{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:2SAK2Y6WZCMCBB2PQDI7BFMOXS","short_pith_number":"pith:2SAK2Y6W","schema_version":"1.0","canonical_sha256":"d480ad63d6c89820874f80d1f0958ebc9b8c50ab6c0c497ce9d1004de3dc1e48","source":{"kind":"arxiv","id":"2302.00067","version":1},"attestation_state":"computed","paper":{"title":"Emergent Unparticles Dark Energy can restore cosmological concordance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Ido Ben-Dayan, Utkarsh Kumar","submitted_at":"2023-01-31T20:01:05Z","abstract_excerpt":"Addressing the discrepancy between the late and early time measurements of the Hubble parameter, $H_0$, and the so-called $S_8$ parameter has been a challenge in precision cosmology. Several models are present to address these tensions, but very few of them can do so simultaneously. In the past, we have suggested Banks-Zaks/Unparticles as an emergent Dark Energy model and claimed that it can ameliorate the Hubble tension. In this work, we test this claim and perform a likelihood analysis of the model and its parameters are given current data and compare it to $\\Lambda$CDM. The model offers a p"},"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":"2302.00067","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-01-31T20:01:05Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"35a70ff0aa3a871370546c14b878836d27fc2feffc57e3471d78e223f3d667ab","abstract_canon_sha256":"47861d5217b550e6298a66fd839f77c79371361e11e94be649d6f9183d8a4dc0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:37:59.028762Z","signature_b64":"PKQqWo7/lCJ0Hr1dtoPAmcxjaypKFWeldYi82byCL1GiZOeb7XQ6FtO6+O/zAzYcvSbDFcz1YxD+2RoOZ9t4Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d480ad63d6c89820874f80d1f0958ebc9b8c50ab6c0c497ce9d1004de3dc1e48","last_reissued_at":"2026-07-05T05:37:59.028227Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:37:59.028227Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Emergent Unparticles Dark Energy can restore cosmological concordance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Ido Ben-Dayan, Utkarsh Kumar","submitted_at":"2023-01-31T20:01:05Z","abstract_excerpt":"Addressing the discrepancy between the late and early time measurements of the Hubble parameter, $H_0$, and the so-called $S_8$ parameter has been a challenge in precision cosmology. Several models are present to address these tensions, but very few of them can do so simultaneously. In the past, we have suggested Banks-Zaks/Unparticles as an emergent Dark Energy model and claimed that it can ameliorate the Hubble tension. In this work, we test this claim and perform a likelihood analysis of the model and its parameters are given current data and compare it to $\\Lambda$CDM. The model offers a p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.00067","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/2302.00067/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":"2302.00067","created_at":"2026-07-05T05:37:59.028301+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.00067v1","created_at":"2026-07-05T05:37:59.028301+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.00067","created_at":"2026-07-05T05:37:59.028301+00:00"},{"alias_kind":"pith_short_12","alias_value":"2SAK2Y6WZCMC","created_at":"2026-07-05T05:37:59.028301+00:00"},{"alias_kind":"pith_short_16","alias_value":"2SAK2Y6WZCMCBB2P","created_at":"2026-07-05T05:37:59.028301+00:00"},{"alias_kind":"pith_short_8","alias_value":"2SAK2Y6W","created_at":"2026-07-05T05:37:59.028301+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"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":206,"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":59,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS","json":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS.json","graph_json":"https://pith.science/api/pith-number/2SAK2Y6WZCMCBB2PQDI7BFMOXS/graph.json","events_json":"https://pith.science/api/pith-number/2SAK2Y6WZCMCBB2PQDI7BFMOXS/events.json","paper":"https://pith.science/paper/2SAK2Y6W"},"agent_actions":{"view_html":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS","download_json":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS.json","view_paper":"https://pith.science/paper/2SAK2Y6W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.00067&json=true","fetch_graph":"https://pith.science/api/pith-number/2SAK2Y6WZCMCBB2PQDI7BFMOXS/graph.json","fetch_events":"https://pith.science/api/pith-number/2SAK2Y6WZCMCBB2PQDI7BFMOXS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS/action/storage_attestation","attest_author":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS/action/author_attestation","sign_citation":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS/action/citation_signature","submit_replication":"https://pith.science/pith/2SAK2Y6WZCMCBB2PQDI7BFMOXS/action/replication_record"}},"created_at":"2026-07-05T05:37:59.028301+00:00","updated_at":"2026-07-05T05:37:59.028301+00:00"}