{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:KBPSRGSVFHBDGM4LUKXLNHARR3","short_pith_number":"pith:KBPSRGSV","schema_version":"1.0","canonical_sha256":"505f289a5529c233338ba2aeb69c118ec71ef4588a555dc234a6a97782fcf757","source":{"kind":"arxiv","id":"2212.08441","version":2},"attestation_state":"computed","paper":{"title":"Shift-symmetric Horndeski gravity in the asymptotic-safety paradigm","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Astrid Eichhorn, Fabian Wagner, Rafael R. Lino dos Santos","submitted_at":"2022-12-16T12:40:54Z","abstract_excerpt":"Horndeski gravity is a popular contender for a phenomenological model of dynamical dark energy, and as such subject to observational constraints. In this work, we ask whether Horndeski gravity can be more than a phenomenological model and instead become a fundamental theory, which extends towards high energy scales and includes quantum effects. We find that within the asymptotic-safety paradigm, an ultraviolet completion of a simple class of models of Horndeski gravity is achievable, but places strong constraints on the couplings of the theory. These constraints are not compatible with dynamic"},"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":"2212.08441","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2022-12-16T12:40:54Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"588f5eb379b2e22fc0fd626af8938ee6e61eb4ee9694bccb3dd2ed2ac59f10e3","abstract_canon_sha256":"aaa5f4c57f2e9a40561d293dadbdbed210c4083e6da2fa020513e9087dc53c1b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:53:09.248041Z","signature_b64":"2E5fElGmbk9Cw23OSIIOsXJPH7rBtGdFR8Ntbx16/C1Rns6hF/aAj/K9l6kvZVsSPfqOpu22Hsj7U5ucBlxRDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"505f289a5529c233338ba2aeb69c118ec71ef4588a555dc234a6a97782fcf757","last_reissued_at":"2026-07-05T05:53:09.247540Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:53:09.247540Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Shift-symmetric Horndeski gravity in the asymptotic-safety paradigm","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Astrid Eichhorn, Fabian Wagner, Rafael R. Lino dos Santos","submitted_at":"2022-12-16T12:40:54Z","abstract_excerpt":"Horndeski gravity is a popular contender for a phenomenological model of dynamical dark energy, and as such subject to observational constraints. In this work, we ask whether Horndeski gravity can be more than a phenomenological model and instead become a fundamental theory, which extends towards high energy scales and includes quantum effects. We find that within the asymptotic-safety paradigm, an ultraviolet completion of a simple class of models of Horndeski gravity is achievable, but places strong constraints on the couplings of the theory. These constraints are not compatible with dynamic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2212.08441","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2212.08441/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2212.08441","created_at":"2026-07-05T05:53:09.247599+00:00"},{"alias_kind":"arxiv_version","alias_value":"2212.08441v2","created_at":"2026-07-05T05:53:09.247599+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2212.08441","created_at":"2026-07-05T05:53:09.247599+00:00"},{"alias_kind":"pith_short_12","alias_value":"KBPSRGSVFHBD","created_at":"2026-07-05T05:53:09.247599+00:00"},{"alias_kind":"pith_short_16","alias_value":"KBPSRGSVFHBDGM4L","created_at":"2026-07-05T05:53:09.247599+00:00"},{"alias_kind":"pith_short_8","alias_value":"KBPSRGSV","created_at":"2026-07-05T05:53:09.247599+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2601.17115","citing_title":"Effective geometrodynamics for renormalization-group improved black-hole spacetimes in spherical symmetry","ref_index":90,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3","json":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3.json","graph_json":"https://pith.science/api/pith-number/KBPSRGSVFHBDGM4LUKXLNHARR3/graph.json","events_json":"https://pith.science/api/pith-number/KBPSRGSVFHBDGM4LUKXLNHARR3/events.json","paper":"https://pith.science/paper/KBPSRGSV"},"agent_actions":{"view_html":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3","download_json":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3.json","view_paper":"https://pith.science/paper/KBPSRGSV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2212.08441&json=true","fetch_graph":"https://pith.science/api/pith-number/KBPSRGSVFHBDGM4LUKXLNHARR3/graph.json","fetch_events":"https://pith.science/api/pith-number/KBPSRGSVFHBDGM4LUKXLNHARR3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3/action/storage_attestation","attest_author":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3/action/author_attestation","sign_citation":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3/action/citation_signature","submit_replication":"https://pith.science/pith/KBPSRGSVFHBDGM4LUKXLNHARR3/action/replication_record"}},"created_at":"2026-07-05T05:53:09.247599+00:00","updated_at":"2026-07-05T05:53:09.247599+00:00"}