{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:2MEBSWGPFBPAYBQC43OH2TJZRZ","short_pith_number":"pith:2MEBSWGP","schema_version":"1.0","canonical_sha256":"d3081958cf285e0c0602e6dc7d4d398e76e689370187c120b9d56b9783793721","source":{"kind":"arxiv","id":"hep-th/0608074","version":2},"attestation_state":"computed","paper":{"title":"Gauge Fields, Fermions and Mass Gaps in 6D Brane Worlds","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"A. Salvio, S. L. Parameswaran, S. Randjbar-Daemi","submitted_at":"2006-08-11T11:07:17Z","abstract_excerpt":"We study fluctuations about axisymmetric warped brane solutions in 6D minimal gauged supergravity. Much of our analysis is general and could be applied to other scenarios. We focus on bulk sectors that could give rise to Standard Model gauge fields and charged matter. We reduce the dynamics to Schroedinger type equations plus physical boundary conditions, and obtain exact solutions for the Kaluza-Klein wave functions and discrete mass spectra. The power-law warping, as opposed to exponential in 5D, means that zero mode wave functions can be peaked on negative tension branes, but only at the pr"},"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-th/0608074","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2006-08-11T11:07:17Z","cross_cats_sorted":[],"title_canon_sha256":"c70cbeb75222202e9ef413db8d30a0f92c20b3ae3e2f522d39d103ece2920eb1","abstract_canon_sha256":"5048f77d258ce7473c8ca62698c1ad7913ef244a9124ea1f9431798d094503f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:22:42.675417Z","signature_b64":"PDlwhpgcZq791oNgGYVaKx3T8m7/W95jElyG18hnRI3CyvkghAv7vHJdS3N5+3gzs9Z8GFJzwkp0Utw0CaSgCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d3081958cf285e0c0602e6dc7d4d398e76e689370187c120b9d56b9783793721","last_reissued_at":"2026-07-04T15:22:42.674225Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:22:42.674225Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gauge Fields, Fermions and Mass Gaps in 6D Brane Worlds","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"A. Salvio, S. L. Parameswaran, S. Randjbar-Daemi","submitted_at":"2006-08-11T11:07:17Z","abstract_excerpt":"We study fluctuations about axisymmetric warped brane solutions in 6D minimal gauged supergravity. Much of our analysis is general and could be applied to other scenarios. We focus on bulk sectors that could give rise to Standard Model gauge fields and charged matter. We reduce the dynamics to Schroedinger type equations plus physical boundary conditions, and obtain exact solutions for the Kaluza-Klein wave functions and discrete mass spectra. The power-law warping, as opposed to exponential in 5D, means that zero mode wave functions can be peaked on negative tension branes, but only at the pr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0608074","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-th/0608074/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-th/0608074","created_at":"2026-07-04T15:22:42.675048+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0608074v2","created_at":"2026-07-04T15:22:42.675048+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0608074","created_at":"2026-07-04T15:22:42.675048+00:00"},{"alias_kind":"pith_short_12","alias_value":"2MEBSWGPFBPA","created_at":"2026-07-04T15:22:42.675048+00:00"},{"alias_kind":"pith_short_16","alias_value":"2MEBSWGPFBPAYBQC","created_at":"2026-07-04T15:22:42.675048+00:00"},{"alias_kind":"pith_short_8","alias_value":"2MEBSWGP","created_at":"2026-07-04T15:22:42.675048+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.13736","citing_title":"Response of Kaluza-Klein mass spectrum to deformations of rugby-ball compact space","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ","json":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ.json","graph_json":"https://pith.science/api/pith-number/2MEBSWGPFBPAYBQC43OH2TJZRZ/graph.json","events_json":"https://pith.science/api/pith-number/2MEBSWGPFBPAYBQC43OH2TJZRZ/events.json","paper":"https://pith.science/paper/2MEBSWGP"},"agent_actions":{"view_html":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ","download_json":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ.json","view_paper":"https://pith.science/paper/2MEBSWGP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0608074&json=true","fetch_graph":"https://pith.science/api/pith-number/2MEBSWGPFBPAYBQC43OH2TJZRZ/graph.json","fetch_events":"https://pith.science/api/pith-number/2MEBSWGPFBPAYBQC43OH2TJZRZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ/action/storage_attestation","attest_author":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ/action/author_attestation","sign_citation":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ/action/citation_signature","submit_replication":"https://pith.science/pith/2MEBSWGPFBPAYBQC43OH2TJZRZ/action/replication_record"}},"created_at":"2026-07-04T15:22:42.675048+00:00","updated_at":"2026-07-04T15:22:42.675048+00:00"}