{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:LMLKKYPSV2YL6WPMR6CCKCD4WB","short_pith_number":"pith:LMLKKYPS","schema_version":"1.0","canonical_sha256":"5b16a561f2aeb0bf59ec8f8425087cb05e9b727a7fae5e8ea4de0935d589927f","source":{"kind":"arxiv","id":"hep-th/0601001","version":2},"attestation_state":"computed","paper":{"title":"The String Landscape, Black Holes and Gravity as the Weakest Force","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alberto Nicolis, Cumrun Vafa, Lubos Motl, Nima Arkani-Hamed","submitted_at":"2006-01-02T14:30:51Z","abstract_excerpt":"We conjecture a general upper bound on the strength of gravity relative to gauge forces in quantum gravity. This implies, in particular, that in a four-dimensional theory with gravity and a U(1) gauge field with gauge coupling g, there is a new ultraviolet scale Lambda=g M_{Pl}, invisible to the low-energy effective field theorist, which sets a cutoff on the validity of the effective theory. Moreover, there is some light charged particle with mass smaller than or equal to Lambda. The bound is motivated by arguments involving holography and absence of remnants, the (in) stability of black holes"},"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/0601001","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2006-01-02T14:30:51Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"ea5b597cc8cd962059419e83fd423121868fc5a09f03a4d68132a9a5cfd5b40e","abstract_canon_sha256":"fbf390f4c9b2d695faa6611c702d6fd4e1f8a6689635e7d0d46ef47e05ed8462"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:25:26.472286Z","signature_b64":"P4BaPfI5RL3N6AdgR30ZyqoRmlvFUtKC5DGPJvDS02huQmDznxSKvzYgc0Pr4QFiD4WW/SlQc4yFlnTegBdEBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b16a561f2aeb0bf59ec8f8425087cb05e9b727a7fae5e8ea4de0935d589927f","last_reissued_at":"2026-07-04T17:25:26.471794Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:25:26.471794Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The String Landscape, Black Holes and Gravity as the Weakest Force","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alberto Nicolis, Cumrun Vafa, Lubos Motl, Nima Arkani-Hamed","submitted_at":"2006-01-02T14:30:51Z","abstract_excerpt":"We conjecture a general upper bound on the strength of gravity relative to gauge forces in quantum gravity. This implies, in particular, that in a four-dimensional theory with gravity and a U(1) gauge field with gauge coupling g, there is a new ultraviolet scale Lambda=g M_{Pl}, invisible to the low-energy effective field theorist, which sets a cutoff on the validity of the effective theory. Moreover, there is some light charged particle with mass smaller than or equal to Lambda. The bound is motivated by arguments involving holography and absence of remnants, the (in) stability of black holes"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0601001","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/0601001/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/0601001","created_at":"2026-07-04T17:25:26.471872+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0601001v2","created_at":"2026-07-04T17:25:26.471872+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0601001","created_at":"2026-07-04T17:25:26.471872+00:00"},{"alias_kind":"pith_short_12","alias_value":"LMLKKYPSV2YL","created_at":"2026-07-04T17:25:26.471872+00:00"},{"alias_kind":"pith_short_16","alias_value":"LMLKKYPSV2YL6WPM","created_at":"2026-07-04T17:25:26.471872+00:00"},{"alias_kind":"pith_short_8","alias_value":"LMLKKYPS","created_at":"2026-07-04T17:25:26.471872+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":34,"internal_anchor_count":25,"sample":[{"citing_arxiv_id":"2606.26004","citing_title":"Non-invertible symmetries in the axiverse, and the imaginary wormholes","ref_index":90,"is_internal_anchor":true},{"citing_arxiv_id":"2606.21650","citing_title":"Quantum Gravity Cutoff from Axions: A Type IIB Landscape Study","ref_index":60,"is_internal_anchor":true},{"citing_arxiv_id":"2606.09996","citing_title":"On BPS Branes","ref_index":4,"is_internal_anchor":true},{"citing_arxiv_id":"2606.09982","citing_title":"Testing F-theory GUTs with the Axiverse","ref_index":126,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08244","citing_title":"Stochastic Survival near Swampland Boundaries","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04933","citing_title":"$\\text{AdS}_D\\times I$ solutions in axio-dilaton gravity","ref_index":2,"is_internal_anchor":true},{"citing_arxiv_id":"2606.05136","citing_title":"Thermal Positivity","ref_index":22,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04938","citing_title":"AdS$_9$ solutions in type II supergravities","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2606.03443","citing_title":"Constraints on long-range neutrino interactions from a variety of $U(1)^\\prime$ symmetries using atmospheric neutrinos at IceCube DeepCore","ref_index":65,"is_internal_anchor":true},{"citing_arxiv_id":"2606.01791","citing_title":"Probing the dark axion portal via $J/\\psi$ decays at BESIII and STCF","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2605.31331","citing_title":"Higher-Derivative Corrections to Reissner--Nordstr\\\"om Black Holes from Worldline QFT","ref_index":27,"is_internal_anchor":true},{"citing_arxiv_id":"2606.30853","citing_title":"Rethinking quantum information in gravity and fields","ref_index":284,"is_internal_anchor":true},{"citing_arxiv_id":"2605.10338","citing_title":"Fifth-Force Constraints from UV-Complete Scalar-Tensor Gravity","ref_index":21,"is_internal_anchor":true},{"citing_arxiv_id":"2605.10476","citing_title":"Breaking Free from the Swampland of Impossible Universes through the DESI Portal","ref_index":102,"is_internal_anchor":true},{"citing_arxiv_id":"2605.23047","citing_title":"On Thermodynamics of Charged Black Holes, Swampland, and Dark Matter","ref_index":30,"is_internal_anchor":true},{"citing_arxiv_id":"2605.22912","citing_title":"Sharpening the Supersymmetric Axion Weak Gravity Conjecture","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"2605.23047","citing_title":"On Thermodynamics of Charged Black Holes, Swampland, and Dark Matter","ref_index":27,"is_internal_anchor":true},{"citing_arxiv_id":"2605.23900","citing_title":"What to do with a Ricci-flat Calabi--Yau metric?","ref_index":94,"is_internal_anchor":true},{"citing_arxiv_id":"2404.07980","citing_title":"ISCOs and the weak gravity conjecture bound in higher derivative theories of gravity","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"2509.06630","citing_title":"Positivity bounds from thermal field theory entropy","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2511.09613","citing_title":"Bounds on Discrete Gauge Symmetries in Supergravity","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"2512.09884","citing_title":"A weakly non-abelian decay channel","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"2512.13780","citing_title":"Positivity with Long-Range Interactions","ref_index":88,"is_internal_anchor":true},{"citing_arxiv_id":"2601.11705","citing_title":"String Theory from Maximal Supersymmetry","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2103.01183","citing_title":"In the Realm of the Hubble tension $-$ a Review of Solutions","ref_index":229,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB","json":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB.json","graph_json":"https://pith.science/api/pith-number/LMLKKYPSV2YL6WPMR6CCKCD4WB/graph.json","events_json":"https://pith.science/api/pith-number/LMLKKYPSV2YL6WPMR6CCKCD4WB/events.json","paper":"https://pith.science/paper/LMLKKYPS"},"agent_actions":{"view_html":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB","download_json":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB.json","view_paper":"https://pith.science/paper/LMLKKYPS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0601001&json=true","fetch_graph":"https://pith.science/api/pith-number/LMLKKYPSV2YL6WPMR6CCKCD4WB/graph.json","fetch_events":"https://pith.science/api/pith-number/LMLKKYPSV2YL6WPMR6CCKCD4WB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB/action/storage_attestation","attest_author":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB/action/author_attestation","sign_citation":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB/action/citation_signature","submit_replication":"https://pith.science/pith/LMLKKYPSV2YL6WPMR6CCKCD4WB/action/replication_record"}},"created_at":"2026-07-04T17:25:26.471872+00:00","updated_at":"2026-07-04T17:25:26.471872+00:00"}