- #1
fab13
- 320
- 7
- TL;DR Summary
- I get below the following contours of a MCMC run with the main cosmological parameters for Brans-Dickce's theory without introducing a cosmological constant (##\Lambda=0##) and considering only baryonic matter component.
Could you justify the anticorrelation that I get between ##H_0## and ##\omega_{BD}## (actually ##\log10(\omega_{BD}##) ?
If we take the relation :
##\Omega_{B D}=\frac{\omega_{B D}}{6}\left(\frac{F_0}{H_0}\right)^2-\frac{F_0}{H_0} ##, then I can express ##H_0## as a function of ##\omega_{BD}## :
##H_0=\frac{-F_0+\sqrt{F_0^2+\frac{2 \Omega_{B D \omega_{B D} F_0^2}}{3}}}{2 \Omega_{B D}} .##
From this relation, we are expected to have a correlation instead of an anti-correlation since if ##\omega_{BD}## increases, then, ##H_0## will increase.
If someone could help me to justify my result (if it is true), this would be great.