{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:QXVWQ3SNXKZGQFUZQJGMHUESE7","short_pith_number":"pith:QXVWQ3SN","schema_version":"1.0","canonical_sha256":"85eb686e4dbab2681699824cc3d09227c4ee77f360aa6e9a514d0a617b63f812","source":{"kind":"arxiv","id":"2006.06696","version":2},"attestation_state":"computed","paper":{"title":"Duality and Supersymmetry Constraints on the Weak Gravity Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Gary Shiu, Gregory J. Loges, Toshifumi Noumi","submitted_at":"2020-06-11T18:00:03Z","abstract_excerpt":"Positivity bounds coming from consistency of UV scattering amplitudes are in general insufficient to prove the weak gravity conjecture for theories beyond Einstein-Maxwell. Additional ingredients about the UV may be necessary to exclude those regions of parameter space which are na\\\"ively in conflict with the predictions of the weak gravity conjecture. In this paper we explore the consequences of imposing additional symmetries inherited from the UV theory on higher-derivative operators for Einstein-Maxwell-dilaton-axion theory. Using black hole thermodynamics, for a preserved SL($2,\\mathbb{R}$"},"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":"2006.06696","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2020-06-11T18:00:03Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"ea9172ae6c78d94c8cd79d3c358f653f43a31eaa2f67aac9573bd1c427eb1095","abstract_canon_sha256":"d87374e2ca4f2eedd2b25a412e0593fa3197988c8a44ee348b0a6cff071d65e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:52:59.144069Z","signature_b64":"xcHFksqLqym1q5d5BITWdCpXnvfEZAzq4FLe2nHFY56TTkOIWmf9SUooUgYBffqi+aqscmt2twixSKZKGeikCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"85eb686e4dbab2681699824cc3d09227c4ee77f360aa6e9a514d0a617b63f812","last_reissued_at":"2026-07-05T01:52:59.143744Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:52:59.143744Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Duality and Supersymmetry Constraints on the Weak Gravity Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Gary Shiu, Gregory J. Loges, Toshifumi Noumi","submitted_at":"2020-06-11T18:00:03Z","abstract_excerpt":"Positivity bounds coming from consistency of UV scattering amplitudes are in general insufficient to prove the weak gravity conjecture for theories beyond Einstein-Maxwell. Additional ingredients about the UV may be necessary to exclude those regions of parameter space which are na\\\"ively in conflict with the predictions of the weak gravity conjecture. In this paper we explore the consequences of imposing additional symmetries inherited from the UV theory on higher-derivative operators for Einstein-Maxwell-dilaton-axion theory. Using black hole thermodynamics, for a preserved SL($2,\\mathbb{R}$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.06696","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/2006.06696/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":"2006.06696","created_at":"2026-07-05T01:52:59.143793+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.06696v2","created_at":"2026-07-05T01:52:59.143793+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.06696","created_at":"2026-07-05T01:52:59.143793+00:00"},{"alias_kind":"pith_short_12","alias_value":"QXVWQ3SNXKZG","created_at":"2026-07-05T01:52:59.143793+00:00"},{"alias_kind":"pith_short_16","alias_value":"QXVWQ3SNXKZGQFUZ","created_at":"2026-07-05T01:52:59.143793+00:00"},{"alias_kind":"pith_short_8","alias_value":"QXVWQ3SN","created_at":"2026-07-05T01:52:59.143793+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2404.07980","citing_title":"ISCOs and the weak gravity conjecture bound in higher derivative theories of gravity","ref_index":22,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7","json":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7.json","graph_json":"https://pith.science/api/pith-number/QXVWQ3SNXKZGQFUZQJGMHUESE7/graph.json","events_json":"https://pith.science/api/pith-number/QXVWQ3SNXKZGQFUZQJGMHUESE7/events.json","paper":"https://pith.science/paper/QXVWQ3SN"},"agent_actions":{"view_html":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7","download_json":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7.json","view_paper":"https://pith.science/paper/QXVWQ3SN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.06696&json=true","fetch_graph":"https://pith.science/api/pith-number/QXVWQ3SNXKZGQFUZQJGMHUESE7/graph.json","fetch_events":"https://pith.science/api/pith-number/QXVWQ3SNXKZGQFUZQJGMHUESE7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7/action/storage_attestation","attest_author":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7/action/author_attestation","sign_citation":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7/action/citation_signature","submit_replication":"https://pith.science/pith/QXVWQ3SNXKZGQFUZQJGMHUESE7/action/replication_record"}},"created_at":"2026-07-05T01:52:59.143793+00:00","updated_at":"2026-07-05T01:52:59.143793+00:00"}