{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:HXZOIESXU25G4F2TF2ANFA5TJV","short_pith_number":"pith:HXZOIESX","schema_version":"1.0","canonical_sha256":"3df2e41257a6ba6e17532e80d283b34d65652edf2f8eb2703de62ae06ba95e8d","source":{"kind":"arxiv","id":"1106.2450","version":1},"attestation_state":"computed","paper":{"title":"Vacuum polarization in a cosmic string spacetime induced by flat boundary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Aram A. Saharian, Eug\\^enio R. Bezerra de Mello","submitted_at":"2011-06-13T14:27:50Z","abstract_excerpt":"In this paper we analyze the vacuum expectation values of the field squared and the energy-momentum tensor associated to a massive scalar field in a higher dimensional cosmic string spacetime, obeying Dirichlet or Neumann boundary conditions on the surface orthogonal to the string."},"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":"1106.2450","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2011-06-13T14:27:50Z","cross_cats_sorted":[],"title_canon_sha256":"72eb704134306ddf4eb97a35efed4f05f89856f7b60fc79972db274cef0ebe8c","abstract_canon_sha256":"7e74a0e03de771643f6c77b3776ad9bd6bc95d1056e4b0214e9477d3295dbe3c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:08:12.413515Z","signature_b64":"bmQBVLoctGOGVR3Bvmcq+dFrRYJIZifrFqbEnHH8XcIRof7pzzAwzhRSEI13t89SZk42JX4/CNSPi7aIKBLyDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3df2e41257a6ba6e17532e80d283b34d65652edf2f8eb2703de62ae06ba95e8d","last_reissued_at":"2026-05-18T04:08:12.413013Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:08:12.413013Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Vacuum polarization in a cosmic string spacetime induced by flat boundary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Aram A. Saharian, Eug\\^enio R. Bezerra de Mello","submitted_at":"2011-06-13T14:27:50Z","abstract_excerpt":"In this paper we analyze the vacuum expectation values of the field squared and the energy-momentum tensor associated to a massive scalar field in a higher dimensional cosmic string spacetime, obeying Dirichlet or Neumann boundary conditions on the surface orthogonal to the string."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.2450","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":"1106.2450","created_at":"2026-05-18T04:08:12.413093+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.2450v1","created_at":"2026-05-18T04:08:12.413093+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.2450","created_at":"2026-05-18T04:08:12.413093+00:00"},{"alias_kind":"pith_short_12","alias_value":"HXZOIESXU25G","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"HXZOIESXU25G4F2T","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"HXZOIESX","created_at":"2026-05-18T12:26:30.835961+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/HXZOIESXU25G4F2TF2ANFA5TJV","json":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV.json","graph_json":"https://pith.science/api/pith-number/HXZOIESXU25G4F2TF2ANFA5TJV/graph.json","events_json":"https://pith.science/api/pith-number/HXZOIESXU25G4F2TF2ANFA5TJV/events.json","paper":"https://pith.science/paper/HXZOIESX"},"agent_actions":{"view_html":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV","download_json":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV.json","view_paper":"https://pith.science/paper/HXZOIESX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.2450&json=true","fetch_graph":"https://pith.science/api/pith-number/HXZOIESXU25G4F2TF2ANFA5TJV/graph.json","fetch_events":"https://pith.science/api/pith-number/HXZOIESXU25G4F2TF2ANFA5TJV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV/action/storage_attestation","attest_author":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV/action/author_attestation","sign_citation":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV/action/citation_signature","submit_replication":"https://pith.science/pith/HXZOIESXU25G4F2TF2ANFA5TJV/action/replication_record"}},"created_at":"2026-05-18T04:08:12.413093+00:00","updated_at":"2026-05-18T04:08:12.413093+00:00"}