{"paper":{"title":"Generation of gravitating solutions with Baryonic charge from Einstein-Scalar-Maxwell seeds","license":"http://creativecommons.org/licenses/by/4.0/","headline":"An exact correspondence maps Einstein-scalar-Maxwell solutions onto gauged Skyrme-Maxwell-Einstein spacetimes carrying baryonic charge.","cross_cats":["hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Anibal Neira, Fabrizio Canfora, Seung Hun Oh","submitted_at":"2026-01-25T14:50:47Z","abstract_excerpt":"We establish, for the first time, an exact correspondence between Einstein-scalar-Maxwell theory and gauged Skyrme-Maxwell-Einstein models in (3+1) dimensions. By constructing the simplest consistent ansatz within the gauged Skyrme-Maxwell framework, we reveal a remarkable equivalence in a sector that admits nonvanishing, highly magnetized baryonic charge. This correspondence has a particularly appealing consequence: it transfers the full power of solution-generating techniques developed for electrovacuum systems-many of which naturally accommodate scalar fields to the considerably more intric"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"We establish, for the first time, an exact correspondence between Einstein-scalar-Maxwell theory and gauged Skyrme-Maxwell-Einstein models in (3+1) dimensions.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"By constructing the simplest consistent ansatz within the gauged Skyrme-Maxwell framework, we reveal a remarkable equivalence in a sector that admits nonvanishing, highly magnetized baryonic charge.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"Exact correspondence maps Einstein-scalar-Maxwell solutions to gauged Skyrme-Maxwell-Einstein solutions with baryonic charge, illustrated by a Kerr-Newman-like example where baryonic charge quantization enforces quantization of the Kerr rotation parameter.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"An exact correspondence maps Einstein-scalar-Maxwell solutions onto gauged Skyrme-Maxwell-Einstein spacetimes carrying baryonic charge.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"7b12a156c7c2613cfee4be1e9e37992e16621a4ac9394f53ff3bfbad6a0e8c47"},"source":{"id":"2601.17864","kind":"arxiv","version":2},"verdict":{"id":"5e016ef2-3401-4b9c-9cfc-d2d4ef218989","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-16T11:07:39.349012Z","strongest_claim":"We establish, for the first time, an exact correspondence between Einstein-scalar-Maxwell theory and gauged Skyrme-Maxwell-Einstein models in (3+1) dimensions.","one_line_summary":"Exact correspondence maps Einstein-scalar-Maxwell solutions to gauged Skyrme-Maxwell-Einstein solutions with baryonic charge, illustrated by a Kerr-Newman-like example where baryonic charge quantization enforces quantization of the Kerr rotation parameter.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"By constructing the simplest consistent ansatz within the gauged Skyrme-Maxwell framework, we reveal a remarkable equivalence in a sector that admits nonvanishing, highly magnetized baryonic charge.","pith_extraction_headline":"An exact correspondence maps Einstein-scalar-Maxwell solutions onto gauged Skyrme-Maxwell-Einstein spacetimes carrying baryonic charge."},"references":{"count":57,"sample":[{"doi":"","year":2002,"title":"Effects of strong magnetic fields in strange baryonic matter,","work_id":"f4025aee-00d8-4e18-bbab-dfe5b60d8b05","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2009,"title":"Physics, Astro- physics and Cosmology with Gravitational Waves,","work_id":"2ada39e3-7567-477d-b3ea-2d6a91cf8949","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2018,"title":"Baryons under Strong Magnetic Fields or in Theories with Space-dependent $\\theta$-term","work_id":"5a7b1ad2-2389-4d7c-9633-632f526e9097","ref_index":3,"cited_arxiv_id":"1805.08245","is_internal_anchor":true},{"doi":"","year":2020,"title":"Searching optimum equations of state of neutron star matter in the presence of magnetic fields and rotation,","work_id":"27695c08-2419-4109-9b00-2d1e96018ccc","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2022,"title":"Neutron Stars with Baryon Number Violation, Probing Dark Sectors","work_id":"da6438b9-303c-43c7-b4a2-99c02cf6372e","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":57,"snapshot_sha256":"6a629a119fc2685540e98b81f876a992589a0027028175a00ddc9cb2180aeecf","internal_anchors":3},"formal_canon":{"evidence_count":2,"snapshot_sha256":"b0328a5e51c0366f58137bfc4416f3fac88b8365e1c4ea4274ef6ffa72951054"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}