{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:OXMDMRLM34IKZY5C4M3SWGQBRY","short_pith_number":"pith:OXMDMRLM","schema_version":"1.0","canonical_sha256":"75d836456cdf10ace3a2e3372b1a018e24ece5d70e3e74ced8a0795504d3598a","source":{"kind":"arxiv","id":"1802.07035","version":2},"attestation_state":"computed","paper":{"title":"Hairy black hole solutions in $U(1)$ gauge-invariant scalar-vector-tensor theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Lavinia Heisenberg, Shinji Tsujikawa","submitted_at":"2018-02-20T09:56:10Z","abstract_excerpt":"In $U(1)$ gauge-invariant scalar-vector-tensor theories with second-order equations of motion, we study the properties of black holes (BH) on a static and spherically symmetric background. In shift-symmetric theories invariant under the shift of scalar $\\phi \\to \\phi+c$, we show the existence of new hairy BH solutions where a cubic-order scalar-vector interaction gives rise to a scalar hair manifesting itself around the event horizon. In the presence of a quartic-order interaction besides the cubic coupling, there are also regular BH solutions endowed with scalar and vector hairs."},"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":"1802.07035","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-02-20T09:56:10Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"8fab303eff734f8d10cfae47fb13e9553a3c55ca155b17c1615e66824b82672d","abstract_canon_sha256":"1efb11f74892b78565fa923d36e01c63db73c300faaa2756814bc955924595f2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:19:02.321356Z","signature_b64":"i/J/QGAZI9mr9fTeYBHs/ctPXHzKntnv/VH9Is9jvlrzOhLKAwskCZv2+2leK1aRgBLFHKwrQKBHOcaZPssNCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"75d836456cdf10ace3a2e3372b1a018e24ece5d70e3e74ced8a0795504d3598a","last_reissued_at":"2026-05-18T00:19:02.320589Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:19:02.320589Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hairy black hole solutions in $U(1)$ gauge-invariant scalar-vector-tensor theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Lavinia Heisenberg, Shinji Tsujikawa","submitted_at":"2018-02-20T09:56:10Z","abstract_excerpt":"In $U(1)$ gauge-invariant scalar-vector-tensor theories with second-order equations of motion, we study the properties of black holes (BH) on a static and spherically symmetric background. In shift-symmetric theories invariant under the shift of scalar $\\phi \\to \\phi+c$, we show the existence of new hairy BH solutions where a cubic-order scalar-vector interaction gives rise to a scalar hair manifesting itself around the event horizon. In the presence of a quartic-order interaction besides the cubic coupling, there are also regular BH solutions endowed with scalar and vector hairs."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.07035","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":""},"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":"1802.07035","created_at":"2026-05-18T00:19:02.320700+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.07035v2","created_at":"2026-05-18T00:19:02.320700+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.07035","created_at":"2026-05-18T00:19:02.320700+00:00"},{"alias_kind":"pith_short_12","alias_value":"OXMDMRLM34IK","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_16","alias_value":"OXMDMRLM34IKZY5C","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_8","alias_value":"OXMDMRLM","created_at":"2026-05-18T12:32:43.782077+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2602.02272","citing_title":"Radial Oscillations of Neutron Stars with Vector-Induced Scalar Hair","ref_index":15,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY","json":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY.json","graph_json":"https://pith.science/api/pith-number/OXMDMRLM34IKZY5C4M3SWGQBRY/graph.json","events_json":"https://pith.science/api/pith-number/OXMDMRLM34IKZY5C4M3SWGQBRY/events.json","paper":"https://pith.science/paper/OXMDMRLM"},"agent_actions":{"view_html":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY","download_json":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY.json","view_paper":"https://pith.science/paper/OXMDMRLM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.07035&json=true","fetch_graph":"https://pith.science/api/pith-number/OXMDMRLM34IKZY5C4M3SWGQBRY/graph.json","fetch_events":"https://pith.science/api/pith-number/OXMDMRLM34IKZY5C4M3SWGQBRY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY/action/storage_attestation","attest_author":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY/action/author_attestation","sign_citation":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY/action/citation_signature","submit_replication":"https://pith.science/pith/OXMDMRLM34IKZY5C4M3SWGQBRY/action/replication_record"}},"created_at":"2026-05-18T00:19:02.320700+00:00","updated_at":"2026-05-18T00:19:02.320700+00:00"}