{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:7MS32PJ6VNNQJHKHOGVHZB6LF7","short_pith_number":"pith:7MS32PJ6","schema_version":"1.0","canonical_sha256":"fb25bd3d3eab5b049d4771aa7c87cb2fe581aa27c8768b86430a6ef6b875dc8d","source":{"kind":"arxiv","id":"2211.14325","version":3},"attestation_state":"computed","paper":{"title":"Implications of the Weak Gravity Conjecture for Tidal Love Numbers of Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Justin Khoury, Sam S. C. Wong, Valerio De Luca","submitted_at":"2022-11-25T19:00:00Z","abstract_excerpt":"The Weak Gravity Conjecture indicates that extremal black holes in the low energy effective field theory should be able to decay. This criterion gives rise to non-trivial constraints on the coefficients of higher-order derivative corrections to gravity. In this paper, we investigate the tidal deformability of neutral black holes due to higher-order derivative corrections. As a proof of concept, we consider a correction of cubic order in the Riemann curvature tensor. The tidal Love numbers of neutral black holes receive leading-order corrections from higher-order derivative terms, since black h"},"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":"2211.14325","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-11-25T19:00:00Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"1c0cb8b1873279255098155f753d1e3c87c486fb192d21a59f43064a0a7e3f19","abstract_canon_sha256":"17f90c8bde6523b8edf35bdd554b05a022e1b2168b0ed4d4a95158e54187fa48"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:58:36.800053Z","signature_b64":"fYfTDAMK4dun0JHUswSCGNCKKXOkLQIWd/4vHbyu06BE4S6kVd2Kr6WndBjpUdwPV1TKIRyvXMeh6KSUq3RcDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fb25bd3d3eab5b049d4771aa7c87cb2fe581aa27c8768b86430a6ef6b875dc8d","last_reissued_at":"2026-07-05T06:58:36.799569Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:58:36.799569Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Implications of the Weak Gravity Conjecture for Tidal Love Numbers of Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Justin Khoury, Sam S. C. Wong, Valerio De Luca","submitted_at":"2022-11-25T19:00:00Z","abstract_excerpt":"The Weak Gravity Conjecture indicates that extremal black holes in the low energy effective field theory should be able to decay. This criterion gives rise to non-trivial constraints on the coefficients of higher-order derivative corrections to gravity. In this paper, we investigate the tidal deformability of neutral black holes due to higher-order derivative corrections. As a proof of concept, we consider a correction of cubic order in the Riemann curvature tensor. The tidal Love numbers of neutral black holes receive leading-order corrections from higher-order derivative terms, since black h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.14325","kind":"arxiv","version":3},"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/2211.14325/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":"2211.14325","created_at":"2026-07-05T06:58:36.799629+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.14325v3","created_at":"2026-07-05T06:58:36.799629+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.14325","created_at":"2026-07-05T06:58:36.799629+00:00"},{"alias_kind":"pith_short_12","alias_value":"7MS32PJ6VNNQ","created_at":"2026-07-05T06:58:36.799629+00:00"},{"alias_kind":"pith_short_16","alias_value":"7MS32PJ6VNNQJHKH","created_at":"2026-07-05T06:58:36.799629+00:00"},{"alias_kind":"pith_short_8","alias_value":"7MS32PJ6","created_at":"2026-07-05T06:58:36.799629+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19446","citing_title":"Dynamical Tidal Response of Neutron Stars: from Effective Field Theory to Gravitational Waveforms","ref_index":68,"is_internal_anchor":false},{"citing_arxiv_id":"2606.07070","citing_title":"Gravitational waveforms from binaries in higher-derivative gravity: a Love story","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2509.06630","citing_title":"Positivity bounds from thermal field theory entropy","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2511.12580","citing_title":"Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2512.05767","citing_title":"Tidal Love numbers for regular black holes","ref_index":40,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03025","citing_title":"Can wormholes have vanishing Love numbers?","ref_index":29,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7","json":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7.json","graph_json":"https://pith.science/api/pith-number/7MS32PJ6VNNQJHKHOGVHZB6LF7/graph.json","events_json":"https://pith.science/api/pith-number/7MS32PJ6VNNQJHKHOGVHZB6LF7/events.json","paper":"https://pith.science/paper/7MS32PJ6"},"agent_actions":{"view_html":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7","download_json":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7.json","view_paper":"https://pith.science/paper/7MS32PJ6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.14325&json=true","fetch_graph":"https://pith.science/api/pith-number/7MS32PJ6VNNQJHKHOGVHZB6LF7/graph.json","fetch_events":"https://pith.science/api/pith-number/7MS32PJ6VNNQJHKHOGVHZB6LF7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7/action/storage_attestation","attest_author":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7/action/author_attestation","sign_citation":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7/action/citation_signature","submit_replication":"https://pith.science/pith/7MS32PJ6VNNQJHKHOGVHZB6LF7/action/replication_record"}},"created_at":"2026-07-05T06:58:36.799629+00:00","updated_at":"2026-07-05T06:58:36.799629+00:00"}