{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:DVI4K7SGMADGSQMZ2GNKT36CD7","short_pith_number":"pith:DVI4K7SG","schema_version":"1.0","canonical_sha256":"1d51c57e466006694199d19aa9efc21fd53e2e925d902945dd367ce3b39d538a","source":{"kind":"arxiv","id":"2301.12172","version":3},"attestation_state":"computed","paper":{"title":"Thermal evolution and stability analysis of phenomenologically emergent dark energy model","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Rosemin John, Sarath N., Titus K. Mathew","submitted_at":"2023-01-28T12:00:09Z","abstract_excerpt":"The phenomenologically emergent dark energy (PEDE) model is a varying dark energy model with no extra degrees of freedom proposed by Li and Shafieloo\\citep{Li_2019} to alleviate the Hubble tension. The statistical consistency of the model has been discussed by many authors. Since the model depicts a phantom dark energy that increases with redshift, its cosmic evolution, particularly during the late phase, must be examined. We discover that the model's Hubble and deceleration parameters display unusual behaviour in the future, which differs from $\\Lambda$CDM cosmology. We find the model also fo"},"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":"2301.12172","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"gr-qc","submitted_at":"2023-01-28T12:00:09Z","cross_cats_sorted":[],"title_canon_sha256":"2988fd34439f5f35f2e882bbdbc075bb5d963a2c50df3365047fb07cbdc55315","abstract_canon_sha256":"24c394bc03a7f908faa3bb39f13873bd1bccae663225afa6fecc0940445fd108"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:38:36.997598Z","signature_b64":"20XDhf+Sdp4Qij8Wjxq1VC075u80tX0A/sZrjmGUO1h6yQjnLcCluXuQqEXFr4td0TM2nfab8IXx+/KtryjaBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1d51c57e466006694199d19aa9efc21fd53e2e925d902945dd367ce3b39d538a","last_reissued_at":"2026-07-05T06:38:36.997125Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:38:36.997125Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermal evolution and stability analysis of phenomenologically emergent dark energy model","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Rosemin John, Sarath N., Titus K. Mathew","submitted_at":"2023-01-28T12:00:09Z","abstract_excerpt":"The phenomenologically emergent dark energy (PEDE) model is a varying dark energy model with no extra degrees of freedom proposed by Li and Shafieloo\\citep{Li_2019} to alleviate the Hubble tension. The statistical consistency of the model has been discussed by many authors. Since the model depicts a phantom dark energy that increases with redshift, its cosmic evolution, particularly during the late phase, must be examined. We discover that the model's Hubble and deceleration parameters display unusual behaviour in the future, which differs from $\\Lambda$CDM cosmology. We find the model also fo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.12172","kind":"arxiv","version":3},"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/2301.12172/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":"2301.12172","created_at":"2026-07-05T06:38:36.997184+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.12172v3","created_at":"2026-07-05T06:38:36.997184+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.12172","created_at":"2026-07-05T06:38:36.997184+00:00"},{"alias_kind":"pith_short_12","alias_value":"DVI4K7SGMADG","created_at":"2026-07-05T06:38:36.997184+00:00"},{"alias_kind":"pith_short_16","alias_value":"DVI4K7SGMADGSQMZ","created_at":"2026-07-05T06:38:36.997184+00:00"},{"alias_kind":"pith_short_8","alias_value":"DVI4K7SG","created_at":"2026-07-05T06:38:36.997184+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.02401","citing_title":"Extended Effective Field Theory of Dark Energy: Ghost Condensate Dark Energy with Sextic Dispersion Relation in de Sitter Spacetime","ref_index":53,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7","json":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7.json","graph_json":"https://pith.science/api/pith-number/DVI4K7SGMADGSQMZ2GNKT36CD7/graph.json","events_json":"https://pith.science/api/pith-number/DVI4K7SGMADGSQMZ2GNKT36CD7/events.json","paper":"https://pith.science/paper/DVI4K7SG"},"agent_actions":{"view_html":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7","download_json":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7.json","view_paper":"https://pith.science/paper/DVI4K7SG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.12172&json=true","fetch_graph":"https://pith.science/api/pith-number/DVI4K7SGMADGSQMZ2GNKT36CD7/graph.json","fetch_events":"https://pith.science/api/pith-number/DVI4K7SGMADGSQMZ2GNKT36CD7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7/action/storage_attestation","attest_author":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7/action/author_attestation","sign_citation":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7/action/citation_signature","submit_replication":"https://pith.science/pith/DVI4K7SGMADGSQMZ2GNKT36CD7/action/replication_record"}},"created_at":"2026-07-05T06:38:36.997184+00:00","updated_at":"2026-07-05T06:38:36.997184+00:00"}