{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:ZAQKYBK2ENU4TF2IZ72I4HQFK4","short_pith_number":"pith:ZAQKYBK2","schema_version":"1.0","canonical_sha256":"c820ac055a2369c99748cff48e1e05570aef4c4449f6f9c4b5f07f07e2883dba","source":{"kind":"arxiv","id":"2412.02132","version":1},"attestation_state":"computed","paper":{"title":"Dynamics of spontaneous scalarization of black holes with nonlinear electromagnetic fields in anti-de Sitter spacetime","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Chao Niu, Cheng-Yong Zhang, Chong-Ye Chen, Ke-Tai Wu, Peng Liu, Yi Li, Zi-Jun Zhong","submitted_at":"2024-12-03T03:38:51Z","abstract_excerpt":"We investigate spontaneous scalarization in the Einstein-Born-Infeld-Scalar (EBIS) model with asymptotically AdS boundary conditions, revealing novel dynamical critical phenomena in black hole evolution. Through numerical analysis, we discover a distinctive ``flip\" phenomenon where the scalar field exhibits critical transitions between different stable configurations. These transitions manifest in two forms: a single flip under variations in initial perturbation amplitude or scalar-electromagnetic coupling, and a double flip when varying black hole charge. Near critical points, the system disp"},"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":"2412.02132","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-12-03T03:38:51Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"0e5c19bc1e2ea346a14b3cf41572c17e3d4cabb77ae1793d46990db921937d5e","abstract_canon_sha256":"b7ac0f8c00109cf875c02340f8202daaf0c732c24f9785b5957de323d47a0cba"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:43:44.528964Z","signature_b64":"JW17SSBRDR9mQgwDg7dDmhkg/UACbQ1zzyEIO8P8CiEgMse2RRXtw0VjwqQgwyx4fFs/olst8rypeszjrzUWBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c820ac055a2369c99748cff48e1e05570aef4c4449f6f9c4b5f07f07e2883dba","last_reissued_at":"2026-07-05T09:43:44.528458Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:43:44.528458Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamics of spontaneous scalarization of black holes with nonlinear electromagnetic fields in anti-de Sitter spacetime","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Chao Niu, Cheng-Yong Zhang, Chong-Ye Chen, Ke-Tai Wu, Peng Liu, Yi Li, Zi-Jun Zhong","submitted_at":"2024-12-03T03:38:51Z","abstract_excerpt":"We investigate spontaneous scalarization in the Einstein-Born-Infeld-Scalar (EBIS) model with asymptotically AdS boundary conditions, revealing novel dynamical critical phenomena in black hole evolution. Through numerical analysis, we discover a distinctive ``flip\" phenomenon where the scalar field exhibits critical transitions between different stable configurations. These transitions manifest in two forms: a single flip under variations in initial perturbation amplitude or scalar-electromagnetic coupling, and a double flip when varying black hole charge. Near critical points, the system disp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.02132","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/2412.02132/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":"2412.02132","created_at":"2026-07-05T09:43:44.528518+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.02132v1","created_at":"2026-07-05T09:43:44.528518+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.02132","created_at":"2026-07-05T09:43:44.528518+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZAQKYBK2ENU4","created_at":"2026-07-05T09:43:44.528518+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZAQKYBK2ENU4TF2I","created_at":"2026-07-05T09:43:44.528518+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZAQKYBK2","created_at":"2026-07-05T09:43:44.528518+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.00879","citing_title":"Rotating Black Holes in Einstein-Born-Infeld Theory","ref_index":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4","json":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4.json","graph_json":"https://pith.science/api/pith-number/ZAQKYBK2ENU4TF2IZ72I4HQFK4/graph.json","events_json":"https://pith.science/api/pith-number/ZAQKYBK2ENU4TF2IZ72I4HQFK4/events.json","paper":"https://pith.science/paper/ZAQKYBK2"},"agent_actions":{"view_html":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4","download_json":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4.json","view_paper":"https://pith.science/paper/ZAQKYBK2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.02132&json=true","fetch_graph":"https://pith.science/api/pith-number/ZAQKYBK2ENU4TF2IZ72I4HQFK4/graph.json","fetch_events":"https://pith.science/api/pith-number/ZAQKYBK2ENU4TF2IZ72I4HQFK4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4/action/storage_attestation","attest_author":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4/action/author_attestation","sign_citation":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4/action/citation_signature","submit_replication":"https://pith.science/pith/ZAQKYBK2ENU4TF2IZ72I4HQFK4/action/replication_record"}},"created_at":"2026-07-05T09:43:44.528518+00:00","updated_at":"2026-07-05T09:43:44.528518+00:00"}