- #1
Tom Weaver
- 5
- 0
Given the metric of the gravitational field of a central gravitational body:
ds2 = -ev(r)dt2 + eμ(r)dr2 + r2 (dθ2 + sin2θdΦ2)
And the Chritofell connection components:
Find the Riemannian curvature tensor component R0110 (which is non-zero).
I believe the answer uses the Ricci tensor:
Rμv = Rλμvλ = Γλμλ,v - Γλμv,λ + ΓρμλΓλvρ - ΓλμvΓρλρ
This is far as I've got:
R0110 = Γ010,1 - Γ011,0 + Γρ10Γ01ρ - Γ011Γρ0ρ
R0110 = 0.5v'' + Γρ10Γ01ρ - Γ011Γρ0ρ
I'm not entirely sure on the meaning of ρ, at first I thought it would cycle through 0, 1, 2 and 3 to represent the 4 dimensions but after working that through I found it didn't work. Any help is much appreciated!
ds2 = -ev(r)dt2 + eμ(r)dr2 + r2 (dθ2 + sin2θdΦ2)
And the Chritofell connection components:
Find the Riemannian curvature tensor component R0110 (which is non-zero).
I believe the answer uses the Ricci tensor:
Rμv = Rλμvλ = Γλμλ,v - Γλμv,λ + ΓρμλΓλvρ - ΓλμvΓρλρ
This is far as I've got:
R0110 = Γ010,1 - Γ011,0 + Γρ10Γ01ρ - Γ011Γρ0ρ
R0110 = 0.5v'' + Γρ10Γ01ρ - Γ011Γρ0ρ
I'm not entirely sure on the meaning of ρ, at first I thought it would cycle through 0, 1, 2 and 3 to represent the 4 dimensions but after working that through I found it didn't work. Any help is much appreciated!