{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:PTZS5CKZHTRIFOPXLHH5MNJIUR","short_pith_number":"pith:PTZS5CKZ","schema_version":"1.0","canonical_sha256":"7cf32e89593ce282b9f759cfd63528a47e0ecae792b671a4577ea8cc1f1fa299","source":{"kind":"arxiv","id":"2403.19733","version":2},"attestation_state":"computed","paper":{"title":"Conservative wormholes in generalized $\\kappa(\\mathcal{R},\\mathcal{T})$-function","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Farook Rahaman, G. R. P. Teruel, Ksh. Newton Singh, S. K. Maurya, Tanmoy Chowdhury","submitted_at":"2024-03-28T14:25:38Z","abstract_excerpt":"We present an exhaustive study of wormhole configurations in $\\kappa(\\mathcal{R},\\mathcal{T})$ gravity with linear and non-linear functions. The model assumed Morrison-Thorne spacetime where the redshift and shape functions linked with the matter contain and geometry of the spacetime through non-covariant conservation equation of the stress-energy tensor. The first solution was explored assuming a constant redshift function that leads to a wormhole (WH) which is asymptotically non-flat. The remaining solutions were explored in two cases. Firstly, assuming a linear equation of state $p(r)=\\omeg"},"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":"2403.19733","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-03-28T14:25:38Z","cross_cats_sorted":[],"title_canon_sha256":"2a1b022f16704aec47fb244b960dabca9954dab912b673eb8105e67e5f9fb8b2","abstract_canon_sha256":"d20ac9c7afbe1560544d602d640ff6a12565d419cd41a7f20e7eced38e18e318"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:19:27.619135Z","signature_b64":"j3f9g9LC9w0tuZDcGGX8WKo87PNTSx2LCBFNN/4KaBHzAmomhMC0FW8liUDwirhgvRvyXtrfOkCRX7N9iOcFAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7cf32e89593ce282b9f759cfd63528a47e0ecae792b671a4577ea8cc1f1fa299","last_reissued_at":"2026-07-05T09:19:27.618685Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:19:27.618685Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Conservative wormholes in generalized $\\kappa(\\mathcal{R},\\mathcal{T})$-function","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Farook Rahaman, G. R. P. Teruel, Ksh. Newton Singh, S. K. Maurya, Tanmoy Chowdhury","submitted_at":"2024-03-28T14:25:38Z","abstract_excerpt":"We present an exhaustive study of wormhole configurations in $\\kappa(\\mathcal{R},\\mathcal{T})$ gravity with linear and non-linear functions. The model assumed Morrison-Thorne spacetime where the redshift and shape functions linked with the matter contain and geometry of the spacetime through non-covariant conservation equation of the stress-energy tensor. The first solution was explored assuming a constant redshift function that leads to a wormhole (WH) which is asymptotically non-flat. The remaining solutions were explored in two cases. Firstly, assuming a linear equation of state $p(r)=\\omeg"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.19733","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.19733/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2403.19733","created_at":"2026-07-05T09:19:27.618742+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.19733v2","created_at":"2026-07-05T09:19:27.618742+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.19733","created_at":"2026-07-05T09:19:27.618742+00:00"},{"alias_kind":"pith_short_12","alias_value":"PTZS5CKZHTRI","created_at":"2026-07-05T09:19:27.618742+00:00"},{"alias_kind":"pith_short_16","alias_value":"PTZS5CKZHTRIFOPX","created_at":"2026-07-05T09:19:27.618742+00:00"},{"alias_kind":"pith_short_8","alias_value":"PTZS5CKZ","created_at":"2026-07-05T09:19:27.618742+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.03939","citing_title":"Study of Wormhole in $f(Q)$ gravity with some dark energy models","ref_index":19,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR","json":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR.json","graph_json":"https://pith.science/api/pith-number/PTZS5CKZHTRIFOPXLHH5MNJIUR/graph.json","events_json":"https://pith.science/api/pith-number/PTZS5CKZHTRIFOPXLHH5MNJIUR/events.json","paper":"https://pith.science/paper/PTZS5CKZ"},"agent_actions":{"view_html":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR","download_json":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR.json","view_paper":"https://pith.science/paper/PTZS5CKZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.19733&json=true","fetch_graph":"https://pith.science/api/pith-number/PTZS5CKZHTRIFOPXLHH5MNJIUR/graph.json","fetch_events":"https://pith.science/api/pith-number/PTZS5CKZHTRIFOPXLHH5MNJIUR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR/action/storage_attestation","attest_author":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR/action/author_attestation","sign_citation":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR/action/citation_signature","submit_replication":"https://pith.science/pith/PTZS5CKZHTRIFOPXLHH5MNJIUR/action/replication_record"}},"created_at":"2026-07-05T09:19:27.618742+00:00","updated_at":"2026-07-05T09:19:27.618742+00:00"}