{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:WOTIBPYNVZ2FP5ZZ47GQL7D2BF","short_pith_number":"pith:WOTIBPYN","schema_version":"1.0","canonical_sha256":"b3a680bf0dae7457f739e7cd05fc7a0967945c733b675b3caf1a4639863d9a66","source":{"kind":"arxiv","id":"1308.5627","version":4},"attestation_state":"computed","paper":{"title":"The tension on the cosmological parameters from different observational data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Qing Gao, Yungui Gong","submitted_at":"2013-08-26T16:18:07Z","abstract_excerpt":"Planck measurements of the cosmic microwave background power spectra find a lower value of the Hubble constant $H_0$ and a higher value of the fractional matter energy density $\\Omega_{m0}$ for the concordance $\\Lambda$CDM model, and these results are in tension with other measurements. The {\\em Planck} group argued that the tension came either from some sources of unknown systematic errors in some astrophysical measurements or the wrong $\\Lambda$CDM model applied in fitting the data. We studied the reason for the tension on $H_0$ from different measurements by considering two dynamical dark e"},"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":"1308.5627","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-08-26T16:18:07Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"7e22c9eec03594c7c09bd991da3ff1d430864bf8595fe5f7ead97164a3c51ec4","abstract_canon_sha256":"b7f94c2e9c83ded564f4fad1ae2161057840fe38adc38582c8d0157af73ed023"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:52:56.039103Z","signature_b64":"/OBRV4wrIumSPnCOUzHJD+P4VRTObKj/an0QLSE5qasXsyYN96xig+5vxwfWCdYnYldhN1pVHIXjdp5tmoH2DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b3a680bf0dae7457f739e7cd05fc7a0967945c733b675b3caf1a4639863d9a66","last_reissued_at":"2026-05-18T02:52:56.038570Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:52:56.038570Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The tension on the cosmological parameters from different observational data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Qing Gao, Yungui Gong","submitted_at":"2013-08-26T16:18:07Z","abstract_excerpt":"Planck measurements of the cosmic microwave background power spectra find a lower value of the Hubble constant $H_0$ and a higher value of the fractional matter energy density $\\Omega_{m0}$ for the concordance $\\Lambda$CDM model, and these results are in tension with other measurements. The {\\em Planck} group argued that the tension came either from some sources of unknown systematic errors in some astrophysical measurements or the wrong $\\Lambda$CDM model applied in fitting the data. We studied the reason for the tension on $H_0$ from different measurements by considering two dynamical dark e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.5627","kind":"arxiv","version":4},"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":"1308.5627","created_at":"2026-05-18T02:52:56.038652+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.5627v4","created_at":"2026-05-18T02:52:56.038652+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.5627","created_at":"2026-05-18T02:52:56.038652+00:00"},{"alias_kind":"pith_short_12","alias_value":"WOTIBPYNVZ2F","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_16","alias_value":"WOTIBPYNVZ2FP5ZZ","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_8","alias_value":"WOTIBPYN","created_at":"2026-05-18T12:28:04.890932+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/WOTIBPYNVZ2FP5ZZ47GQL7D2BF","json":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF.json","graph_json":"https://pith.science/api/pith-number/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/graph.json","events_json":"https://pith.science/api/pith-number/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/events.json","paper":"https://pith.science/paper/WOTIBPYN"},"agent_actions":{"view_html":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF","download_json":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF.json","view_paper":"https://pith.science/paper/WOTIBPYN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.5627&json=true","fetch_graph":"https://pith.science/api/pith-number/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/graph.json","fetch_events":"https://pith.science/api/pith-number/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/action/storage_attestation","attest_author":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/action/author_attestation","sign_citation":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/action/citation_signature","submit_replication":"https://pith.science/pith/WOTIBPYNVZ2FP5ZZ47GQL7D2BF/action/replication_record"}},"created_at":"2026-05-18T02:52:56.038652+00:00","updated_at":"2026-05-18T02:52:56.038652+00:00"}