{"paper":{"title":"Dyonic Ellis-Bronnikov wormholes from warped extra dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"Regular asymptotically flat traversable wormholes in four dimensions arise from a five-dimensional Einstein-Maxwell-Chern-Simons theory via warped compactification.","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Francisco S. N. Lobo, Manuel E. Rodrigues, Miguel A. S. Pinto","submitted_at":"2026-05-02T20:40:16Z","abstract_excerpt":"We investigate traversable wormhole solutions within a four-dimensional effective theory derived from a five-dimensional Einstein-Maxwell-Chern-Simons action with a non-minimally coupled scalar field. A warped Kaluza-Klein compactification yields an Einstein-frame theory containing a phantom dilaton, a canonical axion, a Maxwell field, and a Kaluza-Klein vector, with the couplings fixed by the higher-dimensional origin. Focusing on the Ellis-Bronnikov geometry, we construct solutions that incorporate both dyonic Maxwell and Kaluza-Klein fields. For exponential gauge couplings, the Einstein equ"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"These results show that regular, asymptotically flat traversable four-dimensional wormholes arise naturally from higher-dimensional scalar-tensor theories.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The assumption that the warped Kaluza-Klein reduction of the five-dimensional Einstein-Maxwell-Chern-Simons action with non-minimally coupled scalar produces an effective four-dimensional theory whose field content (phantom dilaton, canonical axion, Maxwell and Kaluza-Klein vectors) can support the Ellis-Bronnikov metric without introducing singularities or violating the required energy conditions.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"Dyonic Ellis-Bronnikov wormholes supported by phantom dilaton, axion, and dyonic gauge fields arise from warped five-dimensional scalar-tensor theories via Kaluza-Klein reduction.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"Regular asymptotically flat traversable wormholes in four dimensions arise from a five-dimensional Einstein-Maxwell-Chern-Simons theory via warped compactification.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"ca2012545c94fd1e7895179b15490309f3f0523aae4128acd47880cf66ac9171"},"source":{"id":"2605.01602","kind":"arxiv","version":1},"verdict":{"id":"b603086a-c507-486e-9101-3f1fef424d2f","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-09T17:45:27.777776Z","strongest_claim":"These results show that regular, asymptotically flat traversable four-dimensional wormholes arise naturally from higher-dimensional scalar-tensor theories.","one_line_summary":"Dyonic Ellis-Bronnikov wormholes supported by phantom dilaton, axion, and dyonic gauge fields arise from warped five-dimensional scalar-tensor theories via Kaluza-Klein reduction.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The assumption that the warped Kaluza-Klein reduction of the five-dimensional Einstein-Maxwell-Chern-Simons action with non-minimally coupled scalar produces an effective four-dimensional theory whose field content (phantom dilaton, canonical axion, Maxwell and Kaluza-Klein vectors) can support the Ellis-Bronnikov metric without introducing singularities or violating the required energy conditions.","pith_extraction_headline":"Regular asymptotically flat traversable wormholes in four dimensions arise from a five-dimensional Einstein-Maxwell-Chern-Simons theory via warped compactification."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.01602/integrity.json","findings":[],"available":true,"detectors_run":[{"name":"ai_meta_artifact","ran_at":"2026-05-20T17:39:15.062401Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"doi_compliance","ran_at":"2026-05-19T17:08:14.836876Z","status":"completed","version":"1.0.0","findings_count":0}],"snapshot_sha256":"6ef6c65e19238515140918de90aaee7f16ec954dfd2e17e5f31bf2f6425035b8"},"references":{"count":28,"sample":[{"doi":"","year":1988,"title":"M. S. Morris and K. S. Thorne, Am. J. Phys.56(1988), 395-412","work_id":"d53b8eb6-be10-4efe-afc8-bccdf29aa060","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1988,"title":"M. S. Morris, K. S. Thorne and U. Yurtsever, Phys. Rev. 6 Lett.61(1988), 1446-1449","work_id":"4872684f-b6ad-4e49-bb25-b6797188a9c1","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2013,"title":"Modified-gravity wormholes without exotic matter","work_id":"ad230ddc-78a2-4354-af4b-0e7517db02fe","ref_index":3,"cited_arxiv_id":"1301.6878","is_internal_anchor":false},{"doi":"","year":2021,"title":"Traversable wormholes in Einstein-Dirac-Maxwell theory","work_id":"870527b9-5d1a-4f12-b96c-06c86feeb3ce","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2022,"title":"R. A. Konoplya and A. Zhidenko, Phys. Rev. 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