{"paper":{"title":"Geodesics Structure and Thermodynamic Properties of Gaussian Black Hole in Quadratic Ricci Scaler Gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"Gaussian black holes show larger thermodynamic differences than geodesic ones between quadratic Ricci scalar gravity and Einstein gravity.","cross_cats":["astro-ph.GA"],"primary_cat":"gr-qc","authors_text":"B. Malekolkalami, M. Haditale","submitted_at":"2026-05-13T11:34:23Z","abstract_excerpt":"The geodesic structure and thermal properties of Gaussian Black Holes (\\textbf{GBH})s in modified and Einstein gravities are studied and compared. In the geodesic part, motion of a test particle (massive and massless) are discussed, specially properties of the circular motion are considered. In the thermodynamic part, the mass, entropy and temperature functions are considered and discussed. The local and global stability is also analyzed through the Heat Capacity (\\textbf{HC}) and Gibbs Energy (\\textbf{GE}). The results show the thermodynamic differences are more than geodesic ones in the two "},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"The results show the thermodynamic differences are more than geodesic ones in the two theories of gravity with the note that the modified gravity is more consistent with the physical world.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The Gaussian black hole metric remains a valid exact solution in quadratic Ricci scalar gravity and that standard thermodynamic and geodesic calculations apply without additional constraints or higher-order corrections.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"Gaussian black holes show larger thermodynamic differences than geodesic differences when studied in quadratic Ricci scalar gravity compared to Einstein gravity, with the modified theory favored for physical consistency.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"Gaussian black holes show larger thermodynamic differences than geodesic ones between quadratic Ricci scalar gravity and Einstein gravity.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"f7b875b4955926c53bd06a77017b06401838f9d9a93ddfc8207ec3f4981a93b2"},"source":{"id":"2605.13377","kind":"arxiv","version":1},"verdict":{"id":"1af03cf8-cd51-4f86-a0ed-b5ae1bda8ea2","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-14T18:38:46.021825Z","strongest_claim":"The results show the thermodynamic differences are more than geodesic ones in the two theories of gravity with the note that the modified gravity is more consistent with the physical world.","one_line_summary":"Gaussian black holes show larger thermodynamic differences than geodesic differences when studied in quadratic Ricci scalar gravity compared to Einstein gravity, with the modified theory favored for physical consistency.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The Gaussian black hole metric remains a valid exact solution in quadratic Ricci scalar gravity and that standard thermodynamic and geodesic calculations apply without additional constraints or higher-order corrections.","pith_extraction_headline":"Gaussian black holes show larger thermodynamic differences than geodesic ones between quadratic Ricci scalar gravity and Einstein gravity."},"references":{"count":34,"sample":[{"doi":"","year":2014,"title":"C. M. Will,Living Rev. Relativ.17, 4 (2014). 13","work_id":"80ea8e8c-b376-4e78-bb0f-e623700636f5","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2008,"title":"M. Kowalski, et al.,Astrophys. J.686, 2 (2008)","work_id":"5cb6902f-5d56-4c17-8a6d-3a575f1a9e3a","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2014,"title":"Z. Hou, C. Reichardt, K. Story, B. Follin, R. Keisler, et al.,Astrophys. J.782, 74 (2014)","work_id":"ae50aad6-1255-44a6-bc4c-b02fbe811e5a","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2013,"title":"J.L. Sievers, et al.,J. Cosmol. Astropart. Phys.1310, 060 (2013)","work_id":"a917a4da-e4a9-44b9-b737-1c5c31316fc6","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2013,"title":"K.T. Story, et al.,Ap. J.779, 86 (2013)","work_id":"39722ef0-4e18-4f6f-aedb-8cd7ccc7dc38","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":34,"snapshot_sha256":"87f2a750deb21da691629bf2da6fb9d48ee302ebfb35b6b83247fbc1de249e74","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"}