{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:JFNDA6JJ653N34YLOJD62EJNAM","short_pith_number":"pith:JFNDA6JJ","schema_version":"1.0","canonical_sha256":"495a307929f776ddf30b7247ed112d0328e7ac4743ee7ff91013e761da043ab6","source":{"kind":"arxiv","id":"hep-th/9605089","version":1},"attestation_state":"computed","paper":{"title":"Cosmological Analogues of the Bartnik--McKinnon Solutions","license":"","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"G. Lavrelashvili, M. Heusler, M.S. Volkov, N. Straumann, O. Brodbeck","submitted_at":"1996-05-13T16:20:38Z","abstract_excerpt":"We present a numerical classification of the spherically symmetric, static solutions to the Einstein--Yang--Mills equations with cosmological constant $\\Lambda$. We find three qualitatively different classes of configurations, where the solutions in each class are characterized by the value of $\\Lambda$ and the number of nodes, $n$, of the Yang--Mills amplitude. For sufficiently small, positive values of the cosmological constant, $\\Lambda < \\Llow(n)$, the solutions generalize the Bartnik--McKinnon solitons, which are now surrounded by a cosmological horizon and approach the deSitter geometry "},"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":"hep-th/9605089","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1996-05-13T16:20:38Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"401c7d948f3476f632257b87531aa9ce080fceb70fc368d59adab26e9273a2e6","abstract_canon_sha256":"1ec818ed4dae0db927b5af856f60e04e2bfe85a984ebb3b5b793b8b1066eb8de"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:06:00.808625Z","signature_b64":"858rRogtFfpPe4wechmAWMKLqlSH0fTu9Wr7RnrE9J8xMTXKGvoEwn+DJp1AoiaKL7FobS7m1RrM5Kt/cQo4BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"495a307929f776ddf30b7247ed112d0328e7ac4743ee7ff91013e761da043ab6","last_reissued_at":"2026-05-18T01:06:00.808236Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:06:00.808236Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological Analogues of the Bartnik--McKinnon Solutions","license":"","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"G. Lavrelashvili, M. Heusler, M.S. Volkov, N. Straumann, O. Brodbeck","submitted_at":"1996-05-13T16:20:38Z","abstract_excerpt":"We present a numerical classification of the spherically symmetric, static solutions to the Einstein--Yang--Mills equations with cosmological constant $\\Lambda$. We find three qualitatively different classes of configurations, where the solutions in each class are characterized by the value of $\\Lambda$ and the number of nodes, $n$, of the Yang--Mills amplitude. For sufficiently small, positive values of the cosmological constant, $\\Lambda < \\Llow(n)$, the solutions generalize the Bartnik--McKinnon solitons, which are now surrounded by a cosmological horizon and approach the deSitter geometry "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9605089","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":""},"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":"hep-th/9605089","created_at":"2026-05-18T01:06:00.808292+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9605089v1","created_at":"2026-05-18T01:06:00.808292+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9605089","created_at":"2026-05-18T01:06:00.808292+00:00"},{"alias_kind":"pith_short_12","alias_value":"JFNDA6JJ653N","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_16","alias_value":"JFNDA6JJ653N34YL","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_8","alias_value":"JFNDA6JJ","created_at":"2026-05-18T12:25:47.700082+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM","json":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM.json","graph_json":"https://pith.science/api/pith-number/JFNDA6JJ653N34YLOJD62EJNAM/graph.json","events_json":"https://pith.science/api/pith-number/JFNDA6JJ653N34YLOJD62EJNAM/events.json","paper":"https://pith.science/paper/JFNDA6JJ"},"agent_actions":{"view_html":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM","download_json":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM.json","view_paper":"https://pith.science/paper/JFNDA6JJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9605089&json=true","fetch_graph":"https://pith.science/api/pith-number/JFNDA6JJ653N34YLOJD62EJNAM/graph.json","fetch_events":"https://pith.science/api/pith-number/JFNDA6JJ653N34YLOJD62EJNAM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM/action/storage_attestation","attest_author":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM/action/author_attestation","sign_citation":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM/action/citation_signature","submit_replication":"https://pith.science/pith/JFNDA6JJ653N34YLOJD62EJNAM/action/replication_record"}},"created_at":"2026-05-18T01:06:00.808292+00:00","updated_at":"2026-05-18T01:06:00.808292+00:00"}