{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:77KGX5ZGGMQFBHRGBIRBUAHURK","short_pith_number":"pith:77KGX5ZG","schema_version":"1.0","canonical_sha256":"ffd46bf7263320509e260a221a00f48aa167b43d19b9f357796e35ecd9f0632b","source":{"kind":"arxiv","id":"2502.07206","version":1},"attestation_state":"computed","paper":{"title":"Einstein-Maxwell-Dilaton Wormholes that meet the Energy Conditions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Leonel Bixano, Tonatiuh Matos","submitted_at":"2025-02-11T03:01:21Z","abstract_excerpt":"One of the latest predictions of Einstein's theory is the existence of Wormholes (WH). In this work, we present exact solutions of the Einstein-Maxwell-Dilaton equations representing traversable Wormholes. These solutions satisfy the energy conditions and have a ring singularity satisfying the cosmic censorship of WHs, i.e. we show that, as in previous solutions, geodesics cannot touch the singularity. We find that the most optimal input regions for the first class of solutions traversing these wormholes are near the poles and near the equatorial plane for the second class. We also find that 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":"2502.07206","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-02-11T03:01:21Z","cross_cats_sorted":[],"title_canon_sha256":"5da6fa6da58dd111b04e6b2b52f7b88ccb10d019e6e52bef4e25d44181dffd06","abstract_canon_sha256":"f30313dc23d50031c0fa0bb76990139808be6551f1dea804117caedca828433e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:47:19.127815Z","signature_b64":"08s8Am2IVyXWy3/jG7th6reg3Q8vPOntThxXpzpOGQyilL7Znq8g11IUX3MGzx5MSkwvMQNecCgIZkmdewHmBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ffd46bf7263320509e260a221a00f48aa167b43d19b9f357796e35ecd9f0632b","last_reissued_at":"2026-07-05T11:47:19.127328Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:47:19.127328Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Einstein-Maxwell-Dilaton Wormholes that meet the Energy Conditions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Leonel Bixano, Tonatiuh Matos","submitted_at":"2025-02-11T03:01:21Z","abstract_excerpt":"One of the latest predictions of Einstein's theory is the existence of Wormholes (WH). In this work, we present exact solutions of the Einstein-Maxwell-Dilaton equations representing traversable Wormholes. These solutions satisfy the energy conditions and have a ring singularity satisfying the cosmic censorship of WHs, i.e. we show that, as in previous solutions, geodesics cannot touch the singularity. We find that the most optimal input regions for the first class of solutions traversing these wormholes are near the poles and near the equatorial plane for the second class. We also find that t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.07206","kind":"arxiv","version":1},"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/2502.07206/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":"2502.07206","created_at":"2026-07-05T11:47:19.127387+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.07206v1","created_at":"2026-07-05T11:47:19.127387+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.07206","created_at":"2026-07-05T11:47:19.127387+00:00"},{"alias_kind":"pith_short_12","alias_value":"77KGX5ZGGMQF","created_at":"2026-07-05T11:47:19.127387+00:00"},{"alias_kind":"pith_short_16","alias_value":"77KGX5ZGGMQFBHRG","created_at":"2026-07-05T11:47:19.127387+00:00"},{"alias_kind":"pith_short_8","alias_value":"77KGX5ZG","created_at":"2026-07-05T11:47:19.127387+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.07206","citing_title":"Einstein-Maxwell-Dilaton Wormholes that meet the Energy Conditions","ref_index":4,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK","json":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK.json","graph_json":"https://pith.science/api/pith-number/77KGX5ZGGMQFBHRGBIRBUAHURK/graph.json","events_json":"https://pith.science/api/pith-number/77KGX5ZGGMQFBHRGBIRBUAHURK/events.json","paper":"https://pith.science/paper/77KGX5ZG"},"agent_actions":{"view_html":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK","download_json":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK.json","view_paper":"https://pith.science/paper/77KGX5ZG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.07206&json=true","fetch_graph":"https://pith.science/api/pith-number/77KGX5ZGGMQFBHRGBIRBUAHURK/graph.json","fetch_events":"https://pith.science/api/pith-number/77KGX5ZGGMQFBHRGBIRBUAHURK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK/action/storage_attestation","attest_author":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK/action/author_attestation","sign_citation":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK/action/citation_signature","submit_replication":"https://pith.science/pith/77KGX5ZGGMQFBHRGBIRBUAHURK/action/replication_record"}},"created_at":"2026-07-05T11:47:19.127387+00:00","updated_at":"2026-07-05T11:47:19.127387+00:00"}