Litcius/Paper detail

Energy condition bounds on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e7460" altimg="si6.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> model parameters in a curved FLRW Universe

Ganesh Subramaniam, Avik De, Tee‐How Loo, Yong Kheng Goh

2023Physics of the Dark Universe26 citationsDOI

Topics & Concepts

Friedmann–Lemaître–Robertson–Walker metricPhysicsDeceleration parameterHubble's lawUniverseAccelerationEnergy (signal processing)Range (aeronautics)Dark energyScalable Vector GraphicsMathematical physicsCosmologyAstrophysicsClassical mechanicsQuantum mechanicsComputer scienceAerospace engineeringOperating systemEngineeringCosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsGalaxies: Formation, Evolution, Phenomena
Energy condition bounds on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e7460" altimg="si6.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> model parameters in a curved FLRW Universe | Litcius