{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:AXAK5RFPVTCZKB3LUR4XORFTQY","short_pith_number":"pith:AXAK5RFP","schema_version":"1.0","canonical_sha256":"05c0aec4afacc595076ba4797744b38637738df835e6b424b383cf5c49987edd","source":{"kind":"arxiv","id":"hep-th/9610013","version":1},"attestation_state":"computed","paper":{"title":"Stationary Dilatons with Arbitrary Electromagnetic Field","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Cesar Mora (CNVESTAV-IPN), Tonatiuh Matos (Ifm, UMSNH)","submitted_at":"1996-10-02T21:21:30Z","abstract_excerpt":"We present two new classes of axisymmetric stationary solutions of the Einstein-Maxwell-Dilaton equations with coupling constant $\\alpha^2=3$. Both classes are written in terms of two harmonic maps $\\lambda$ and $\\tau$. $\\lambda$ determines the gravitational potential and $\\tau$ the electromagnetic one in such a form that we can have an arbitrary electromagnetic field. As examples we generate two solutions with mass ($M$), rotation ($s$) and scalar ($\\delta$) parameters, one with electric charge ($q$) another one with magnetic dipole ($Q$) parameter. The first solution contains the Kerr metric"},"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/9610013","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1996-10-02T21:21:30Z","cross_cats_sorted":[],"title_canon_sha256":"38d96beaa9dcbc084f836b38441d93d49bb752141b9b88d87e70563cf6c7eb02","abstract_canon_sha256":"6df1aa0efdc40b303c0f503ba795eafb47790568e8bf628c5e427c08795e92ef"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:36:03.042577Z","signature_b64":"zUVmj8giZScPR2E/oI0OKC4nxN7Uf7XGtxZqyaEVgwbVhlRC/NdMf++hQnheS12bhlj7cWmcL7EnzMaGh78HAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"05c0aec4afacc595076ba4797744b38637738df835e6b424b383cf5c49987edd","last_reissued_at":"2026-05-18T02:36:03.042074Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:36:03.042074Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stationary Dilatons with Arbitrary Electromagnetic Field","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Cesar Mora (CNVESTAV-IPN), Tonatiuh Matos (Ifm, UMSNH)","submitted_at":"1996-10-02T21:21:30Z","abstract_excerpt":"We present two new classes of axisymmetric stationary solutions of the Einstein-Maxwell-Dilaton equations with coupling constant $\\alpha^2=3$. Both classes are written in terms of two harmonic maps $\\lambda$ and $\\tau$. $\\lambda$ determines the gravitational potential and $\\tau$ the electromagnetic one in such a form that we can have an arbitrary electromagnetic field. As examples we generate two solutions with mass ($M$), rotation ($s$) and scalar ($\\delta$) parameters, one with electric charge ($q$) another one with magnetic dipole ($Q$) parameter. The first solution contains the Kerr metric"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9610013","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":""},"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/9610013","created_at":"2026-05-18T02:36:03.042151+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9610013v1","created_at":"2026-05-18T02:36:03.042151+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9610013","created_at":"2026-05-18T02:36:03.042151+00:00"},{"alias_kind":"pith_short_12","alias_value":"AXAK5RFPVTCZ","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_16","alias_value":"AXAK5RFPVTCZKB3L","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_8","alias_value":"AXAK5RFP","created_at":"2026-05-18T12:25:47.700082+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.17843","citing_title":"Potential Space Symmetries in Ernst-like Formulations of Einstein-Maxwell/ModMax-Scalar field Theories","ref_index":32,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY","json":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY.json","graph_json":"https://pith.science/api/pith-number/AXAK5RFPVTCZKB3LUR4XORFTQY/graph.json","events_json":"https://pith.science/api/pith-number/AXAK5RFPVTCZKB3LUR4XORFTQY/events.json","paper":"https://pith.science/paper/AXAK5RFP"},"agent_actions":{"view_html":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY","download_json":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY.json","view_paper":"https://pith.science/paper/AXAK5RFP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9610013&json=true","fetch_graph":"https://pith.science/api/pith-number/AXAK5RFPVTCZKB3LUR4XORFTQY/graph.json","fetch_events":"https://pith.science/api/pith-number/AXAK5RFPVTCZKB3LUR4XORFTQY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY/action/storage_attestation","attest_author":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY/action/author_attestation","sign_citation":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY/action/citation_signature","submit_replication":"https://pith.science/pith/AXAK5RFPVTCZKB3LUR4XORFTQY/action/replication_record"}},"created_at":"2026-05-18T02:36:03.042151+00:00","updated_at":"2026-05-18T02:36:03.042151+00:00"}