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Luminosity Distance
Linked via "cosmological model parameters"
The Role of Cosmological Models
The mathematical expression for $DL$ depends explicitly on the cosmological model parameters, specifically the density parameters for matter ($\Omegam$)) and dark energy ($\Omega\Lambda$)), and the Hubble constant ($H0$)).
For a general Friedmann–Lemaître–Robertson–Walker (FLRW) metric-metric), the luminosity dista…