{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:SCBJD74W2MP3W4KNX5RPXCHRMR","short_pith_number":"pith:SCBJD74W","schema_version":"1.0","canonical_sha256":"908291ff96d31fbb714dbf62fb88f1644b4a49a02c175acfa1447bc5db63b36d","source":{"kind":"arxiv","id":"gr-qc/9605059","version":1},"attestation_state":"computed","paper":{"title":"Black hole hair: twenty--five years after","license":"","headline":"","cross_cats":["astro-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Jacob D. Bekenstein","submitted_at":"1996-05-28T12:41:00Z","abstract_excerpt":"Originally regarded as forbidden, black hole ``hair'' are fields associated with a stationary black hole apart from the gravitational and electromagnetic ones. Several stable stationary black hole solutions with gauge or Skyrme field hair are known today within general relativity. We formulate here a ``no scalar--hair'' conjecture, and adduce some new theorems that almost establish it by ruling out - for all but a small parameter range - scalar field hair of spherical black holes in general relativity, whether the field be self--interacting, coupled to an Abelian gauge field, or nonminimally c"},"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":"gr-qc/9605059","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1996-05-28T12:41:00Z","cross_cats_sorted":["astro-ph","hep-th"],"title_canon_sha256":"8b33d3a922ccae0c6bcb2089e5cac35f252b2bcee8b9326b525456a47bbf4903","abstract_canon_sha256":"f710aafc148512c767f54f9938e54128060186275be0e95e8e82b414333d4a71"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:26:04.646787Z","signature_b64":"BaM0xOPxgyARJqzRlQP1hRb+5HURB+/9tF8dFu1Rhr/dfkQmuwc7fdcG9A95YhbPrdNWH4of/WQOr3hs1u3uCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"908291ff96d31fbb714dbf62fb88f1644b4a49a02c175acfa1447bc5db63b36d","last_reissued_at":"2026-07-04T14:26:04.646398Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:26:04.646398Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black hole hair: twenty--five years after","license":"","headline":"","cross_cats":["astro-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Jacob D. Bekenstein","submitted_at":"1996-05-28T12:41:00Z","abstract_excerpt":"Originally regarded as forbidden, black hole ``hair'' are fields associated with a stationary black hole apart from the gravitational and electromagnetic ones. Several stable stationary black hole solutions with gauge or Skyrme field hair are known today within general relativity. We formulate here a ``no scalar--hair'' conjecture, and adduce some new theorems that almost establish it by ruling out - for all but a small parameter range - scalar field hair of spherical black holes in general relativity, whether the field be self--interacting, coupled to an Abelian gauge field, or nonminimally c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9605059","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/gr-qc/9605059/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":"gr-qc/9605059","created_at":"2026-07-04T14:26:04.646461+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9605059v1","created_at":"2026-07-04T14:26:04.646461+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9605059","created_at":"2026-07-04T14:26:04.646461+00:00"},{"alias_kind":"pith_short_12","alias_value":"SCBJD74W2MP3","created_at":"2026-07-04T14:26:04.646461+00:00"},{"alias_kind":"pith_short_16","alias_value":"SCBJD74W2MP3W4KN","created_at":"2026-07-04T14:26:04.646461+00:00"},{"alias_kind":"pith_short_8","alias_value":"SCBJD74W","created_at":"2026-07-04T14:26:04.646461+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2605.20320","citing_title":"Ringdown and lensing of triple systems","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2603.22398","citing_title":"Stable black hole solutions with cosmological hair","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13036","citing_title":"Inspiral gravitational waveforms from charged compact binaries with scalar hair","ref_index":27,"is_internal_anchor":true},{"citing_arxiv_id":"2505.23895","citing_title":"Black hole spectroscopy: from theory to experiment","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2604.08951","citing_title":"Weyl-type solutions with multipolar scalar fields","ref_index":27,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR","json":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR.json","graph_json":"https://pith.science/api/pith-number/SCBJD74W2MP3W4KNX5RPXCHRMR/graph.json","events_json":"https://pith.science/api/pith-number/SCBJD74W2MP3W4KNX5RPXCHRMR/events.json","paper":"https://pith.science/paper/SCBJD74W"},"agent_actions":{"view_html":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR","download_json":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR.json","view_paper":"https://pith.science/paper/SCBJD74W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/9605059&json=true","fetch_graph":"https://pith.science/api/pith-number/SCBJD74W2MP3W4KNX5RPXCHRMR/graph.json","fetch_events":"https://pith.science/api/pith-number/SCBJD74W2MP3W4KNX5RPXCHRMR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR/action/storage_attestation","attest_author":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR/action/author_attestation","sign_citation":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR/action/citation_signature","submit_replication":"https://pith.science/pith/SCBJD74W2MP3W4KNX5RPXCHRMR/action/replication_record"}},"created_at":"2026-07-04T14:26:04.646461+00:00","updated_at":"2026-07-04T14:26:04.646461+00:00"}