{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:BHGXFCSYV3F5DYMMJVI6AHERSO","short_pith_number":"pith:BHGXFCSY","canonical_record":{"source":{"id":"1308.3076","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-08-14T10:00:32Z","cross_cats_sorted":[],"title_canon_sha256":"c000d32df98b90b22848348eda363b10de467241ad255999fef975b60f526905","abstract_canon_sha256":"75271829b2040ad20e8bd4ffc8a5cb8fe91dd7c04663696b9aaae3cf36585467"},"schema_version":"1.0"},"canonical_sha256":"09cd728a58aecbd1e18c4d51e01c9193b5544175c6c2c6479ab063b790c2ed19","source":{"kind":"arxiv","id":"1308.3076","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1308.3076","created_at":"2026-05-18T03:06:44Z"},{"alias_kind":"arxiv_version","alias_value":"1308.3076v2","created_at":"2026-05-18T03:06:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.3076","created_at":"2026-05-18T03:06:44Z"},{"alias_kind":"pith_short_12","alias_value":"BHGXFCSYV3F5","created_at":"2026-05-18T12:27:38Z"},{"alias_kind":"pith_short_16","alias_value":"BHGXFCSYV3F5DYMM","created_at":"2026-05-18T12:27:38Z"},{"alias_kind":"pith_short_8","alias_value":"BHGXFCSY","created_at":"2026-05-18T12:27:38Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:BHGXFCSYV3F5DYMMJVI6AHERSO","target":"record","payload":{"canonical_record":{"source":{"id":"1308.3076","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-08-14T10:00:32Z","cross_cats_sorted":[],"title_canon_sha256":"c000d32df98b90b22848348eda363b10de467241ad255999fef975b60f526905","abstract_canon_sha256":"75271829b2040ad20e8bd4ffc8a5cb8fe91dd7c04663696b9aaae3cf36585467"},"schema_version":"1.0"},"canonical_sha256":"09cd728a58aecbd1e18c4d51e01c9193b5544175c6c2c6479ab063b790c2ed19","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:06:44.365615Z","signature_b64":"cOH9FWXHPJ14DA2BRpizd4GNrEm8Z5N3ny+6LJZgTXMwi6GUsF5tc1cNZXtqjvcHu0Xp3OpFT74G6MO8YbMUAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"09cd728a58aecbd1e18c4d51e01c9193b5544175c6c2c6479ab063b790c2ed19","last_reissued_at":"2026-05-18T03:06:44.365208Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:06:44.365208Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1308.3076","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:06:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"aZs9D3c8+oVju5pld2alLgRVAXmAfe7laF8TMTMdcQkxFia2Mr8/8HUYkN89tSixirArOPLAMhjYb0p2Bb6xDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T19:33:11.452384Z"},"content_sha256":"a87c9fc2d4371854ff0f23fae0a024bb4788b4cdd5873892d99458e0a93d5d1a","schema_version":"1.0","event_id":"sha256:a87c9fc2d4371854ff0f23fae0a024bb4788b4cdd5873892d99458e0a93d5d1a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:BHGXFCSYV3F5DYMMJVI6AHERSO","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Topological black holes for Einstein-Gauss-Bonnet gravity with a nonminimal scalar field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Moises Bravo Gaete, Mokhtar Hassaine","submitted_at":"2013-08-14T10:00:32Z","abstract_excerpt":"We consider the Einstein-Gauss-Bonnet gravity with a negative cosmological constant together with a source given by a scalar field nonminimally coupled in arbitrary dimension D. For a certain election of the cosmological and Gauss-Bonnet coupling constants, we derive two classes of AdS black hole solutions whose horizon is planar. The first family of black holes obtained for a particular value of the nonminimal coupling parameter only depends on a constant M, and the scalar field vanishes as M=0. The second class of solutions corresponds to a two-parametric (with constants M and A) black hole "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.3076","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:06:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"tUF+rMTTi8Co1nA3I7yNArTlV/qrLCUUyJNa38+XtqVx0/jOxcbD3ZtZ3vsE69mXXqvujex5v97JpMtiXyJ1Dw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T19:33:11.452739Z"},"content_sha256":"58b7ddde1efa7d633f8880dd6cbc991d7ff69ab633805bef270cac676b9a019c","schema_version":"1.0","event_id":"sha256:58b7ddde1efa7d633f8880dd6cbc991d7ff69ab633805bef270cac676b9a019c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/BHGXFCSYV3F5DYMMJVI6AHERSO/bundle.json","state_url":"https://pith.science/pith/BHGXFCSYV3F5DYMMJVI6AHERSO/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/BHGXFCSYV3F5DYMMJVI6AHERSO/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-02T19:33:11Z","links":{"resolver":"https://pith.science/pith/BHGXFCSYV3F5DYMMJVI6AHERSO","bundle":"https://pith.science/pith/BHGXFCSYV3F5DYMMJVI6AHERSO/bundle.json","state":"https://pith.science/pith/BHGXFCSYV3F5DYMMJVI6AHERSO/state.json","well_known_bundle":"https://pith.science/.well-known/pith/BHGXFCSYV3F5DYMMJVI6AHERSO/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:BHGXFCSYV3F5DYMMJVI6AHERSO","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"75271829b2040ad20e8bd4ffc8a5cb8fe91dd7c04663696b9aaae3cf36585467","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-08-14T10:00:32Z","title_canon_sha256":"c000d32df98b90b22848348eda363b10de467241ad255999fef975b60f526905"},"schema_version":"1.0","source":{"id":"1308.3076","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1308.3076","created_at":"2026-05-18T03:06:44Z"},{"alias_kind":"arxiv_version","alias_value":"1308.3076v2","created_at":"2026-05-18T03:06:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.3076","created_at":"2026-05-18T03:06:44Z"},{"alias_kind":"pith_short_12","alias_value":"BHGXFCSYV3F5","created_at":"2026-05-18T12:27:38Z"},{"alias_kind":"pith_short_16","alias_value":"BHGXFCSYV3F5DYMM","created_at":"2026-05-18T12:27:38Z"},{"alias_kind":"pith_short_8","alias_value":"BHGXFCSY","created_at":"2026-05-18T12:27:38Z"}],"graph_snapshots":[{"event_id":"sha256:58b7ddde1efa7d633f8880dd6cbc991d7ff69ab633805bef270cac676b9a019c","target":"graph","created_at":"2026-05-18T03:06:44Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We consider the Einstein-Gauss-Bonnet gravity with a negative cosmological constant together with a source given by a scalar field nonminimally coupled in arbitrary dimension D. For a certain election of the cosmological and Gauss-Bonnet coupling constants, we derive two classes of AdS black hole solutions whose horizon is planar. The first family of black holes obtained for a particular value of the nonminimal coupling parameter only depends on a constant M, and the scalar field vanishes as M=0. The second class of solutions corresponds to a two-parametric (with constants M and A) black hole ","authors_text":"Moises Bravo Gaete, Mokhtar Hassaine","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-08-14T10:00:32Z","title":"Topological black holes for Einstein-Gauss-Bonnet gravity with a nonminimal scalar field"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.3076","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:a87c9fc2d4371854ff0f23fae0a024bb4788b4cdd5873892d99458e0a93d5d1a","target":"record","created_at":"2026-05-18T03:06:44Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"75271829b2040ad20e8bd4ffc8a5cb8fe91dd7c04663696b9aaae3cf36585467","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-08-14T10:00:32Z","title_canon_sha256":"c000d32df98b90b22848348eda363b10de467241ad255999fef975b60f526905"},"schema_version":"1.0","source":{"id":"1308.3076","kind":"arxiv","version":2}},"canonical_sha256":"09cd728a58aecbd1e18c4d51e01c9193b5544175c6c2c6479ab063b790c2ed19","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"09cd728a58aecbd1e18c4d51e01c9193b5544175c6c2c6479ab063b790c2ed19","first_computed_at":"2026-05-18T03:06:44.365208Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:06:44.365208Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"cOH9FWXHPJ14DA2BRpizd4GNrEm8Z5N3ny+6LJZgTXMwi6GUsF5tc1cNZXtqjvcHu0Xp3OpFT74G6MO8YbMUAw==","signature_status":"signed_v1","signed_at":"2026-05-18T03:06:44.365615Z","signed_message":"canonical_sha256_bytes"},"source_id":"1308.3076","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:a87c9fc2d4371854ff0f23fae0a024bb4788b4cdd5873892d99458e0a93d5d1a","sha256:58b7ddde1efa7d633f8880dd6cbc991d7ff69ab633805bef270cac676b9a019c"],"state_sha256":"38de5f99f67556db6cef5365eb99886913fc6b1c5f4cee59134aa69ac334649b"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"YFfpSZ70GWhrDu47M7EYArisLhNVfDUAYI3BTPTeO/anebhI/YYU3s9nwBeCu9+av278lzh6iKW70K2a3BQADQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T19:33:11.454744Z","bundle_sha256":"6b18a4599ad59b176629be72ac78b52973cd0c4fe481f0d427eaf438cd865193"}}