{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:OSMWNTF4ZW6GTQGXLE5HXJDJB6","short_pith_number":"pith:OSMWNTF4","schema_version":"1.0","canonical_sha256":"749966ccbccdbc69c0d7593a7ba4690fb83c5c88753268d56b4552e02ca47a69","source":{"kind":"arxiv","id":"1706.07655","version":3},"attestation_state":"computed","paper":{"title":"Cosmological models with the energy density of random fluctuations and the Hubble-constant problem","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Kenji Tomita","submitted_at":"2017-06-18T00:54:28Z","abstract_excerpt":"First the fluctuation energy is derived from the adiabatic random fluctuations due to the second-order perturbation theory, and the evolutionary relation for it is expressed in the form of rho_f = rho_f (rho), where rho and rho_f are the densities of ordinary dust and the fluctuation energy, respectively. The pressureless matter as a constituent of the universe at the later stage is assumed to consist of ordinary dust and the fluctuation energy. Next, cosmological models including the fluctuation energy as a kind of dark matter are derived using the above relation, and it is found that the Hub"},"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":"1706.07655","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-06-18T00:54:28Z","cross_cats_sorted":[],"title_canon_sha256":"fb87f70d64172c9b98fc588f77b81a7c470de9b93ce9e0fc42113cba4aa32c6f","abstract_canon_sha256":"1bdd1bbe9b014b9144de830aa7fb58242567c2e5a870b8b4a5b7d415d21460f4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:41.051569Z","signature_b64":"vsTTFQt6p8qOAWsE6wUzR/W/cWO2ubUPNbqGrV45GrSLgpoM6WJ7XAXOdM2FqHqaxrMvsgWVjiWVqsmkjB7FDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"749966ccbccdbc69c0d7593a7ba4690fb83c5c88753268d56b4552e02ca47a69","last_reissued_at":"2026-05-18T00:35:41.050922Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:41.050922Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological models with the energy density of random fluctuations and the Hubble-constant problem","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Kenji Tomita","submitted_at":"2017-06-18T00:54:28Z","abstract_excerpt":"First the fluctuation energy is derived from the adiabatic random fluctuations due to the second-order perturbation theory, and the evolutionary relation for it is expressed in the form of rho_f = rho_f (rho), where rho and rho_f are the densities of ordinary dust and the fluctuation energy, respectively. The pressureless matter as a constituent of the universe at the later stage is assumed to consist of ordinary dust and the fluctuation energy. Next, cosmological models including the fluctuation energy as a kind of dark matter are derived using the above relation, and it is found that the Hub"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.07655","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":""},"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":"1706.07655","created_at":"2026-05-18T00:35:41.051007+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.07655v3","created_at":"2026-05-18T00:35:41.051007+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.07655","created_at":"2026-05-18T00:35:41.051007+00:00"},{"alias_kind":"pith_short_12","alias_value":"OSMWNTF4ZW6G","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"OSMWNTF4ZW6GTQGX","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"OSMWNTF4","created_at":"2026-05-18T12:31:34.259226+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/OSMWNTF4ZW6GTQGXLE5HXJDJB6","json":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6.json","graph_json":"https://pith.science/api/pith-number/OSMWNTF4ZW6GTQGXLE5HXJDJB6/graph.json","events_json":"https://pith.science/api/pith-number/OSMWNTF4ZW6GTQGXLE5HXJDJB6/events.json","paper":"https://pith.science/paper/OSMWNTF4"},"agent_actions":{"view_html":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6","download_json":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6.json","view_paper":"https://pith.science/paper/OSMWNTF4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.07655&json=true","fetch_graph":"https://pith.science/api/pith-number/OSMWNTF4ZW6GTQGXLE5HXJDJB6/graph.json","fetch_events":"https://pith.science/api/pith-number/OSMWNTF4ZW6GTQGXLE5HXJDJB6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6/action/storage_attestation","attest_author":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6/action/author_attestation","sign_citation":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6/action/citation_signature","submit_replication":"https://pith.science/pith/OSMWNTF4ZW6GTQGXLE5HXJDJB6/action/replication_record"}},"created_at":"2026-05-18T00:35:41.051007+00:00","updated_at":"2026-05-18T00:35:41.051007+00:00"}