{"id":"fe3ce344-ad2a-4bc7-b98f-1e01be20409c","arxiv_id":"2504.20060","paper_version":1,"verdict":"CONDITIONAL","confidence":"MODERATE","novelty_score":4.0,"correctness_risk":"medium","formal_verification":"none","parameter_count":1,"one_line_summary":"The interior black hole spacetime satisfies a family of pseudosymmetry-type curvature identities and admits generalized curvature inheritance for a specific non-Killing vector field.","lead":"This paper computes curvature identities for the interior Schwarzschild black hole metric, showing that certain curvature operators are linearly dependent. It also maps the inheritance symmetries of that metric with respect to a chosen non-Killing vector field.","discovery_kind":"extension","skeptic_critique":null,"referee_report":null,"author_rebuttal":null,"desk_editor":null,"rs_alignment":null,"lean_confirmation":null,"pith_extraction":null,"created_at":"2026-08-16T12:41:29.249234+00:00","model_set":{"reader":"deepseek-v4-flash"},"falsifier":null,"supporting_citations":[],"review_version":1}