{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:RY3UELCZ6XKQDXQLLLZWKHPARR","short_pith_number":"pith:RY3UELCZ","schema_version":"1.0","canonical_sha256":"8e37422c59f5d501de0b5af3651de08c5a07a87c3b62a8458b1520c5264a7e73","source":{"kind":"arxiv","id":"2504.10464","version":1},"attestation_state":"computed","paper":{"title":"Implications of distance duality violation for the $H_0$ tension and evolving dark energy","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Ad\\`ele Poudou, Elsa M. Teixeira, Natalie B. Hogg, Thomas Montandon, Vivian Poulin, William Giar\\`e","submitted_at":"2025-04-14T17:52:05Z","abstract_excerpt":"We investigate whether a violation of the distance duality relation (DDR), $D_L(z) = (1+z)^2 D_A(z)$, connecting the angular diameter and luminosity distances, can explain the Hubble tension and alter the evidence for dynamical dark energy in recent cosmological observations. We constrain five phenomenological parameterisations of DDR violation using Baryon Acoustic Oscillation measurements from the DESI survey calibrated with the sound horizon derived from \\textit{Planck} Cosmic Microwave Background data and the Pantheon+ Type Ia supernova (SNIa) catalogue calibrated with the supernova absolu"},"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":"2504.10464","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-04-14T17:52:05Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"d17882884e01858ef66573a692d4fe20086e5d57e4c8bf618cb611084d9f0bff","abstract_canon_sha256":"17d99e58c089cac2a321264d0ad3d81ff3ae78af648c0c915e474189d1d83b0f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:49:00.905964Z","signature_b64":"fHoiaO8aWY/PSSGO/Z7UT2Vi/fvOt6emLWW57XERxBUxOpc3Rb2jKTM4+AeyXLAfPDmMxMzM8uM/5ne8BB+VAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8e37422c59f5d501de0b5af3651de08c5a07a87c3b62a8458b1520c5264a7e73","last_reissued_at":"2026-07-05T10:49:00.905451Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:49:00.905451Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Implications of distance duality violation for the $H_0$ tension and evolving dark energy","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Ad\\`ele Poudou, Elsa M. Teixeira, Natalie B. Hogg, Thomas Montandon, Vivian Poulin, William Giar\\`e","submitted_at":"2025-04-14T17:52:05Z","abstract_excerpt":"We investigate whether a violation of the distance duality relation (DDR), $D_L(z) = (1+z)^2 D_A(z)$, connecting the angular diameter and luminosity distances, can explain the Hubble tension and alter the evidence for dynamical dark energy in recent cosmological observations. We constrain five phenomenological parameterisations of DDR violation using Baryon Acoustic Oscillation measurements from the DESI survey calibrated with the sound horizon derived from \\textit{Planck} Cosmic Microwave Background data and the Pantheon+ Type Ia supernova (SNIa) catalogue calibrated with the supernova absolu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.10464","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/2504.10464/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":"2504.10464","created_at":"2026-07-05T10:49:00.905514+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.10464v1","created_at":"2026-07-05T10:49:00.905514+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.10464","created_at":"2026-07-05T10:49:00.905514+00:00"},{"alias_kind":"pith_short_12","alias_value":"RY3UELCZ6XKQ","created_at":"2026-07-05T10:49:00.905514+00:00"},{"alias_kind":"pith_short_16","alias_value":"RY3UELCZ6XKQDXQL","created_at":"2026-07-05T10:49:00.905514+00:00"},{"alias_kind":"pith_short_8","alias_value":"RY3UELCZ","created_at":"2026-07-05T10:49:00.905514+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":17,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08654","citing_title":"Can Distance Duality Violation Save Late-time Solutions to the Hubble Tension?","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2606.20434","citing_title":"The Hubble tension: A decade review","ref_index":102,"is_internal_anchor":false},{"citing_arxiv_id":"2606.19090","citing_title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","ref_index":86,"is_internal_anchor":false},{"citing_arxiv_id":"2606.05853","citing_title":"Reconstructing dark energy with fewer assumptions","ref_index":88,"is_internal_anchor":false},{"citing_arxiv_id":"2606.05005","citing_title":"Neutrino mass constraints in interacting dark energy models after DESI DR2","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2607.01226","citing_title":"Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation","ref_index":151,"is_internal_anchor":false},{"citing_arxiv_id":"2605.26116","citing_title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","ref_index":143,"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":264,"is_internal_anchor":false},{"citing_arxiv_id":"2605.26050","citing_title":"Early- and Late-Time Modifications to $\\Lambda$CDM: Implications for the Hubble Tension","ref_index":67,"is_internal_anchor":false},{"citing_arxiv_id":"2602.11936","citing_title":"Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework","ref_index":190,"is_internal_anchor":false},{"citing_arxiv_id":"2510.04179","citing_title":"Crosschecking Cosmic Distances from DESI BAO and DES SNe","ref_index":33,"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":121,"is_internal_anchor":false},{"citing_arxiv_id":"2603.26560","citing_title":"Exploring the interplay of late-time dynamical dark energy and new physics before recombination","ref_index":108,"is_internal_anchor":false},{"citing_arxiv_id":"2603.27616","citing_title":"Model-independent test of the cosmic distance duality relation with recent observational data","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2604.02433","citing_title":"Cosmology-Independent Constraints on the Etherington Relation and SNeIa Absolute Magnitude Evolution from DESI-DR2","ref_index":74,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25813","citing_title":"Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension","ref_index":60,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13535","citing_title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","ref_index":77,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR","json":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR.json","graph_json":"https://pith.science/api/pith-number/RY3UELCZ6XKQDXQLLLZWKHPARR/graph.json","events_json":"https://pith.science/api/pith-number/RY3UELCZ6XKQDXQLLLZWKHPARR/events.json","paper":"https://pith.science/paper/RY3UELCZ"},"agent_actions":{"view_html":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR","download_json":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR.json","view_paper":"https://pith.science/paper/RY3UELCZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.10464&json=true","fetch_graph":"https://pith.science/api/pith-number/RY3UELCZ6XKQDXQLLLZWKHPARR/graph.json","fetch_events":"https://pith.science/api/pith-number/RY3UELCZ6XKQDXQLLLZWKHPARR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR/action/storage_attestation","attest_author":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR/action/author_attestation","sign_citation":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR/action/citation_signature","submit_replication":"https://pith.science/pith/RY3UELCZ6XKQDXQLLLZWKHPARR/action/replication_record"}},"created_at":"2026-07-05T10:49:00.905514+00:00","updated_at":"2026-07-05T10:49:00.905514+00:00"}