{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:AUF5QNXOVL4NNUOMOOZUAOUBAB","short_pith_number":"pith:AUF5QNXO","schema_version":"1.0","canonical_sha256":"050bd836eeaaf8d6d1cc73b3403a8100506537707be41afaf528439902ae69b3","source":{"kind":"arxiv","id":"2104.11134","version":2},"attestation_state":"computed","paper":{"title":"Trapping Horizons of the Evolving Charged Wormhole and Black Bounce","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Hyat Huang, Jinbo Yang","submitted_at":"2021-04-22T15:37:44Z","abstract_excerpt":"We obtain one family of dynamic solutions in the Einstein-Maxwell-scalar(EMS) theory. Our solutions could describe the evolving charged black(white) hole or wormhole and its transition, including the case of black bounce/wormhole transition. We compare different wormhole throat definitions and suggest that the usage of trapping horizons is the most suitable choice for tracking the evolution of the dynamic black(white) hole and wormhole, and their conversion in a unified framework. Then we research several evolving processes in the appropriate parameters region, including the charge, the initia"},"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":"2104.11134","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-04-22T15:37:44Z","cross_cats_sorted":[],"title_canon_sha256":"c540c3d3265face54f680168e512cd7450814b90a34563eaca468109f3d30033","abstract_canon_sha256":"74d36b555cb5da2332c776734add8bd964dde158c098eaee59357ce2f9f4e589"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:22:21.789204Z","signature_b64":"EUbVYiY2pSpkd94HiaickPLeIl6nIfbAujv0QFkqpJDQokxowSzHnDMS8URLCqy0rWSx99NmMZGWmr96aqM3CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"050bd836eeaaf8d6d1cc73b3403a8100506537707be41afaf528439902ae69b3","last_reissued_at":"2026-07-05T03:22:21.788699Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:22:21.788699Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Trapping Horizons of the Evolving Charged Wormhole and Black Bounce","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Hyat Huang, Jinbo Yang","submitted_at":"2021-04-22T15:37:44Z","abstract_excerpt":"We obtain one family of dynamic solutions in the Einstein-Maxwell-scalar(EMS) theory. Our solutions could describe the evolving charged black(white) hole or wormhole and its transition, including the case of black bounce/wormhole transition. We compare different wormhole throat definitions and suggest that the usage of trapping horizons is the most suitable choice for tracking the evolution of the dynamic black(white) hole and wormhole, and their conversion in a unified framework. Then we research several evolving processes in the appropriate parameters region, including the charge, the initia"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2104.11134","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/2104.11134/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":"2104.11134","created_at":"2026-07-05T03:22:21.788766+00:00"},{"alias_kind":"arxiv_version","alias_value":"2104.11134v2","created_at":"2026-07-05T03:22:21.788766+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2104.11134","created_at":"2026-07-05T03:22:21.788766+00:00"},{"alias_kind":"pith_short_12","alias_value":"AUF5QNXOVL4N","created_at":"2026-07-05T03:22:21.788766+00:00"},{"alias_kind":"pith_short_16","alias_value":"AUF5QNXOVL4NNUOM","created_at":"2026-07-05T03:22:21.788766+00:00"},{"alias_kind":"pith_short_8","alias_value":"AUF5QNXO","created_at":"2026-07-05T03:22:21.788766+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.05801","citing_title":"Asymptotically-flat Black holes in Bumblebee gravity: Exact solutions and Thermodynamics","ref_index":54,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB","json":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB.json","graph_json":"https://pith.science/api/pith-number/AUF5QNXOVL4NNUOMOOZUAOUBAB/graph.json","events_json":"https://pith.science/api/pith-number/AUF5QNXOVL4NNUOMOOZUAOUBAB/events.json","paper":"https://pith.science/paper/AUF5QNXO"},"agent_actions":{"view_html":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB","download_json":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB.json","view_paper":"https://pith.science/paper/AUF5QNXO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2104.11134&json=true","fetch_graph":"https://pith.science/api/pith-number/AUF5QNXOVL4NNUOMOOZUAOUBAB/graph.json","fetch_events":"https://pith.science/api/pith-number/AUF5QNXOVL4NNUOMOOZUAOUBAB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB/action/storage_attestation","attest_author":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB/action/author_attestation","sign_citation":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB/action/citation_signature","submit_replication":"https://pith.science/pith/AUF5QNXOVL4NNUOMOOZUAOUBAB/action/replication_record"}},"created_at":"2026-07-05T03:22:21.788766+00:00","updated_at":"2026-07-05T03:22:21.788766+00:00"}