{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:2YLSXY7WN3OZN6GYOTZJQIEPSA","short_pith_number":"pith:2YLSXY7W","schema_version":"1.0","canonical_sha256":"d6172be3f66edd96f8d874f298208f900fc50a6778ccc8b38b6b542f6a4b74ee","source":{"kind":"arxiv","id":"1104.1181","version":2},"attestation_state":"computed","paper":{"title":"The cosmology of an holographic induced gravity model with curvature effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Ahmed Errahmani, Mariam Bouhmadi-Lopez, Taoufiq Ouali","submitted_at":"2011-04-06T20:01:13Z","abstract_excerpt":"We present an holographic model of the Dvali-Gabadadze-Porrati scenario with a Gauss-Bonnet term in the bulk. We concentrate on the solution that generalises the normal Dvali-Gabadadze-Porrati branch. It is well known that this branch cannot describe the late-time acceleration of the universe even with the inclusion of a Gauss-Bonnet term. Here, we show that this branch in the presence of a Gauss-Bonnet curvature effect and an holographic dark energy with the Hubble scale as the infra-red cutoff can describe the late-time acceleration of the universe. It is worthwhile to stress that such an en"},"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":"1104.1181","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-04-06T20:01:13Z","cross_cats_sorted":["gr-qc","hep-th"],"title_canon_sha256":"acdf87b698158f85728e90e6dd2d7ec738380eec9446e9efd6e56d7b9d1a01d9","abstract_canon_sha256":"2b3093814ca2ce848b47a40f749ec382a4d49aefa0a15ea16aea8e0a25f76cec"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:23:34.903629Z","signature_b64":"DUV5Gym3pbDMUvTKhiXae0vUPop9TOKBZV4jCwFv17VkDtkoNBMqzN3PYtrqX5N21eHmC7JddYInZFbD12pWBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d6172be3f66edd96f8d874f298208f900fc50a6778ccc8b38b6b542f6a4b74ee","last_reissued_at":"2026-05-18T03:23:34.902896Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:23:34.902896Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The cosmology of an holographic induced gravity model with curvature effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Ahmed Errahmani, Mariam Bouhmadi-Lopez, Taoufiq Ouali","submitted_at":"2011-04-06T20:01:13Z","abstract_excerpt":"We present an holographic model of the Dvali-Gabadadze-Porrati scenario with a Gauss-Bonnet term in the bulk. We concentrate on the solution that generalises the normal Dvali-Gabadadze-Porrati branch. It is well known that this branch cannot describe the late-time acceleration of the universe even with the inclusion of a Gauss-Bonnet term. Here, we show that this branch in the presence of a Gauss-Bonnet curvature effect and an holographic dark energy with the Hubble scale as the infra-red cutoff can describe the late-time acceleration of the universe. It is worthwhile to stress that such an en"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.1181","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":"1104.1181","created_at":"2026-05-18T03:23:34.903011+00:00"},{"alias_kind":"arxiv_version","alias_value":"1104.1181v2","created_at":"2026-05-18T03:23:34.903011+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1104.1181","created_at":"2026-05-18T03:23:34.903011+00:00"},{"alias_kind":"pith_short_12","alias_value":"2YLSXY7WN3OZ","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_16","alias_value":"2YLSXY7WN3OZN6GY","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_8","alias_value":"2YLSXY7W","created_at":"2026-05-18T12:26:18.847500+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/2YLSXY7WN3OZN6GYOTZJQIEPSA","json":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA.json","graph_json":"https://pith.science/api/pith-number/2YLSXY7WN3OZN6GYOTZJQIEPSA/graph.json","events_json":"https://pith.science/api/pith-number/2YLSXY7WN3OZN6GYOTZJQIEPSA/events.json","paper":"https://pith.science/paper/2YLSXY7W"},"agent_actions":{"view_html":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA","download_json":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA.json","view_paper":"https://pith.science/paper/2YLSXY7W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1104.1181&json=true","fetch_graph":"https://pith.science/api/pith-number/2YLSXY7WN3OZN6GYOTZJQIEPSA/graph.json","fetch_events":"https://pith.science/api/pith-number/2YLSXY7WN3OZN6GYOTZJQIEPSA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA/action/storage_attestation","attest_author":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA/action/author_attestation","sign_citation":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA/action/citation_signature","submit_replication":"https://pith.science/pith/2YLSXY7WN3OZN6GYOTZJQIEPSA/action/replication_record"}},"created_at":"2026-05-18T03:23:34.903011+00:00","updated_at":"2026-05-18T03:23:34.903011+00:00"}