{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:DOHUGVTHIKHZJMJQ5GQ4XGAQC6","short_pith_number":"pith:DOHUGVTH","schema_version":"1.0","canonical_sha256":"1b8f435667428f94b130e9a1cb981017978d19deb6238538b0726a682f980286","source":{"kind":"arxiv","id":"hep-th/9803132","version":2},"attestation_state":"computed","paper":{"title":"Effective Field Theory, Black Holes, and the Cosmological Constant","license":"","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Andrew G. Cohen, Ann E. Nelson, David B. Kaplan","submitted_at":"1998-03-17T00:26:13Z","abstract_excerpt":"Bekenstein has proposed the bound S < pi M_P^2 L^2 on the total entropy S in a volume L^3. This non-extensive scaling suggests that quantum field theory breaks down in large volume. To reconcile this breakdown with the success of local quantum field theory in describing observed particle phenomenology, we propose a relationship between UV and IR cutoffs such that an effective field theory should be a good description of Nature. We discuss implications for the cosmological constant problem. We find a limitation on the accuracy which can be achieved by conventional effective field theory: for ex"},"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":"hep-th/9803132","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1998-03-17T00:26:13Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"e96a2cc3af0850f732224d91fddbca611a52eff2517b89b7cdc8932ed5d5a730","abstract_canon_sha256":"55200c0b793def741eb06b541457875e312c53c1a2791d16cbdfcdc6d50247f7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:45:47.480190Z","signature_b64":"rXnMCT25dMjqmBnH3QeXRmlHjS+WfedFXz6D8EqkgxU9FW9WTB7ZrPCMn8z7B4RI0/BnYu8mDjy7pcSdQdpXCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b8f435667428f94b130e9a1cb981017978d19deb6238538b0726a682f980286","last_reissued_at":"2026-07-04T15:45:47.479805Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:45:47.479805Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Effective Field Theory, Black Holes, and the Cosmological Constant","license":"","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Andrew G. Cohen, Ann E. Nelson, David B. Kaplan","submitted_at":"1998-03-17T00:26:13Z","abstract_excerpt":"Bekenstein has proposed the bound S < pi M_P^2 L^2 on the total entropy S in a volume L^3. This non-extensive scaling suggests that quantum field theory breaks down in large volume. To reconcile this breakdown with the success of local quantum field theory in describing observed particle phenomenology, we propose a relationship between UV and IR cutoffs such that an effective field theory should be a good description of Nature. We discuss implications for the cosmological constant problem. We find a limitation on the accuracy which can be achieved by conventional effective field theory: for ex"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9803132","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/hep-th/9803132/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":"hep-th/9803132","created_at":"2026-07-04T15:45:47.479867+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9803132v2","created_at":"2026-07-04T15:45:47.479867+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9803132","created_at":"2026-07-04T15:45:47.479867+00:00"},{"alias_kind":"pith_short_12","alias_value":"DOHUGVTHIKHZ","created_at":"2026-07-04T15:45:47.479867+00:00"},{"alias_kind":"pith_short_16","alias_value":"DOHUGVTHIKHZJMJQ","created_at":"2026-07-04T15:45:47.479867+00:00"},{"alias_kind":"pith_short_8","alias_value":"DOHUGVTH","created_at":"2026-07-04T15:45:47.479867+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":10,"sample":[{"citing_arxiv_id":"2606.17147","citing_title":"When Renormalisation Remembers: UV/IR Mixing as an Entanglement Bridge","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2606.06372","citing_title":"Quantum Geometry from Area Fluctuations","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2605.29374","citing_title":"Candidate collapse-noise correlators from Generalized Trace Dynamics: a Hubble-scale spectral line under structural assumptions","ref_index":32,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04318","citing_title":"The Awada-Gibbons-Shaw Algebra in de Sitter Space and SUSY Breaking","ref_index":21,"is_internal_anchor":true},{"citing_arxiv_id":"2601.17849","citing_title":"Geometric noise spectrum in interferometers","ref_index":4,"is_internal_anchor":true},{"citing_arxiv_id":"2507.01070","citing_title":"Barrow holographic dark energy interacting model in the presence of radiation and matter","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2507.22093","citing_title":"Field theory vacuum and entropic dark energy models","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2603.10787","citing_title":"Measuring neutrino mass in light of ACT DR6 and DESI DR2","ref_index":181,"is_internal_anchor":true},{"citing_arxiv_id":"2603.27824","citing_title":"Higher-spin composites and emergent AdS$_3$ geometry in the $(1+1)$-dimensional Gross-Neveu model","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13490","citing_title":"What does it mean to have a quantum gravitational theory of de Sitter Space?","ref_index":4,"is_internal_anchor":true},{"citing_arxiv_id":"2604.23492","citing_title":"The open-Universe signal: A model artifact rather than genuine curvature","ref_index":45,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18246","citing_title":"Holographic dark energy as a source for slowly rotating wormholes: Implications for null geodesics and shadows","ref_index":26,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6","json":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6.json","graph_json":"https://pith.science/api/pith-number/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/graph.json","events_json":"https://pith.science/api/pith-number/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/events.json","paper":"https://pith.science/paper/DOHUGVTH"},"agent_actions":{"view_html":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6","download_json":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6.json","view_paper":"https://pith.science/paper/DOHUGVTH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9803132&json=true","fetch_graph":"https://pith.science/api/pith-number/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/graph.json","fetch_events":"https://pith.science/api/pith-number/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/action/storage_attestation","attest_author":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/action/author_attestation","sign_citation":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/action/citation_signature","submit_replication":"https://pith.science/pith/DOHUGVTHIKHZJMJQ5GQ4XGAQC6/action/replication_record"}},"created_at":"2026-07-04T15:45:47.479867+00:00","updated_at":"2026-07-04T15:45:47.479867+00:00"}