{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:5VNKA3VKR3G5KB72EM24OWTMZ6","short_pith_number":"pith:5VNKA3VK","schema_version":"1.0","canonical_sha256":"ed5aa06eaa8ecdd507fa2335c75a6ccfa24cf397a4f8c5b8576f17e941365e61","source":{"kind":"arxiv","id":"1704.01860","version":3},"attestation_state":"computed","paper":{"title":"Scalar Casimir effect in a high-dimensional cosmic dispiration spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"E. R. Bezerra de Mello, H. F. Mota, K. Bakke","submitted_at":"2017-04-06T14:32:19Z","abstract_excerpt":"In this paper we present a complete and detailed analysis of the calculation of both the Wightman function and the vacuum expectation value of the energy-momentum tensor that arise from quantum vacuum fluctuations of massive and massless scalar fields in the cosmic dispiration spacetime, which is formed by the combination of two topological defects: a cosmic string and a screw dislocation. This spacetime is obtained in the framework of the Einstein-Cartan theory of gravity and is considered to be a chiral space-like cosmic string. For completeness we perform the calculation in a high-dimension"},"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":"1704.01860","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-04-06T14:32:19Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"f166e425950b6057484607d688690894161371e2f08d2118f5b17af17f763be6","abstract_canon_sha256":"0d2f329dcd98ef452ac7e18bb9ef335601de8471049fec6c140c1788fb4ee9cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:06:06.330427Z","signature_b64":"df9id5V6DX1VaQl0YS6PycspMuD2Vhu829ZS1Ew0fWZXBzMpZS5AZYv1RF6BrrjayIJOTwtiJGvBRrLBOWx+BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ed5aa06eaa8ecdd507fa2335c75a6ccfa24cf397a4f8c5b8576f17e941365e61","last_reissued_at":"2026-05-18T00:06:06.329796Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:06:06.329796Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scalar Casimir effect in a high-dimensional cosmic dispiration spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"E. R. Bezerra de Mello, H. F. Mota, K. Bakke","submitted_at":"2017-04-06T14:32:19Z","abstract_excerpt":"In this paper we present a complete and detailed analysis of the calculation of both the Wightman function and the vacuum expectation value of the energy-momentum tensor that arise from quantum vacuum fluctuations of massive and massless scalar fields in the cosmic dispiration spacetime, which is formed by the combination of two topological defects: a cosmic string and a screw dislocation. This spacetime is obtained in the framework of the Einstein-Cartan theory of gravity and is considered to be a chiral space-like cosmic string. For completeness we perform the calculation in a high-dimension"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.01860","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":"1704.01860","created_at":"2026-05-18T00:06:06.329898+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.01860v3","created_at":"2026-05-18T00:06:06.329898+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.01860","created_at":"2026-05-18T00:06:06.329898+00:00"},{"alias_kind":"pith_short_12","alias_value":"5VNKA3VKR3G5","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_16","alias_value":"5VNKA3VKR3G5KB72","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_8","alias_value":"5VNKA3VK","created_at":"2026-05-18T12:31:00.734936+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.07648","citing_title":"Vacuum-induced current density from a magnetic flux threading a cosmic dispiration in $(D+1)$-dimensional spacetime","ref_index":10,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6","json":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6.json","graph_json":"https://pith.science/api/pith-number/5VNKA3VKR3G5KB72EM24OWTMZ6/graph.json","events_json":"https://pith.science/api/pith-number/5VNKA3VKR3G5KB72EM24OWTMZ6/events.json","paper":"https://pith.science/paper/5VNKA3VK"},"agent_actions":{"view_html":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6","download_json":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6.json","view_paper":"https://pith.science/paper/5VNKA3VK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.01860&json=true","fetch_graph":"https://pith.science/api/pith-number/5VNKA3VKR3G5KB72EM24OWTMZ6/graph.json","fetch_events":"https://pith.science/api/pith-number/5VNKA3VKR3G5KB72EM24OWTMZ6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6/action/storage_attestation","attest_author":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6/action/author_attestation","sign_citation":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6/action/citation_signature","submit_replication":"https://pith.science/pith/5VNKA3VKR3G5KB72EM24OWTMZ6/action/replication_record"}},"created_at":"2026-05-18T00:06:06.329898+00:00","updated_at":"2026-05-18T00:06:06.329898+00:00"}