{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:S3373E6KQ5ZQTFMCIDGXAEUCSC","short_pith_number":"pith:S3373E6K","schema_version":"1.0","canonical_sha256":"96f7fd93ca877309958240cd70128290b68f54a53bffcdfe284d148fb360ec8e","source":{"kind":"arxiv","id":"1607.06463","version":1},"attestation_state":"computed","paper":{"title":"Einsteinian cubic gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Pablo A. Cano, Pablo Bueno","submitted_at":"2016-07-21T20:00:07Z","abstract_excerpt":"We drastically simplify the problem of linearizing a general higher-order theory of gravity. We reduce it to the evaluation of its Lagrangian on a particular Riemann tensor depending on two parameters, and the computation of two derivatives with respect to one of those parameters. We use our method to construct a D-dimensional cubic theory of gravity which satisfies the following properties: 1) it shares the spectrum of Einstein gravity, i.e., it only propagates a transverse and massless graviton on a maximally symmetric background; 2) the relative coefficients of the different curvature invar"},"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":"1607.06463","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2016-07-21T20:00:07Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"dbe62fb9b542ce7ba845c2767a78d8478ed28a532e57df62492724230ce0bbc0","abstract_canon_sha256":"154a25eaff875b4bf2267c1739114cb10067aa637b21725cbe3bc5bea553d43e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:59:57.771875Z","signature_b64":"i2/g8XYmxsmPZJMC9jJ2+8LEztPW6wWp1h6dfUP/e6d29UuEFrgw5OwJUKJkEWBaUFfFHx49G5F3pGS39ySdAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96f7fd93ca877309958240cd70128290b68f54a53bffcdfe284d148fb360ec8e","last_reissued_at":"2026-05-18T00:59:57.771192Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:59:57.771192Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Einsteinian cubic gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Pablo A. Cano, Pablo Bueno","submitted_at":"2016-07-21T20:00:07Z","abstract_excerpt":"We drastically simplify the problem of linearizing a general higher-order theory of gravity. We reduce it to the evaluation of its Lagrangian on a particular Riemann tensor depending on two parameters, and the computation of two derivatives with respect to one of those parameters. We use our method to construct a D-dimensional cubic theory of gravity which satisfies the following properties: 1) it shares the spectrum of Einstein gravity, i.e., it only propagates a transverse and massless graviton on a maximally symmetric background; 2) the relative coefficients of the different curvature invar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.06463","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":"1607.06463","created_at":"2026-05-18T00:59:57.771300+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.06463v1","created_at":"2026-05-18T00:59:57.771300+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.06463","created_at":"2026-05-18T00:59:57.771300+00:00"},{"alias_kind":"pith_short_12","alias_value":"S3373E6KQ5ZQ","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_16","alias_value":"S3373E6KQ5ZQTFMC","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_8","alias_value":"S3373E6K","created_at":"2026-05-18T12:30:41.710351+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2607.07831","citing_title":"Charging up regular black holes","ref_index":22,"is_internal_anchor":true},{"citing_arxiv_id":"2606.17784","citing_title":"Quasi-topological gravity for 4-dimensional Taub-NUT, near-horizon extreme Kerr, and swirling symmetries","ref_index":26,"is_internal_anchor":true},{"citing_arxiv_id":"2605.26173","citing_title":"Effect of $R^2$ on the stability of de Sitter solution of the generalized Einsteinian cubic gravity","ref_index":50,"is_internal_anchor":true},{"citing_arxiv_id":"2311.12104","citing_title":"Cosmological higher-curvature gravities","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2506.14875","citing_title":"Regular Vaidya solutions of effective gravitational theories","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2604.04601","citing_title":"Cosmic Inflation From Regular Black Holes","ref_index":20,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC","json":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC.json","graph_json":"https://pith.science/api/pith-number/S3373E6KQ5ZQTFMCIDGXAEUCSC/graph.json","events_json":"https://pith.science/api/pith-number/S3373E6KQ5ZQTFMCIDGXAEUCSC/events.json","paper":"https://pith.science/paper/S3373E6K"},"agent_actions":{"view_html":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC","download_json":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC.json","view_paper":"https://pith.science/paper/S3373E6K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.06463&json=true","fetch_graph":"https://pith.science/api/pith-number/S3373E6KQ5ZQTFMCIDGXAEUCSC/graph.json","fetch_events":"https://pith.science/api/pith-number/S3373E6KQ5ZQTFMCIDGXAEUCSC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC/action/storage_attestation","attest_author":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC/action/author_attestation","sign_citation":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC/action/citation_signature","submit_replication":"https://pith.science/pith/S3373E6KQ5ZQTFMCIDGXAEUCSC/action/replication_record"}},"created_at":"2026-05-18T00:59:57.771300+00:00","updated_at":"2026-05-18T00:59:57.771300+00:00"}