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Ish: Charged stellar structure with Krori–Barua potentials in f(R,ϕ,X) gravity admitting Chaplygin equation of state

1. Implication of f(Q,T) gravity on the formation of the charge compact stars and constraining their mass-radius relations in lower mass gap region

   S. K. Maurya, Abdelghani Errehymy, Zhanbala Umbetova +4

   MaqolaCosmology and Gravitation TheoriesJournal of High Energy Astrophysics20254 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.109622

2. Testing linear non-minimal coupling in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si447.svg" display="inline" id="d1e4384"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>,</mml:mo> <mml:mi>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity using X-ray binary pulsars constrained by NICER observations

   Abdelghani Errehymy, S. K. Maurya, Orhan Dönmez +4

   MaqolaPulsars and Gravitational Waves ResearchPhysics of the Dark Universe20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.001332