Influence of minimal gravitational decoupling and pseudo isothermal dark matter halo on mass-radius relation and stability of anisotropic compact stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"> <mml:mi>f</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo stretchy="false">)</mml:mo> </mml:math> –gravity

S. K. Maurya, Abdelghani Errehymy, Baiju Dayanandan, Orhan Dönmez, Kairat Myrzakulov, Kottakkaran Sooppy Nisar, Mona Mahmoud