{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:X6FI6TI74NJSRO2N3NE3FZF64F","short_pith_number":"pith:X6FI6TI7","schema_version":"1.0","canonical_sha256":"bf8a8f4d1fe35328bb4ddb49b2e4bee17b8fefe1c29e5d215689d92d69326ae8","source":{"kind":"arxiv","id":"hep-ph/9811291","version":2},"attestation_state":"computed","paper":{"title":"Quantum Gravity and Extra Dimensions at High-Energy Colliders","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Gian F. Giudice, James D. Wells, Riccardo Rattazzi","submitted_at":"1998-11-10T15:44:32Z","abstract_excerpt":"Recently it has been pointed out that the characteristic quantum-gravity scale could be as low as the weak scale in theories with gravity propagating in higher dimensions. The observed smallness of Newton's constant is a consequence of the large compactified volume of the extra dimensions. We investigate the consequences of this supposition for high-energy collider experiments. We do this by first compactifying the higher dimensional theory and constructing a 3+1-dimensional low-energy effective field theory of the graviton Kaluza-Klein excitations and their interactions with ordinary matter. "},"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-ph/9811291","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1998-11-10T15:44:32Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"e7a49ebf97db0e5a50a2b21c0467410ced2f35d2adaaac0be8e65c4429710fa3","abstract_canon_sha256":"dafe52aaacffd3d092bc6df4904b376d10132c4b1c6d64ebf6e1647d9bf587e1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:09:35.443392Z","signature_b64":"MLT7QXlsQEmw4eXZrPQOBIn2M/3+g5DxFgmo1J74gK/bK6suWR4enIM4EeVzEyO64G1sisYixiqFrSU0wlX0CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bf8a8f4d1fe35328bb4ddb49b2e4bee17b8fefe1c29e5d215689d92d69326ae8","last_reissued_at":"2026-07-04T16:09:35.442996Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:09:35.442996Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum Gravity and Extra Dimensions at High-Energy Colliders","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Gian F. Giudice, James D. Wells, Riccardo Rattazzi","submitted_at":"1998-11-10T15:44:32Z","abstract_excerpt":"Recently it has been pointed out that the characteristic quantum-gravity scale could be as low as the weak scale in theories with gravity propagating in higher dimensions. The observed smallness of Newton's constant is a consequence of the large compactified volume of the extra dimensions. We investigate the consequences of this supposition for high-energy collider experiments. We do this by first compactifying the higher dimensional theory and constructing a 3+1-dimensional low-energy effective field theory of the graviton Kaluza-Klein excitations and their interactions with ordinary matter. "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9811291","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-ph/9811291/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-ph/9811291","created_at":"2026-07-04T16:09:35.443053+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9811291v2","created_at":"2026-07-04T16:09:35.443053+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9811291","created_at":"2026-07-04T16:09:35.443053+00:00"},{"alias_kind":"pith_short_12","alias_value":"X6FI6TI74NJS","created_at":"2026-07-04T16:09:35.443053+00:00"},{"alias_kind":"pith_short_16","alias_value":"X6FI6TI74NJSRO2N","created_at":"2026-07-04T16:09:35.443053+00:00"},{"alias_kind":"pith_short_8","alias_value":"X6FI6TI7","created_at":"2026-07-04T16:09:35.443053+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.23178","citing_title":"Signatures of gravity-mediated dark matter interaction in theories with large extra dimensions","ref_index":24,"is_internal_anchor":true},{"citing_arxiv_id":"2512.03146","citing_title":"Homotopy transfer for massive Kaluza-Klein modes","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"hep-ph/9905221","citing_title":"A Large Mass Hierarchy from a Small Extra Dimension","ref_index":2,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F","json":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F.json","graph_json":"https://pith.science/api/pith-number/X6FI6TI74NJSRO2N3NE3FZF64F/graph.json","events_json":"https://pith.science/api/pith-number/X6FI6TI74NJSRO2N3NE3FZF64F/events.json","paper":"https://pith.science/paper/X6FI6TI7"},"agent_actions":{"view_html":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F","download_json":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F.json","view_paper":"https://pith.science/paper/X6FI6TI7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9811291&json=true","fetch_graph":"https://pith.science/api/pith-number/X6FI6TI74NJSRO2N3NE3FZF64F/graph.json","fetch_events":"https://pith.science/api/pith-number/X6FI6TI74NJSRO2N3NE3FZF64F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F/action/storage_attestation","attest_author":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F/action/author_attestation","sign_citation":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F/action/citation_signature","submit_replication":"https://pith.science/pith/X6FI6TI74NJSRO2N3NE3FZF64F/action/replication_record"}},"created_at":"2026-07-04T16:09:35.443053+00:00","updated_at":"2026-07-04T16:09:35.443053+00:00"}