{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:AMN5NYD3FD7TO2NW736LISAARQ","short_pith_number":"pith:AMN5NYD3","schema_version":"1.0","canonical_sha256":"031bd6e07b28ff3769b6fefcb448008c3e748c1c3dbd04ee5b6bc888f086fcbb","source":{"kind":"arxiv","id":"1709.04055","version":2},"attestation_state":"computed","paper":{"title":"Bouncing universe of entropy-corrected Friedmann equations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Amin.Salehi, Mojtaba.Mahmoudi fard","submitted_at":"2017-09-12T20:47:11Z","abstract_excerpt":"The investigation of quantum gravity effects in order to avoid the big bang singularity is a requisite, so that the idea of oscillating universes is introduced as an alternative for standard cosmological model. Therefore, the Friedmann equations arising from the quantum corrections of entropy-area relation provide the possibility of studying the oscillating universes. Addition to necessity of surveying the bouncing solutions, however, the values of unknown constant parameters are still a matter of open debate. In this paper, we consider modified Friedmann equations with logarithmic entropy cor"},"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":"1709.04055","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-09-12T20:47:11Z","cross_cats_sorted":[],"title_canon_sha256":"b33744e26878690a4c133c65d12ac80cb757681397fa8284da405dbfd1f76286","abstract_canon_sha256":"49bc787bd482be30f20527a8328dcff71f8eadcd3edac29d455e7a75817a5423"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:18:19.417731Z","signature_b64":"mq01HTQDRXqIoaNhpsyOhklJjnn6Y88XEqFkLRTmNNDAnNvx96y/gnXFGmjaTLau6V14iR28kvj6nXMv603dAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"031bd6e07b28ff3769b6fefcb448008c3e748c1c3dbd04ee5b6bc888f086fcbb","last_reissued_at":"2026-05-18T00:18:19.417057Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:18:19.417057Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bouncing universe of entropy-corrected Friedmann equations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Amin.Salehi, Mojtaba.Mahmoudi fard","submitted_at":"2017-09-12T20:47:11Z","abstract_excerpt":"The investigation of quantum gravity effects in order to avoid the big bang singularity is a requisite, so that the idea of oscillating universes is introduced as an alternative for standard cosmological model. Therefore, the Friedmann equations arising from the quantum corrections of entropy-area relation provide the possibility of studying the oscillating universes. Addition to necessity of surveying the bouncing solutions, however, the values of unknown constant parameters are still a matter of open debate. In this paper, we consider modified Friedmann equations with logarithmic entropy cor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.04055","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":"1709.04055","created_at":"2026-05-18T00:18:19.417145+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.04055v2","created_at":"2026-05-18T00:18:19.417145+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.04055","created_at":"2026-05-18T00:18:19.417145+00:00"},{"alias_kind":"pith_short_12","alias_value":"AMN5NYD3FD7T","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"AMN5NYD3FD7TO2NW","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"AMN5NYD3","created_at":"2026-05-18T12:31:05.417338+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.10495","citing_title":"The generalized second law as a thermodynamic selection criterion for dynamical dark energy","ref_index":51,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ","json":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ.json","graph_json":"https://pith.science/api/pith-number/AMN5NYD3FD7TO2NW736LISAARQ/graph.json","events_json":"https://pith.science/api/pith-number/AMN5NYD3FD7TO2NW736LISAARQ/events.json","paper":"https://pith.science/paper/AMN5NYD3"},"agent_actions":{"view_html":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ","download_json":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ.json","view_paper":"https://pith.science/paper/AMN5NYD3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.04055&json=true","fetch_graph":"https://pith.science/api/pith-number/AMN5NYD3FD7TO2NW736LISAARQ/graph.json","fetch_events":"https://pith.science/api/pith-number/AMN5NYD3FD7TO2NW736LISAARQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ/action/storage_attestation","attest_author":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ/action/author_attestation","sign_citation":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ/action/citation_signature","submit_replication":"https://pith.science/pith/AMN5NYD3FD7TO2NW736LISAARQ/action/replication_record"}},"created_at":"2026-05-18T00:18:19.417145+00:00","updated_at":"2026-05-18T00:18:19.417145+00:00"}