{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:XF3MBK2KCGLNSJ7H6HEWX5KPT4","short_pith_number":"pith:XF3MBK2K","schema_version":"1.0","canonical_sha256":"b976c0ab4a1196d927e7f1c96bf54f9f0d88d497f1331a19b38ee219415f6ebf","source":{"kind":"arxiv","id":"1801.01409","version":2},"attestation_state":"computed","paper":{"title":"Anisotropic strange stars under simplest minimal matter-geometry coupling in the $f(R,\\mathcal{T})$ gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"B.K. Guha, Debabrata Deb, Farook Rahaman, Saibal Ray","submitted_at":"2017-12-30T15:08:47Z","abstract_excerpt":"We study strange stars in the framework of $f\\left(R,\\mathcal{T}\\right)$ theory of gravity where the strange quark matter distribution inside the stellar system is governed by the phenomenological MIT Bag model equation of state (EOS). Further, for a specific value of $B$ and observed values of mass of the strange star candidates we obtain the exact solution of the modified Tolman-Oppenheimer-Volkoff (TOV) equation in the framework of $f\\left(R,\\mathcal{T}\\right)$ gravity and have studied in detail the dependence of the different physical parameters due to the chosen different values of $\\chi$"},"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":"1801.01409","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.gen-ph","submitted_at":"2017-12-30T15:08:47Z","cross_cats_sorted":[],"title_canon_sha256":"1ec2ee9b7d1dbe98c8261e7572a0ea2c453a5127a959461d72c9e7629cf7b937","abstract_canon_sha256":"1d29076c5c99f62323dfad1680acbc48e6d2579d243027da61da90617768191e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:17:53.732714Z","signature_b64":"i2cUR4jqI//z4gcegxgiG8ivjpMyI9gFSox2j3ZVVcV+nmqvrpUPxbNzl+j8O3UrBH6P07mrgubNN12wrBFqAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b976c0ab4a1196d927e7f1c96bf54f9f0d88d497f1331a19b38ee219415f6ebf","last_reissued_at":"2026-05-18T00:17:53.732144Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:17:53.732144Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Anisotropic strange stars under simplest minimal matter-geometry coupling in the $f(R,\\mathcal{T})$ gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"B.K. Guha, Debabrata Deb, Farook Rahaman, Saibal Ray","submitted_at":"2017-12-30T15:08:47Z","abstract_excerpt":"We study strange stars in the framework of $f\\left(R,\\mathcal{T}\\right)$ theory of gravity where the strange quark matter distribution inside the stellar system is governed by the phenomenological MIT Bag model equation of state (EOS). Further, for a specific value of $B$ and observed values of mass of the strange star candidates we obtain the exact solution of the modified Tolman-Oppenheimer-Volkoff (TOV) equation in the framework of $f\\left(R,\\mathcal{T}\\right)$ gravity and have studied in detail the dependence of the different physical parameters due to the chosen different values of $\\chi$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.01409","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":"1801.01409","created_at":"2026-05-18T00:17:53.732228+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.01409v2","created_at":"2026-05-18T00:17:53.732228+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.01409","created_at":"2026-05-18T00:17:53.732228+00:00"},{"alias_kind":"pith_short_12","alias_value":"XF3MBK2KCGLN","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_16","alias_value":"XF3MBK2KCGLNSJ7H","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_8","alias_value":"XF3MBK2K","created_at":"2026-05-18T12:31:53.515858+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/XF3MBK2KCGLNSJ7H6HEWX5KPT4","json":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4.json","graph_json":"https://pith.science/api/pith-number/XF3MBK2KCGLNSJ7H6HEWX5KPT4/graph.json","events_json":"https://pith.science/api/pith-number/XF3MBK2KCGLNSJ7H6HEWX5KPT4/events.json","paper":"https://pith.science/paper/XF3MBK2K"},"agent_actions":{"view_html":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4","download_json":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4.json","view_paper":"https://pith.science/paper/XF3MBK2K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.01409&json=true","fetch_graph":"https://pith.science/api/pith-number/XF3MBK2KCGLNSJ7H6HEWX5KPT4/graph.json","fetch_events":"https://pith.science/api/pith-number/XF3MBK2KCGLNSJ7H6HEWX5KPT4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4/action/storage_attestation","attest_author":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4/action/author_attestation","sign_citation":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4/action/citation_signature","submit_replication":"https://pith.science/pith/XF3MBK2KCGLNSJ7H6HEWX5KPT4/action/replication_record"}},"created_at":"2026-05-18T00:17:53.732228+00:00","updated_at":"2026-05-18T00:17:53.732228+00:00"}