Litcius/Paper detail

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

Ksh. Newton Singh, S. K. Maurya, Abdelghani Errehymy, Farook Rahaman, M. Daoud

2020Physics of the Dark Universe41 citationsDOI

Topics & Concepts

PhysicsMathematical physicsCurvatureScalar (mathematics)GeometryMathematicsCosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsGalaxies: Formation, Evolution, Phenomena
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 | Litcius