{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:5JJBHCQJDCULBK3P7SMBOIBBKP","short_pith_number":"pith:5JJBHCQJ","schema_version":"1.0","canonical_sha256":"ea52138a0918a8b0ab6ffc9817202153dd0c3daa16cdfac98ac40e9c0a071368","source":{"kind":"arxiv","id":"2008.10832","version":2},"attestation_state":"computed","paper":{"title":"$T_0$ censorship of early dark energy and AdS vacua","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Gen Ye, Yun-Song Piao","submitted_at":"2020-08-25T05:58:04Z","abstract_excerpt":"Present-day temperature $T_0$ of cosmic microwave background has been precisely measured by the FIRAS experiment. We identify that the early dark energy (EDE) (non-negligible around matter-radiation equality) scenario can remain compatible with the FIRAS result, while lifting the Hubble constant $H_0$. We perform Monte Carlo Markov chain analysis to confirm our observations. We also present an $\\alpha$-attractor Anti-de Sitter (AdS) model of EDE, in which the AdS depth is consistently varied in the Monte Carlo Markov chain analysis. We found that our datasets weakly hinted the existence of an "},"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":"2008.10832","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2020-08-25T05:58:04Z","cross_cats_sorted":["gr-qc","hep-th"],"title_canon_sha256":"ed34b8bb37f9f0da34088d51131f924f74fe3b08c1b4b2c3d5af4386aa28b785","abstract_canon_sha256":"061680584264d417bf9c1f5a4f70969e45062155e885b5e83952c11179ba0255"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:49:20.235282Z","signature_b64":"r+ud/vCdPCM0vEvmxI8KiBnyFZzg8t3VNYtZILTMrBm+7U0Cgp+NCqhfjP7gmW9u4fUtQk54FMDIo8zqAdH3Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ea52138a0918a8b0ab6ffc9817202153dd0c3daa16cdfac98ac40e9c0a071368","last_reissued_at":"2026-07-05T01:49:20.234768Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:49:20.234768Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"$T_0$ censorship of early dark energy and AdS vacua","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Gen Ye, Yun-Song Piao","submitted_at":"2020-08-25T05:58:04Z","abstract_excerpt":"Present-day temperature $T_0$ of cosmic microwave background has been precisely measured by the FIRAS experiment. We identify that the early dark energy (EDE) (non-negligible around matter-radiation equality) scenario can remain compatible with the FIRAS result, while lifting the Hubble constant $H_0$. We perform Monte Carlo Markov chain analysis to confirm our observations. We also present an $\\alpha$-attractor Anti-de Sitter (AdS) model of EDE, in which the AdS depth is consistently varied in the Monte Carlo Markov chain analysis. We found that our datasets weakly hinted the existence of an "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.10832","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2008.10832/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2008.10832","created_at":"2026-07-05T01:49:20.234827+00:00"},{"alias_kind":"arxiv_version","alias_value":"2008.10832v2","created_at":"2026-07-05T01:49:20.234827+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2008.10832","created_at":"2026-07-05T01:49:20.234827+00:00"},{"alias_kind":"pith_short_12","alias_value":"5JJBHCQJDCUL","created_at":"2026-07-05T01:49:20.234827+00:00"},{"alias_kind":"pith_short_16","alias_value":"5JJBHCQJDCULBK3P","created_at":"2026-07-05T01:49:20.234827+00:00"},{"alias_kind":"pith_short_8","alias_value":"5JJBHCQJ","created_at":"2026-07-05T01:49:20.234827+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06147","citing_title":"Imprint of swampland-inspired coupled early dark energy","ref_index":103,"is_internal_anchor":true},{"citing_arxiv_id":"2606.19090","citing_title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","ref_index":59,"is_internal_anchor":false},{"citing_arxiv_id":"2606.31362","citing_title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","ref_index":298,"is_internal_anchor":false},{"citing_arxiv_id":"2402.07716","citing_title":"$\\Lambda_{\\rm s}$CDM cosmology from a type-II minimally modified gravity","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2510.18741","citing_title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","ref_index":162,"is_internal_anchor":false},{"citing_arxiv_id":"2103.01183","citing_title":"In the Realm of the Hubble tension $-$ a Review of Solutions","ref_index":124,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP","json":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP.json","graph_json":"https://pith.science/api/pith-number/5JJBHCQJDCULBK3P7SMBOIBBKP/graph.json","events_json":"https://pith.science/api/pith-number/5JJBHCQJDCULBK3P7SMBOIBBKP/events.json","paper":"https://pith.science/paper/5JJBHCQJ"},"agent_actions":{"view_html":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP","download_json":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP.json","view_paper":"https://pith.science/paper/5JJBHCQJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2008.10832&json=true","fetch_graph":"https://pith.science/api/pith-number/5JJBHCQJDCULBK3P7SMBOIBBKP/graph.json","fetch_events":"https://pith.science/api/pith-number/5JJBHCQJDCULBK3P7SMBOIBBKP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP/action/storage_attestation","attest_author":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP/action/author_attestation","sign_citation":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP/action/citation_signature","submit_replication":"https://pith.science/pith/5JJBHCQJDCULBK3P7SMBOIBBKP/action/replication_record"}},"created_at":"2026-07-05T01:49:20.234827+00:00","updated_at":"2026-07-05T01:49:20.234827+00:00"}