Arman777
Gold Member
- 2,163
- 191
Vishal Rana said:How do u know this? I thought it was accelerating cause of dark energy?
Well Expansion rate can be defined as ##H(t)## where ##H(t)=\frac {\dot {a}(t)} {a(t)}##. Now we can write the Friedmann Equation in the form of,
##\frac {H^2} {(H_0)^2}=Ω_ma^{-3}+Ω_Λ## and Now in here ##H## is Hubble parameter at any time t. ##H_0## Hubble parameter now. ##Ω_m## matter density
##Ω_Λ## dark energy density and ##a## is the value of the scale factor at that time respeect to the ##a(t_0)=1##.
Note: ##Ω_m## and ##Ω_Λ## should be current (Now) values
Now we can re-write the equation as,
##H^2={(H_0)^2}[Ω_ma^{-3}+Ω_Λ]##
take square root and we get,
##H=H_0\sqrt{Ω_ma^{-3}+Ω_Λ}##
Since, ##H_0##, ##Ω_m## and ##Ω_Λ## are constant numbers, we can simply think this equation like this,
##H=\sqrt{x^{-3}}##
and I graphed it in desmos and I get,
As PeterDonis Said ##\ddot {a}(t)## is icreasing but it doesn't mean ##H(t)## is also increasing.