{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:MJGT3SIOHMDJWXKZFEHER3GXRT","short_pith_number":"pith:MJGT3SIO","schema_version":"1.0","canonical_sha256":"624d3dc90e3b069b5d59290e48ecd78ccc560f6134871b57eab8a9138002afe6","source":{"kind":"arxiv","id":"1605.06314","version":1},"attestation_state":"computed","paper":{"title":"Scale invariant cosmology III: dynamical models and comparisons with observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Andre Maeder","submitted_at":"2016-05-19T07:44:33Z","abstract_excerpt":"We examine the properties of the scale invariant cosmological models, also making the specific hypothesis of the scale invariance of the empty space at large scales. Numerical integrations of the cosmological equations for different values of the curvature parameter k and of the density parameter Omega_m are performed. We compare the dynamical properties of the models to the observations at different epochs. The main numerical data and graphical representations are given for models computed with different curvatures and density parameters. The models with non-zero density start explosively wit"},"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":"1605.06314","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-05-19T07:44:33Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"26938b5f52ef874a4ff83f00de608b543cd26d397e9f9f121b76490fa4416af5","abstract_canon_sha256":"23a734ba88a2ef43e0f60acc482c814da60b980f41a39fc759f227a62979326c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:46.804101Z","signature_b64":"t1zIfuL93vbtXosLKBZlmIYKBB6R3T42eMNKrDcop6Jhj2fnHqicZlczpj+eBgPJwR2DxlQH5iLsm8dxA47SDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"624d3dc90e3b069b5d59290e48ecd78ccc560f6134871b57eab8a9138002afe6","last_reissued_at":"2026-05-18T01:13:46.803427Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:46.803427Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scale invariant cosmology III: dynamical models and comparisons with observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Andre Maeder","submitted_at":"2016-05-19T07:44:33Z","abstract_excerpt":"We examine the properties of the scale invariant cosmological models, also making the specific hypothesis of the scale invariance of the empty space at large scales. Numerical integrations of the cosmological equations for different values of the curvature parameter k and of the density parameter Omega_m are performed. We compare the dynamical properties of the models to the observations at different epochs. The main numerical data and graphical representations are given for models computed with different curvatures and density parameters. The models with non-zero density start explosively wit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.06314","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":""},"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":"1605.06314","created_at":"2026-05-18T01:13:46.803535+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.06314v1","created_at":"2026-05-18T01:13:46.803535+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.06314","created_at":"2026-05-18T01:13:46.803535+00:00"},{"alias_kind":"pith_short_12","alias_value":"MJGT3SIOHMDJ","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_16","alias_value":"MJGT3SIOHMDJWXKZ","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_8","alias_value":"MJGT3SIO","created_at":"2026-05-18T12:30:32.724797+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/MJGT3SIOHMDJWXKZFEHER3GXRT","json":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT.json","graph_json":"https://pith.science/api/pith-number/MJGT3SIOHMDJWXKZFEHER3GXRT/graph.json","events_json":"https://pith.science/api/pith-number/MJGT3SIOHMDJWXKZFEHER3GXRT/events.json","paper":"https://pith.science/paper/MJGT3SIO"},"agent_actions":{"view_html":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT","download_json":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT.json","view_paper":"https://pith.science/paper/MJGT3SIO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.06314&json=true","fetch_graph":"https://pith.science/api/pith-number/MJGT3SIOHMDJWXKZFEHER3GXRT/graph.json","fetch_events":"https://pith.science/api/pith-number/MJGT3SIOHMDJWXKZFEHER3GXRT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT/action/storage_attestation","attest_author":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT/action/author_attestation","sign_citation":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT/action/citation_signature","submit_replication":"https://pith.science/pith/MJGT3SIOHMDJWXKZFEHER3GXRT/action/replication_record"}},"created_at":"2026-05-18T01:13:46.803535+00:00","updated_at":"2026-05-18T01:13:46.803535+00:00"}