{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:TR4HLLO7LRZHC6RJ2HHI7VJY6H","short_pith_number":"pith:TR4HLLO7","schema_version":"1.0","canonical_sha256":"9c7875addf5c72717a29d1ce8fd538f1d795e471a7d8ccddf75567588696c5dd","source":{"kind":"arxiv","id":"1202.4228","version":3},"attestation_state":"computed","paper":{"title":"Holographic Dark Energy Characterized by the Total Comoving Horizon and Insights to Cosmological Constant and Coincidence Problem","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Yue-Liang Wu, Zhuo-Peng Huang","submitted_at":"2012-02-20T05:13:11Z","abstract_excerpt":"The observed acceleration of the present universe is shown to be well explained by the holographic dark energy characterized by the total comoving horizon of the universe ($\\eta$HDE). It is of interest to notice that the very large primordial part of the comoving horizon generated by the inflation of early universe makes the $\\eta$HDE behave like a cosmological constant. As a consequence, both the fine-tuning problem and the coincidence problem can reasonably be understood with the inflationary universe and holographical principle. We present a systematic analysis and obtain a consistent cosmo"},"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":"1202.4228","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-02-20T05:13:11Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"c6b99e474f20ba7cbc486a9e597beddf6752507e3f19a1850918c23e19a6c0d4","abstract_canon_sha256":"0e0e275ef9b1ca91b35f9ce3456060fe85412ee1d9866f6bfdabd5eb67ecb0d6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:23.703453Z","signature_b64":"0HQ3wSCs8/SS6RfZYfr/yjzVdNq10FxuU+PkKxOueeDNaFay0TtlqEZBZzB0AR0j6uJK1B5mhE9BtTyDC0PoAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c7875addf5c72717a29d1ce8fd538f1d795e471a7d8ccddf75567588696c5dd","last_reissued_at":"2026-05-18T01:58:23.702909Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:23.702909Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holographic Dark Energy Characterized by the Total Comoving Horizon and Insights to Cosmological Constant and Coincidence Problem","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Yue-Liang Wu, Zhuo-Peng Huang","submitted_at":"2012-02-20T05:13:11Z","abstract_excerpt":"The observed acceleration of the present universe is shown to be well explained by the holographic dark energy characterized by the total comoving horizon of the universe ($\\eta$HDE). It is of interest to notice that the very large primordial part of the comoving horizon generated by the inflation of early universe makes the $\\eta$HDE behave like a cosmological constant. As a consequence, both the fine-tuning problem and the coincidence problem can reasonably be understood with the inflationary universe and holographical principle. We present a systematic analysis and obtain a consistent cosmo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.4228","kind":"arxiv","version":3},"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":"1202.4228","created_at":"2026-05-18T01:58:23.703004+00:00"},{"alias_kind":"arxiv_version","alias_value":"1202.4228v3","created_at":"2026-05-18T01:58:23.703004+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.4228","created_at":"2026-05-18T01:58:23.703004+00:00"},{"alias_kind":"pith_short_12","alias_value":"TR4HLLO7LRZH","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"TR4HLLO7LRZHC6RJ","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"TR4HLLO7","created_at":"2026-05-18T12:27:23.164592+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2511.09467","citing_title":"Revisiting the Hubble tension problem in the framework of holographic dark energy","ref_index":74,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H","json":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H.json","graph_json":"https://pith.science/api/pith-number/TR4HLLO7LRZHC6RJ2HHI7VJY6H/graph.json","events_json":"https://pith.science/api/pith-number/TR4HLLO7LRZHC6RJ2HHI7VJY6H/events.json","paper":"https://pith.science/paper/TR4HLLO7"},"agent_actions":{"view_html":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H","download_json":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H.json","view_paper":"https://pith.science/paper/TR4HLLO7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1202.4228&json=true","fetch_graph":"https://pith.science/api/pith-number/TR4HLLO7LRZHC6RJ2HHI7VJY6H/graph.json","fetch_events":"https://pith.science/api/pith-number/TR4HLLO7LRZHC6RJ2HHI7VJY6H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H/action/storage_attestation","attest_author":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H/action/author_attestation","sign_citation":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H/action/citation_signature","submit_replication":"https://pith.science/pith/TR4HLLO7LRZHC6RJ2HHI7VJY6H/action/replication_record"}},"created_at":"2026-05-18T01:58:23.703004+00:00","updated_at":"2026-05-18T01:58:23.703004+00:00"}