{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TDCHGJLERKFFBQ73Y2OWGDUVXY","short_pith_number":"pith:TDCHGJLE","schema_version":"1.0","canonical_sha256":"98c47325648a8a50c3fbc69d630e95be37a35dc9123686d4b67438b2a839eda5","source":{"kind":"arxiv","id":"2305.16919","version":2},"attestation_state":"computed","paper":{"title":"CMB Anomalies and the Hubble Tension","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"William Giar\\`e","submitted_at":"2023-05-26T13:33:18Z","abstract_excerpt":"The standard $\\Lambda$CDM model of cosmology is largely successful in describing many observations, including precise measurements of the Cosmic Microwave Background (CMB) radiation. However, some intriguing anomalies remain currently unexplained within this theoretical framework. Such discrepancies can be broadly categorized into two groups: those involving CMB-independent probes and those within different CMB experiments. Examples of the former category include the $H_0$-tension between the value of the present-day expansion rate of the Universe inferred by CMB observations and local distanc"},"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":"2305.16919","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-05-26T13:33:18Z","cross_cats_sorted":[],"title_canon_sha256":"489f30728f4ace485ff117ddaea41a273a139aa73d7fc88d870a435c33d80737","abstract_canon_sha256":"94887859ba5cd0203613bee5df53f6327f4cdbd9ec0244a51cfecfd720bab7dc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:06:00.128383Z","signature_b64":"jVD7YM2Z+j1ZDPxg7kZxe9nQF7fqkkY8LR8n3s2LaN09BbYNmqXEhDLeZRhkZGOzfkRxQ7bWG6DAQ8V2Nf30Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98c47325648a8a50c3fbc69d630e95be37a35dc9123686d4b67438b2a839eda5","last_reissued_at":"2026-07-05T09:06:00.127884Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:06:00.127884Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CMB Anomalies and the Hubble Tension","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"William Giar\\`e","submitted_at":"2023-05-26T13:33:18Z","abstract_excerpt":"The standard $\\Lambda$CDM model of cosmology is largely successful in describing many observations, including precise measurements of the Cosmic Microwave Background (CMB) radiation. However, some intriguing anomalies remain currently unexplained within this theoretical framework. Such discrepancies can be broadly categorized into two groups: those involving CMB-independent probes and those within different CMB experiments. Examples of the former category include the $H_0$-tension between the value of the present-day expansion rate of the Universe inferred by CMB observations and local distanc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.16919","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/2305.16919/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":"2305.16919","created_at":"2026-07-05T09:06:00.127942+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.16919v2","created_at":"2026-07-05T09:06:00.127942+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.16919","created_at":"2026-07-05T09:06:00.127942+00:00"},{"alias_kind":"pith_short_12","alias_value":"TDCHGJLERKFF","created_at":"2026-07-05T09:06:00.127942+00:00"},{"alias_kind":"pith_short_16","alias_value":"TDCHGJLERKFFBQ73","created_at":"2026-07-05T09:06:00.127942+00:00"},{"alias_kind":"pith_short_8","alias_value":"TDCHGJLE","created_at":"2026-07-05T09:06:00.127942+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.01226","citing_title":"Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation","ref_index":103,"is_internal_anchor":false},{"citing_arxiv_id":"2605.26116","citing_title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","ref_index":23,"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":13,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21456","citing_title":"Negative neutrino mass or negative dark energy?","ref_index":73,"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":15,"is_internal_anchor":false},{"citing_arxiv_id":"2601.14222","citing_title":"Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension","ref_index":55,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY","json":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY.json","graph_json":"https://pith.science/api/pith-number/TDCHGJLERKFFBQ73Y2OWGDUVXY/graph.json","events_json":"https://pith.science/api/pith-number/TDCHGJLERKFFBQ73Y2OWGDUVXY/events.json","paper":"https://pith.science/paper/TDCHGJLE"},"agent_actions":{"view_html":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY","download_json":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY.json","view_paper":"https://pith.science/paper/TDCHGJLE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.16919&json=true","fetch_graph":"https://pith.science/api/pith-number/TDCHGJLERKFFBQ73Y2OWGDUVXY/graph.json","fetch_events":"https://pith.science/api/pith-number/TDCHGJLERKFFBQ73Y2OWGDUVXY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY/action/storage_attestation","attest_author":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY/action/author_attestation","sign_citation":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY/action/citation_signature","submit_replication":"https://pith.science/pith/TDCHGJLERKFFBQ73Y2OWGDUVXY/action/replication_record"}},"created_at":"2026-07-05T09:06:00.127942+00:00","updated_at":"2026-07-05T09:06:00.127942+00:00"}