{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:W2YTPOEAIBOEVEPHKPKIPU6O62","short_pith_number":"pith:W2YTPOEA","schema_version":"1.0","canonical_sha256":"b6b137b880405c4a91e753d487d3cef6983e7be80454aae2fae4e7c32dd84d3f","source":{"kind":"arxiv","id":"1906.11098","version":3},"attestation_state":"computed","paper":{"title":"Scattering Amplitudes of Massive Spin-2 Kaluza-Klein States Grow Only as ${\\cal O}(s)$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Dennis Foren, Dipan Sengupta, Elizabeth Simmons, Kirtimaan A Mohan, R. Sekhar Chivukula","submitted_at":"2019-06-26T13:46:00Z","abstract_excerpt":"We present the results of the first complete calculation of the tree-level $2\\to 2$ high-energy scattering amplitudes of the longitudinal modes of massive spin-2 Kaluza-Klein states, both in the case where the internal space is a torus and in the Randall-Sundrum model where the internal space has constant negative curvature. While individual contributions to this amplitude grow as ${\\cal O}(s^5$), we demonstrate explicitly that intricate cancellations occur between different contributions, reducing the growth to ${\\cal O}(s)$, a slower rate of growth than previously argued in the literature. T"},"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":"1906.11098","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-06-26T13:46:00Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"b4b1d2cbb6dd426a59fc962861fe5e3c3122fcc188734a977658599ed6d2b98c","abstract_canon_sha256":"e6b478c53ce67c417907d70b590c02f57ca2c76b99516a14ea74861e66539be5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:46:46.494889Z","signature_b64":"z4M5fCaTUeEcVY+1qWOG4AV2LxIc+AgwQ+g3RPjGnmjOrg1AcDaTYXmbPwIJz6atZxMHEy/wyMUbWw7g64ruBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b6b137b880405c4a91e753d487d3cef6983e7be80454aae2fae4e7c32dd84d3f","last_reissued_at":"2026-07-05T00:46:46.494545Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:46:46.494545Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scattering Amplitudes of Massive Spin-2 Kaluza-Klein States Grow Only as ${\\cal O}(s)$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Dennis Foren, Dipan Sengupta, Elizabeth Simmons, Kirtimaan A Mohan, R. Sekhar Chivukula","submitted_at":"2019-06-26T13:46:00Z","abstract_excerpt":"We present the results of the first complete calculation of the tree-level $2\\to 2$ high-energy scattering amplitudes of the longitudinal modes of massive spin-2 Kaluza-Klein states, both in the case where the internal space is a torus and in the Randall-Sundrum model where the internal space has constant negative curvature. While individual contributions to this amplitude grow as ${\\cal O}(s^5$), we demonstrate explicitly that intricate cancellations occur between different contributions, reducing the growth to ${\\cal O}(s)$, a slower rate of growth than previously argued in the literature. T"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.11098","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/1906.11098/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":"1906.11098","created_at":"2026-07-05T00:46:46.494602+00:00"},{"alias_kind":"arxiv_version","alias_value":"1906.11098v3","created_at":"2026-07-05T00:46:46.494602+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.11098","created_at":"2026-07-05T00:46:46.494602+00:00"},{"alias_kind":"pith_short_12","alias_value":"W2YTPOEAIBOE","created_at":"2026-07-05T00:46:46.494602+00:00"},{"alias_kind":"pith_short_16","alias_value":"W2YTPOEAIBOEVEPH","created_at":"2026-07-05T00:46:46.494602+00:00"},{"alias_kind":"pith_short_8","alias_value":"W2YTPOEA","created_at":"2026-07-05T00:46:46.494602+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.21218","citing_title":"Radion Portal Freeze-Out Dark-Matter","ref_index":17,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62","json":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62.json","graph_json":"https://pith.science/api/pith-number/W2YTPOEAIBOEVEPHKPKIPU6O62/graph.json","events_json":"https://pith.science/api/pith-number/W2YTPOEAIBOEVEPHKPKIPU6O62/events.json","paper":"https://pith.science/paper/W2YTPOEA"},"agent_actions":{"view_html":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62","download_json":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62.json","view_paper":"https://pith.science/paper/W2YTPOEA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1906.11098&json=true","fetch_graph":"https://pith.science/api/pith-number/W2YTPOEAIBOEVEPHKPKIPU6O62/graph.json","fetch_events":"https://pith.science/api/pith-number/W2YTPOEAIBOEVEPHKPKIPU6O62/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62/action/storage_attestation","attest_author":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62/action/author_attestation","sign_citation":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62/action/citation_signature","submit_replication":"https://pith.science/pith/W2YTPOEAIBOEVEPHKPKIPU6O62/action/replication_record"}},"created_at":"2026-07-05T00:46:46.494602+00:00","updated_at":"2026-07-05T00:46:46.494602+00:00"}