{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:22XOMSZD6X6RGTZ65HP6RVCIM4","short_pith_number":"pith:22XOMSZD","schema_version":"1.0","canonical_sha256":"d6aee64b23f5fd134f3ee9dfe8d4486726a331e9615f76ca9789681622371aeb","source":{"kind":"arxiv","id":"1812.01012","version":2},"attestation_state":"computed","paper":{"title":"Spin-2 and the Weak Gravity Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andrew J. Tolley, Claudia de Rham, Lavinia Heisenberg","submitted_at":"2018-12-03T19:00:01Z","abstract_excerpt":"Recently, it has been argued that application of the Weak Gravity Conjecture (WGC) to spin-2 fields implies a universal upper bound on the cutoff of the effective theory for a single spin-2 field. We point out here that these arguments are largely spurious, because of the absence of states carrying spin-2 Stuckelberg $U(1)$ charge, and because of incorrect scaling assumptions. Known examples such as Kaluza-Klein theory that respect the usual WGC do so because of the existence of a genuine $U(1)$ field under which states are charged, as in the case of the Stuckelberg formulation of spin-1 theor"},"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":"1812.01012","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2018-12-03T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"49a22cd39612ce50619e59094b76ae47960a5f8b85f7bb00a0c3d8f0228b4de6","abstract_canon_sha256":"15a34f25cb0a9834b287fdc16f210002fa1ec6a7d1b1ea3dd4fa3940622ae4b5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:21:47.928348Z","signature_b64":"UE4KOyXgO7LZRg7AhC+8cQNDXZ/hzFkC2f/YeGZo4jOYmS6itjbkf/oh8xpOIqcrm5glJWPQahevnkMBuPfwBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d6aee64b23f5fd134f3ee9dfe8d4486726a331e9615f76ca9789681622371aeb","last_reissued_at":"2026-07-05T00:21:47.927866Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:21:47.927866Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spin-2 and the Weak Gravity Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andrew J. Tolley, Claudia de Rham, Lavinia Heisenberg","submitted_at":"2018-12-03T19:00:01Z","abstract_excerpt":"Recently, it has been argued that application of the Weak Gravity Conjecture (WGC) to spin-2 fields implies a universal upper bound on the cutoff of the effective theory for a single spin-2 field. We point out here that these arguments are largely spurious, because of the absence of states carrying spin-2 Stuckelberg $U(1)$ charge, and because of incorrect scaling assumptions. Known examples such as Kaluza-Klein theory that respect the usual WGC do so because of the existence of a genuine $U(1)$ field under which states are charged, as in the case of the Stuckelberg formulation of spin-1 theor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.01012","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/1812.01012/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":"1812.01012","created_at":"2026-07-05T00:21:47.927923+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.01012v2","created_at":"2026-07-05T00:21:47.927923+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.01012","created_at":"2026-07-05T00:21:47.927923+00:00"},{"alias_kind":"pith_short_12","alias_value":"22XOMSZD6X6R","created_at":"2026-07-05T00:21:47.927923+00:00"},{"alias_kind":"pith_short_16","alias_value":"22XOMSZD6X6RGTZ6","created_at":"2026-07-05T00:21:47.927923+00:00"},{"alias_kind":"pith_short_8","alias_value":"22XOMSZD","created_at":"2026-07-05T00:21:47.927923+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1909.00881","citing_title":"The Speed of Gravity","ref_index":63,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4","json":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4.json","graph_json":"https://pith.science/api/pith-number/22XOMSZD6X6RGTZ65HP6RVCIM4/graph.json","events_json":"https://pith.science/api/pith-number/22XOMSZD6X6RGTZ65HP6RVCIM4/events.json","paper":"https://pith.science/paper/22XOMSZD"},"agent_actions":{"view_html":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4","download_json":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4.json","view_paper":"https://pith.science/paper/22XOMSZD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.01012&json=true","fetch_graph":"https://pith.science/api/pith-number/22XOMSZD6X6RGTZ65HP6RVCIM4/graph.json","fetch_events":"https://pith.science/api/pith-number/22XOMSZD6X6RGTZ65HP6RVCIM4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4/action/storage_attestation","attest_author":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4/action/author_attestation","sign_citation":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4/action/citation_signature","submit_replication":"https://pith.science/pith/22XOMSZD6X6RGTZ65HP6RVCIM4/action/replication_record"}},"created_at":"2026-07-05T00:21:47.927923+00:00","updated_at":"2026-07-05T00:21:47.927923+00:00"}