{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RNA2X3OH7TVZYDMFF52KDNCEOQ","short_pith_number":"pith:RNA2X3OH","schema_version":"1.0","canonical_sha256":"8b41abedc7fceb9c0d852f74a1b444741e2582253a0ec0977f861fb991648ec5","source":{"kind":"arxiv","id":"2408.13121","version":1},"attestation_state":"computed","paper":{"title":"The Hubble parameter of the Local Distance Ladder from dynamical dark energy with no free parameters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Maurice H.P.M. van Putten","submitted_at":"2024-08-12T09:07:51Z","abstract_excerpt":"Our cosmology contains Big Bang relic fluctuations by a loss of time-translation symmetry on a Hubble time scale. The contribution to the vacuum is identified with dynamical dark energy $\\Lambda\\simeq \\alpha_p\\Lambda_0$ by an IR coupling $\\alpha_p\\sim \\hbar$ of the bare cosmological constant $\\Lambda_0\\sim\\hbar^{-1}$ consistent with general relativity, where $\\hbar$ is the Planck constant. Described by the trace $J=(1-q)H^2$ of the Schouten tensor derived from a path integral formulation with gauged global phase, the proposed $J$CDM takes us beyond the $\\Lambda$CDM limit of frozen $J=\\Lambda$."},"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":"2408.13121","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-08-12T09:07:51Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"9905e6fee4676b859b08b4b41fd1ffc049d274e192b27a8f4e13c93b71daa50d","abstract_canon_sha256":"85fe16d63cfd32d89c6a6ae0d4846f5f1204e8bced331c48711514e8cafb595a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:58:35.608212Z","signature_b64":"8oavmTTTmvX2VjEahJKzSf15wC0uDXyaV4mtjpEK6zGGVwJg1hTiwWEGwYOaoT8IKegX4zk57emNs0Ec3CM/Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b41abedc7fceb9c0d852f74a1b444741e2582253a0ec0977f861fb991648ec5","last_reissued_at":"2026-07-05T08:58:35.607763Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:58:35.607763Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Hubble parameter of the Local Distance Ladder from dynamical dark energy with no free parameters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Maurice H.P.M. van Putten","submitted_at":"2024-08-12T09:07:51Z","abstract_excerpt":"Our cosmology contains Big Bang relic fluctuations by a loss of time-translation symmetry on a Hubble time scale. The contribution to the vacuum is identified with dynamical dark energy $\\Lambda\\simeq \\alpha_p\\Lambda_0$ by an IR coupling $\\alpha_p\\sim \\hbar$ of the bare cosmological constant $\\Lambda_0\\sim\\hbar^{-1}$ consistent with general relativity, where $\\hbar$ is the Planck constant. Described by the trace $J=(1-q)H^2$ of the Schouten tensor derived from a path integral formulation with gauged global phase, the proposed $J$CDM takes us beyond the $\\Lambda$CDM limit of frozen $J=\\Lambda$."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.13121","kind":"arxiv","version":1},"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/2408.13121/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":"2408.13121","created_at":"2026-07-05T08:58:35.607818+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.13121v1","created_at":"2026-07-05T08:58:35.607818+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.13121","created_at":"2026-07-05T08:58:35.607818+00:00"},{"alias_kind":"pith_short_12","alias_value":"RNA2X3OH7TVZ","created_at":"2026-07-05T08:58:35.607818+00:00"},{"alias_kind":"pith_short_16","alias_value":"RNA2X3OH7TVZYDMF","created_at":"2026-07-05T08:58:35.607818+00:00"},{"alias_kind":"pith_short_8","alias_value":"RNA2X3OH","created_at":"2026-07-05T08:58:35.607818+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2603.25999","citing_title":"Cosmological constraints on the big bang quantum cosmology model","ref_index":57,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ","json":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ.json","graph_json":"https://pith.science/api/pith-number/RNA2X3OH7TVZYDMFF52KDNCEOQ/graph.json","events_json":"https://pith.science/api/pith-number/RNA2X3OH7TVZYDMFF52KDNCEOQ/events.json","paper":"https://pith.science/paper/RNA2X3OH"},"agent_actions":{"view_html":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ","download_json":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ.json","view_paper":"https://pith.science/paper/RNA2X3OH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.13121&json=true","fetch_graph":"https://pith.science/api/pith-number/RNA2X3OH7TVZYDMFF52KDNCEOQ/graph.json","fetch_events":"https://pith.science/api/pith-number/RNA2X3OH7TVZYDMFF52KDNCEOQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ/action/storage_attestation","attest_author":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ/action/author_attestation","sign_citation":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ/action/citation_signature","submit_replication":"https://pith.science/pith/RNA2X3OH7TVZYDMFF52KDNCEOQ/action/replication_record"}},"created_at":"2026-07-05T08:58:35.607818+00:00","updated_at":"2026-07-05T08:58:35.607818+00:00"}