{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:3YNELUYOWBJD5WCZ2YE4HP4NL2","short_pith_number":"pith:3YNELUYO","schema_version":"1.0","canonical_sha256":"de1a45d30eb0523ed859d609c3bf8d5e9fa68e397b92d19b971e9528e5c701c3","source":{"kind":"arxiv","id":"1107.3532","version":2},"attestation_state":"computed","paper":{"title":"Dynamics and constraints of the dissipative Liouville cosmology","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Barcelona U.), CERN), Ific), INAOE, Manolis Plionis (Athens Observ., Nick E. Mavromatos (King's Coll. London, Puebla), Spyros Basilakos (Athens Academy, Vasiliki A. Mitsou (Valencia U.","submitted_at":"2011-07-18T19:28:57Z","abstract_excerpt":"In this article we investigate the properties of the FLRW flat cosmological models in which the cosmic expansion of the Universe is affected by a dilaton dark energy (Liouville scenario). In particular, we perform a detailed study of these models in the light of the latest cosmological data, which serves to illustrate the phenomenological viability of the new dark energy paradigm as a serious alternative to the traditional scalar field approaches. By performing a joint likelihood analysis of the recent supernovae type Ia data (SNIa), the differential ages of passively evolving galaxies, and th"},"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":"1107.3532","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-07-18T19:28:57Z","cross_cats_sorted":["gr-qc","hep-th"],"title_canon_sha256":"8f8213bc73fc17deb48540be01d576b73a79f109a569649026b9d6435aaf8072","abstract_canon_sha256":"2e078b9aa93248c411bc2200b6fdd7aa46618e73cc0b412322ffcdf67fa1d980"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:45:53.332471Z","signature_b64":"l5JsHG1jRTTkgODTo9Ry3qpSymR5WtCcbYT0Xo78ulIhAPZtbs6qRaidAqkt4c0+KqCFhpDu81K3DTuf3QF5Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de1a45d30eb0523ed859d609c3bf8d5e9fa68e397b92d19b971e9528e5c701c3","last_reissued_at":"2026-05-18T03:45:53.331648Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:45:53.331648Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamics and constraints of the dissipative Liouville cosmology","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Barcelona U.), CERN), Ific), INAOE, Manolis Plionis (Athens Observ., Nick E. Mavromatos (King's Coll. London, Puebla), Spyros Basilakos (Athens Academy, Vasiliki A. Mitsou (Valencia U.","submitted_at":"2011-07-18T19:28:57Z","abstract_excerpt":"In this article we investigate the properties of the FLRW flat cosmological models in which the cosmic expansion of the Universe is affected by a dilaton dark energy (Liouville scenario). In particular, we perform a detailed study of these models in the light of the latest cosmological data, which serves to illustrate the phenomenological viability of the new dark energy paradigm as a serious alternative to the traditional scalar field approaches. By performing a joint likelihood analysis of the recent supernovae type Ia data (SNIa), the differential ages of passively evolving galaxies, and th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.3532","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":""},"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":"1107.3532","created_at":"2026-05-18T03:45:53.331775+00:00"},{"alias_kind":"arxiv_version","alias_value":"1107.3532v2","created_at":"2026-05-18T03:45:53.331775+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.3532","created_at":"2026-05-18T03:45:53.331775+00:00"},{"alias_kind":"pith_short_12","alias_value":"3YNELUYOWBJD","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_16","alias_value":"3YNELUYOWBJD5WCZ","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_8","alias_value":"3YNELUYO","created_at":"2026-05-18T12:26:20.644004+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2","json":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2.json","graph_json":"https://pith.science/api/pith-number/3YNELUYOWBJD5WCZ2YE4HP4NL2/graph.json","events_json":"https://pith.science/api/pith-number/3YNELUYOWBJD5WCZ2YE4HP4NL2/events.json","paper":"https://pith.science/paper/3YNELUYO"},"agent_actions":{"view_html":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2","download_json":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2.json","view_paper":"https://pith.science/paper/3YNELUYO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1107.3532&json=true","fetch_graph":"https://pith.science/api/pith-number/3YNELUYOWBJD5WCZ2YE4HP4NL2/graph.json","fetch_events":"https://pith.science/api/pith-number/3YNELUYOWBJD5WCZ2YE4HP4NL2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2/action/storage_attestation","attest_author":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2/action/author_attestation","sign_citation":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2/action/citation_signature","submit_replication":"https://pith.science/pith/3YNELUYOWBJD5WCZ2YE4HP4NL2/action/replication_record"}},"created_at":"2026-05-18T03:45:53.331775+00:00","updated_at":"2026-05-18T03:45:53.331775+00:00"}