Ushbu ishga iqtibos qilgan ishlar

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Ish: Physical properties of class I compact star model for linear and Starobinsky <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1207" altimg="si25.svg"> <mml:mrow> <mml:mo>−</mml:mo> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> functions

1. A Brief analysis of isotropic Karmarkar models in modified gravity theory

   Yihu Feng, Tayyab Naseer, Asifa Ashraf +2

   MaqolaCosmology and Gravitation TheoriesChinese Journal of Physics20248 iqtibos

   ABIABI:AkademIndex/2024.article.000022

2. 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

   MaqolaOAOchiq kirishCosmology and Gravitation TheoriesJournal of High Energy Astrophysics20254 iqtibos

   ABIABI:AkademIndex/2026.other.109622

3. Constraining <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mi mathvariant="script">L</mml:mi> <mml:mi>m</mml:mi> </mml:msub> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:math> gravity with millisecond pulsar observations

   S.K. Maurya, A. Errehymy, K.N. Singh +4

   MaqolaOAOchiq kirish20261 iqtibos

   ABIABI:AkademIndex/2026.article.041236