A constrained cosmological model in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si11.svg" display="inline" id="d1e694"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity
J. K. Singh, Shaily, Ratbay Myrzakulov, Harshna Balhara
Topics & Concepts
PhysicsDark energyDeceleration parameterQuintessenceFriedmann–Lemaître–Robertson–Walker metricHubble's lawUniverseAccelerationAstrophysicsAlgorithmMathematical physicsCosmologyClassical mechanicsComputer scienceCosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsGalaxies: Formation, Evolution, Phenomena