- #1
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- Homework Statement
- We have a flat Universe with a positive Λ, density matter ρ[SUB]m[/SUB]. Need to prove the formula for a[SUP]3[/SUP](t) below from the first Friedmann equation and changing the variable from the u=(...) given below
- Relevant Equations
- - Friedmann's first equation; H[SUP]2[/SUP]= 8πGρ[SUB]total[/SUB]/3 - k/a[SUP]2[/SUP]
- New variable; u=2Λa[SUP]3[/SUP]/ρ[SUB]o[/SUB]
We need to prove that a3(t)= ρo/2Λ [cosh(sqrt(24πGΛ)*t) -1] by changing into a variable of u, where
u=2Λa3/ρo
From Friedmann's second equation we know that Λ= ρm/ 2
Also ρm= ρo/ a3
[First attempt]
I begin from Friedmann's equation where (for here), ρtotal= ρm + Λ and k=0;
a'2/a2 = 8πG(ρm + Λ)/3 , (a'=da/dt)
⇒ a'/a = sqrt ((8πG/3) * (3ρo/2a3) )
⇒∫ da/a = ∫sqrt((8πG/3) * (3ρo/2a3))dt
⇒ lna = sqrt((8πG) * (ρo/2a3)) t
⇒ a= exp [sqrt((8πG) * (ρo/2a3))t ]
which is not close with what we're trying to prove, and I didn't use the variable u I was supposed to. The solution is the correct for a flat universe, but when we're looking for the a(t). Seems like I have to change the a into u completely inside friedmann's equation.
So I tried this too; (second attempt)
a'2/a2 = 8πG(ρm + Λ)/3
⇒ a'/a = sqrt ((8πG/3) * (3ρo/2a3)) = sqrt(4πGρo/a3) ⇒
⇒ da/dt = a*sqrt(4πGρo/a3) = sqrt(a24πGρo/a3)=
= sqrt(4πGρo/a) (a)
and now changing the variable from a to u;
u=2Λa3/ρo ⇒ a3 = uρo/2Λ ⇒
a= [uρo/2Λ] 3/2 (1)
So,
da= (ρo/2Λ) 3/2 u1/2du (2)
(a),(1),(2) → ... du/u1/2= sqrt(8πGΛ)dt = sqrt(8πGΛ)t
Where the cosh() is still missing...
In the first attempt I had the exact same problem too. The first integral was always da/sqrt(a) that doesn't give a cosh for a solution
u=2Λa3/ρo
From Friedmann's second equation we know that Λ= ρm/ 2
Also ρm= ρo/ a3
[First attempt]
I begin from Friedmann's equation where (for here), ρtotal= ρm + Λ and k=0;
a'2/a2 = 8πG(ρm + Λ)/3 , (a'=da/dt)
⇒ a'/a = sqrt ((8πG/3) * (3ρo/2a3) )
⇒∫ da/a = ∫sqrt((8πG/3) * (3ρo/2a3))dt
⇒ lna = sqrt((8πG) * (ρo/2a3)) t
⇒ a= exp [sqrt((8πG) * (ρo/2a3))t ]
which is not close with what we're trying to prove, and I didn't use the variable u I was supposed to. The solution is the correct for a flat universe, but when we're looking for the a(t). Seems like I have to change the a into u completely inside friedmann's equation.
So I tried this too; (second attempt)
a'2/a2 = 8πG(ρm + Λ)/3
⇒ a'/a = sqrt ((8πG/3) * (3ρo/2a3)) = sqrt(4πGρo/a3) ⇒
⇒ da/dt = a*sqrt(4πGρo/a3) = sqrt(a24πGρo/a3)=
= sqrt(4πGρo/a) (a)
and now changing the variable from a to u;
u=2Λa3/ρo ⇒ a3 = uρo/2Λ ⇒
a= [uρo/2Λ] 3/2 (1)
So,
da= (ρo/2Λ) 3/2 u1/2du (2)
(a),(1),(2) → ... du/u1/2= sqrt(8πGΛ)dt = sqrt(8πGΛ)t
Where the cosh() is still missing...
In the first attempt I had the exact same problem too. The first integral was always da/sqrt(a) that doesn't give a cosh for a solution