Constrained <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si21.svg" display="inline" id="d1e1764"><mml:mi>Λ</mml:mi></mml:math>CDM dark energy models in higher derivative <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si401.svg" display="inline" id="d1e1769"><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 theory
Dinesh Chandra Maurya
Topics & Concepts
Dark energyPhysicsHubble's lawEquation of stateDeceleration parameterUniverseCosmological constantMathematical physicsParticle physicsCosmologyAstrophysicsQuantum mechanicsCosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaBlack Holes and Theoretical Physics