{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:AAHNUBXTVPSCNRC65LL466RVEH","short_pith_number":"pith:AAHNUBXT","schema_version":"1.0","canonical_sha256":"000eda06f3abe426c45eead7cf7a3521f7b85cc3e39923c0b8515020ed483484","source":{"kind":"arxiv","id":"1607.06695","version":2},"attestation_state":"computed","paper":{"title":"Investigation of energy conditions in the vicinity of future cosmological singularities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Fatimah Shojai, Mahsa Sanati","submitted_at":"2016-07-21T07:44:29Z","abstract_excerpt":"In this paper, considering the energy conditions we shall show that some of the energy conditions are violated in the vicinity of future singularities with the scale factor suggested by Dabrowski - Marosek."},"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":"1607.06695","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-07-21T07:44:29Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"87c354ff8231aa35bdd65def2b52b20960ad5fce3a59e7ae6d17c94032926018","abstract_canon_sha256":"7e74f0d85556b0945812a7449667934604cdc49e56d2e2989c746b6c331ad7a6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:28.600520Z","signature_b64":"FLO+myXhEn+rOCCgu0wLMXi/pIWkM47xrvhP1caH4ckJQcl+T2T2d+7++KOyhz/WQ0frP9O8eIXtHeqR/LorAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"000eda06f3abe426c45eead7cf7a3521f7b85cc3e39923c0b8515020ed483484","last_reissued_at":"2026-05-18T01:10:28.600108Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:28.600108Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigation of energy conditions in the vicinity of future cosmological singularities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Fatimah Shojai, Mahsa Sanati","submitted_at":"2016-07-21T07:44:29Z","abstract_excerpt":"In this paper, considering the energy conditions we shall show that some of the energy conditions are violated in the vicinity of future singularities with the scale factor suggested by Dabrowski - Marosek."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.06695","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":"1607.06695","created_at":"2026-05-18T01:10:28.600171+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.06695v2","created_at":"2026-05-18T01:10:28.600171+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.06695","created_at":"2026-05-18T01:10:28.600171+00:00"},{"alias_kind":"pith_short_12","alias_value":"AAHNUBXTVPSC","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"AAHNUBXTVPSCNRC6","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"AAHNUBXT","created_at":"2026-05-18T12:30:04.600751+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/AAHNUBXTVPSCNRC65LL466RVEH","json":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH.json","graph_json":"https://pith.science/api/pith-number/AAHNUBXTVPSCNRC65LL466RVEH/graph.json","events_json":"https://pith.science/api/pith-number/AAHNUBXTVPSCNRC65LL466RVEH/events.json","paper":"https://pith.science/paper/AAHNUBXT"},"agent_actions":{"view_html":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH","download_json":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH.json","view_paper":"https://pith.science/paper/AAHNUBXT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.06695&json=true","fetch_graph":"https://pith.science/api/pith-number/AAHNUBXTVPSCNRC65LL466RVEH/graph.json","fetch_events":"https://pith.science/api/pith-number/AAHNUBXTVPSCNRC65LL466RVEH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH/action/storage_attestation","attest_author":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH/action/author_attestation","sign_citation":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH/action/citation_signature","submit_replication":"https://pith.science/pith/AAHNUBXTVPSCNRC65LL466RVEH/action/replication_record"}},"created_at":"2026-05-18T01:10:28.600171+00:00","updated_at":"2026-05-18T01:10:28.600171+00:00"}