{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:PPRGSXWOD4PYUFDWF277HVFQAQ","short_pith_number":"pith:PPRGSXWO","schema_version":"1.0","canonical_sha256":"7be2695ece1f1f8a14762ebff3d4b0041a7c8549deeee6ba582ba2857e0f275b","source":{"kind":"arxiv","id":"1108.4367","version":1},"attestation_state":"computed","paper":{"title":"Generalizing the ADM Computation to Quantum Field Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"N. C. Tsamis (University of Crete), P. J. Mora (University of Florida), R. P. Woodard (University of Florida)","submitted_at":"2011-08-22T16:14:54Z","abstract_excerpt":"The absence of recognizable, low energy quantum gravitational effects requires that some asymptotic series expansion be wonderfully accurate, but the correct expansion might involve logarithms or fractional powers of Newton's constant. That would explain why conventional perturbation theory shows uncontrollable ultraviolet divergences. We explore this possibility in the context of the mass of a charged, gravitating scalar. The classical limit of this system was solved exactly in 1960 by Arnowitt, Deser and Misner, and their solution does exhibit nonanalytic dependence on Newton's constant. We "},"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":"1108.4367","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2011-08-22T16:14:54Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"4595dbec4564be2fbdef72501957f82865410c232971110a1c980a977ce8cc6e","abstract_canon_sha256":"20a5f6e80dee382c30e7ac941cfc62fa4675ad7d7febde18c9cbd7596da03587"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:49.763449Z","signature_b64":"mX6EGwSbp2xJE5RfGPUCBFbzMg+t+27qCeDAMdPuLzGUawQg4sRWXtt6EOks4qZWLpdaedcJXDoHKxq0qI0fBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7be2695ece1f1f8a14762ebff3d4b0041a7c8549deeee6ba582ba2857e0f275b","last_reissued_at":"2026-05-18T02:00:49.762841Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:49.762841Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Generalizing the ADM Computation to Quantum Field Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"N. C. Tsamis (University of Crete), P. J. Mora (University of Florida), R. P. Woodard (University of Florida)","submitted_at":"2011-08-22T16:14:54Z","abstract_excerpt":"The absence of recognizable, low energy quantum gravitational effects requires that some asymptotic series expansion be wonderfully accurate, but the correct expansion might involve logarithms or fractional powers of Newton's constant. That would explain why conventional perturbation theory shows uncontrollable ultraviolet divergences. We explore this possibility in the context of the mass of a charged, gravitating scalar. The classical limit of this system was solved exactly in 1960 by Arnowitt, Deser and Misner, and their solution does exhibit nonanalytic dependence on Newton's constant. We "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.4367","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":"1108.4367","created_at":"2026-05-18T02:00:49.762941+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.4367v1","created_at":"2026-05-18T02:00:49.762941+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.4367","created_at":"2026-05-18T02:00:49.762941+00:00"},{"alias_kind":"pith_short_12","alias_value":"PPRGSXWOD4PY","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_16","alias_value":"PPRGSXWOD4PYUFDW","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_8","alias_value":"PPRGSXWO","created_at":"2026-05-18T12:26:39.201973+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ","json":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ.json","graph_json":"https://pith.science/api/pith-number/PPRGSXWOD4PYUFDWF277HVFQAQ/graph.json","events_json":"https://pith.science/api/pith-number/PPRGSXWOD4PYUFDWF277HVFQAQ/events.json","paper":"https://pith.science/paper/PPRGSXWO"},"agent_actions":{"view_html":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ","download_json":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ.json","view_paper":"https://pith.science/paper/PPRGSXWO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.4367&json=true","fetch_graph":"https://pith.science/api/pith-number/PPRGSXWOD4PYUFDWF277HVFQAQ/graph.json","fetch_events":"https://pith.science/api/pith-number/PPRGSXWOD4PYUFDWF277HVFQAQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ/action/storage_attestation","attest_author":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ/action/author_attestation","sign_citation":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ/action/citation_signature","submit_replication":"https://pith.science/pith/PPRGSXWOD4PYUFDWF277HVFQAQ/action/replication_record"}},"created_at":"2026-05-18T02:00:49.762941+00:00","updated_at":"2026-05-18T02:00:49.762941+00:00"}