{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:B7BHTPQWTZ5B2GXMA5J7AAIH4M","short_pith_number":"pith:B7BHTPQW","schema_version":"1.0","canonical_sha256":"0fc279be169e7a1d1aec0753f00107e32a654d2bf38008af2f1e1b3f0a48f3bf","source":{"kind":"arxiv","id":"1301.4191","version":2},"attestation_state":"computed","paper":{"title":"A bootstrap strategy for asymptotic safety","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"C. Rahmede, D. F. Litim, K. Falls, K. Nikolakopoulos","submitted_at":"2013-01-17T19:13:49Z","abstract_excerpt":"A search strategy for asymptotic safety is put forward and tested for a simplified version of gravity in four dimensions using the renormalization group. Taking the action to be a high-order polynomial of the Ricci scalar, a self-consistent ultraviolet fixed point is found where curvature invariants become increasingly irrelevant with increasing mass dimension. Intriguingly, universal scaling exponents take near-Gaussian values despite the presence of residual interactions. Asymptotic safety of metric gravity would seem in reach if this pattern carries over to the full theory."},"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":"1301.4191","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-01-17T19:13:49Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"aa392fbad1042eddd05850378eba8d8ef5d6a249e99380dcc826f0418f967508","abstract_canon_sha256":"db8f53f9e6ef6da2169ffdf1f4c161df0df2258b1b7a1d65c1c2c6f251b2f5c9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:17:33.693630Z","signature_b64":"nxoNeFxGYqR3mX9q1v/Pn2fE2twDfwBDkcHEaGh2CUBv6ZqT/auX0K7vX5pVDLzdeTbdFcqbEpozV07VoO3lCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0fc279be169e7a1d1aec0753f00107e32a654d2bf38008af2f1e1b3f0a48f3bf","last_reissued_at":"2026-05-18T01:17:33.692909Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:17:33.692909Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A bootstrap strategy for asymptotic safety","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"C. Rahmede, D. F. Litim, K. Falls, K. Nikolakopoulos","submitted_at":"2013-01-17T19:13:49Z","abstract_excerpt":"A search strategy for asymptotic safety is put forward and tested for a simplified version of gravity in four dimensions using the renormalization group. Taking the action to be a high-order polynomial of the Ricci scalar, a self-consistent ultraviolet fixed point is found where curvature invariants become increasingly irrelevant with increasing mass dimension. Intriguingly, universal scaling exponents take near-Gaussian values despite the presence of residual interactions. Asymptotic safety of metric gravity would seem in reach if this pattern carries over to the full theory."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.4191","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":"1301.4191","created_at":"2026-05-18T01:17:33.693022+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.4191v2","created_at":"2026-05-18T01:17:33.693022+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.4191","created_at":"2026-05-18T01:17:33.693022+00:00"},{"alias_kind":"pith_short_12","alias_value":"B7BHTPQWTZ5B","created_at":"2026-05-18T12:27:38.830355+00:00"},{"alias_kind":"pith_short_16","alias_value":"B7BHTPQWTZ5B2GXM","created_at":"2026-05-18T12:27:38.830355+00:00"},{"alias_kind":"pith_short_8","alias_value":"B7BHTPQW","created_at":"2026-05-18T12:27:38.830355+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2508.00807","citing_title":"Proper-time functional renormalization in $O(N)$ scalar models coupled to gravity","ref_index":52,"is_internal_anchor":true},{"citing_arxiv_id":"2510.23808","citing_title":"Towards theory constraints on ultralight dark matter from quantum gravity","ref_index":90,"is_internal_anchor":true},{"citing_arxiv_id":"2604.03033","citing_title":"Quantum gravity contributions to the gauge and Yukawa couplings in proper time flow","ref_index":14,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M","json":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M.json","graph_json":"https://pith.science/api/pith-number/B7BHTPQWTZ5B2GXMA5J7AAIH4M/graph.json","events_json":"https://pith.science/api/pith-number/B7BHTPQWTZ5B2GXMA5J7AAIH4M/events.json","paper":"https://pith.science/paper/B7BHTPQW"},"agent_actions":{"view_html":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M","download_json":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M.json","view_paper":"https://pith.science/paper/B7BHTPQW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.4191&json=true","fetch_graph":"https://pith.science/api/pith-number/B7BHTPQWTZ5B2GXMA5J7AAIH4M/graph.json","fetch_events":"https://pith.science/api/pith-number/B7BHTPQWTZ5B2GXMA5J7AAIH4M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M/action/storage_attestation","attest_author":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M/action/author_attestation","sign_citation":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M/action/citation_signature","submit_replication":"https://pith.science/pith/B7BHTPQWTZ5B2GXMA5J7AAIH4M/action/replication_record"}},"created_at":"2026-05-18T01:17:33.693022+00:00","updated_at":"2026-05-18T01:17:33.693022+00:00"}