FEF","created_at":"2026-05-18T12:29:42.218222+00:00"},{"alias_kind":"pith_short_8","alias_value":"T3PAY6BI","created_at":"2026-05-18T12:29:42.218222+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2602.16237","citing_title":"Rotating Black Holes with Primary Scalar Hair: Shadow Signatures in Beyond Horndeski Gravity","ref_index":63,"is_internal_anchor":true},{"citing_arxiv_id":"2603.22398","citing_title":"Stable black hole solutions with cosmological hair","ref_index":12,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33","json":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33.json","graph_json":"https://pith.science/api/pith-number/T3PAY6BIDRXN7FEFILW4MZFG33/graph.json","events_json":"https://pith.science/api/pith-number/T3PAY6BIDRXN7FEFILW4MZFG33/events.json","paper":"https://pith.science/paper/T3PAY6BI"},"agent_actions":{"view_html":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33","download_json":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33.json","view_paper":"https://pith.science/paper/T3PAY6BI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.03044&json=true","fetch_graph":"https://pith.science/api/pith-number/T3PAY6BIDRXN7FEFILW4MZFG33/graph.json","fetch_events":"https://pith.science/api/pith-number/T3PAY6BIDRXN7FEFILW4MZFG33/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33/action/storage_attestation","attest_author":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33/action/author_attestation","sign_citation":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33/action/citation_signature","submit_replication":"https://pith.science/pith/T3PAY6BIDRXN7FEFILW4MZFG33/action/replication_record"}},"created_at":"2026-05-18T01:25:31.429705+00:00","updated_at":"2026-05-18T01:25:31.429705+00:00"}