{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:I3DFXA7YBFROEADDAU2FUIHKWJ","short_pith_number":"pith:I3DFXA7Y","schema_version":"1.0","canonical_sha256":"46c65b83f80962e2006305345a20eab240cfc69d14fafa7875cda85855c5cd1c","source":{"kind":"arxiv","id":"1904.09864","version":2},"attestation_state":"computed","paper":{"title":"Stability of scalarized charged black holes in the Einstein-Maxwell-Scalar theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"De-Cheng Zou, Yun Soo Myung","submitted_at":"2019-04-19T03:07:54Z","abstract_excerpt":"We analyze the stability of scalarized charged black holes in the Einstein-Maxwell-Scalar (EMS) theory with quadratic coupling. These black holes are labelled by the number of $n=0,1,2,\\cdots$, where $n=0$ is called the fundamental black hole and $n=1,2,\\cdots$ denote the $n$-excited black holes. We show that the $n=0$ black hole is stable against full perturbations, whereas the $n=1,2$ excited black holes are unstable against the $s(l=0)$-mode scalar perturbation. This is consistent with the EMS theory with exponential coupling, but it contrasts to the $n=0$ scalarized black hole in the Einst"},"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":"1904.09864","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-04-19T03:07:54Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"9f2ca6c852fefd5dacdde7b53e0920b91ee3cbf74ef2d405b98f4a51104bc4d2","abstract_canon_sha256":"2e7a3550eb3dc0e70a36791b231edc39606d42ff74743212e071b9cbec0d60d7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:56:35.761115Z","signature_b64":"bQm68LnoNqQUEmaPOhfHwiZ7QddMWOenw/ZWqnfz6T9gqDe25wXnyTrKdcjKao089+dKLjkZ9e48sqhL4uyMCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"46c65b83f80962e2006305345a20eab240cfc69d14fafa7875cda85855c5cd1c","last_reissued_at":"2026-07-04T23:56:35.760626Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:56:35.760626Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stability of scalarized charged black holes in the Einstein-Maxwell-Scalar theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"De-Cheng Zou, Yun Soo Myung","submitted_at":"2019-04-19T03:07:54Z","abstract_excerpt":"We analyze the stability of scalarized charged black holes in the Einstein-Maxwell-Scalar (EMS) theory with quadratic coupling. These black holes are labelled by the number of $n=0,1,2,\\cdots$, where $n=0$ is called the fundamental black hole and $n=1,2,\\cdots$ denote the $n$-excited black holes. We show that the $n=0$ black hole is stable against full perturbations, whereas the $n=1,2$ excited black holes are unstable against the $s(l=0)$-mode scalar perturbation. This is consistent with the EMS theory with exponential coupling, but it contrasts to the $n=0$ scalarized black hole in the Einst"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.09864","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/1904.09864/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":"1904.09864","created_at":"2026-07-04T23:56:35.760684+00:00"},{"alias_kind":"arxiv_version","alias_value":"1904.09864v2","created_at":"2026-07-04T23:56:35.760684+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1904.09864","created_at":"2026-07-04T23:56:35.760684+00:00"},{"alias_kind":"pith_short_12","alias_value":"I3DFXA7YBFRO","created_at":"2026-07-04T23:56:35.760684+00:00"},{"alias_kind":"pith_short_16","alias_value":"I3DFXA7YBFROEADD","created_at":"2026-07-04T23:56:35.760684+00:00"},{"alias_kind":"pith_short_8","alias_value":"I3DFXA7Y","created_at":"2026-07-04T23:56:35.760684+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.11652","citing_title":"Optical Appearance of Scalarized Kerr-Newman Black Holes with Multiple Light Rings","ref_index":68,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ","json":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ.json","graph_json":"https://pith.science/api/pith-number/I3DFXA7YBFROEADDAU2FUIHKWJ/graph.json","events_json":"https://pith.science/api/pith-number/I3DFXA7YBFROEADDAU2FUIHKWJ/events.json","paper":"https://pith.science/paper/I3DFXA7Y"},"agent_actions":{"view_html":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ","download_json":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ.json","view_paper":"https://pith.science/paper/I3DFXA7Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1904.09864&json=true","fetch_graph":"https://pith.science/api/pith-number/I3DFXA7YBFROEADDAU2FUIHKWJ/graph.json","fetch_events":"https://pith.science/api/pith-number/I3DFXA7YBFROEADDAU2FUIHKWJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ/action/storage_attestation","attest_author":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ/action/author_attestation","sign_citation":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ/action/citation_signature","submit_replication":"https://pith.science/pith/I3DFXA7YBFROEADDAU2FUIHKWJ/action/replication_record"}},"created_at":"2026-07-04T23:56:35.760684+00:00","updated_at":"2026-07-04T23:56:35.760684+00:00"}