{"paper":{"title":"Exploring physical features of anisotropic strange stars beyond standard maximum mass limit in $f\\left(R,\\mathcal{T}\\right)$ gravity","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Debabrata Deb, Maxim Khlopov, P.H.R.S. Moraes, Saibal Ray, Sergei V. Ketov, S.K. Maurya","submitted_at":"2018-10-17T17:27:50Z","abstract_excerpt":"We study a specific model of anisotropic strange stars in the modified $f\\left(R,\\mathcal{T}\\right)$-type gravity by deriving solutions to the modified Einstein field equations representing a spherically symmetric anisotropic stellar object. We take a standard assumption that $f(R,\\mathcal{T})=R+2\\chi\\mathcal{T}$, where $R$ is Ricci scalar, $\\mathcal{T}$ is the trace of the energy-momentum tensor of matter, and $\\chi$ is a coupling constant. To obtain our solution to the modified Einstein equations, we successfully apply the `embedding class 1' techniques. We also consider the case when the st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.07678","kind":"arxiv","version":3},"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"}