Christoffel symbol from Variational Principle

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Homework Help Overview

The discussion revolves around the calculation of Christoffel symbols using the variational principle in the context of a weak gravitational field. The original poster presents a metric and attempts to derive the symbols but encounters difficulties, particularly resulting in zero values.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants explore the implications of treating the gravitational potential as constant versus variable. There are attempts to differentiate the potential and apply the Euler-Lagrange equation, with some participants expressing confusion about index notation and the application of the chain rule.

Discussion Status

There is an ongoing exploration of the calculations involved in deriving the Christoffel symbols. Some participants have provided insights into the differentiation process and the use of index notation, while others are questioning the assumptions made regarding the gravitational potential and its dependence on spatial coordinates.

Contextual Notes

Participants note the complexity of differentiating the gravitational potential, which is a function of spatial coordinates, and the challenges posed by the notation used in the calculations. There is also mention of the need for careful handling of indices in tensor calculations.

psimeson
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Homework Statement



It's not exactly a homework question. I can find Christoffel Symbols using general definition of Christoffel symbol. But, when I try to find Christoffel Symbols using variational principle, I end up getting zero.

I have started with the space-time metric in a weak gravitational field (with the assumption of low velocity):
ds2=−(1+2ϕ)dt2+(1−2ϕ)(dx2+dy2+dz2)

Where
ϕ<<1 is the gravitational potential.

Homework Equations



Euler Lagrange(EL) Equation: [itex]\frac{d}{d\tau}[/itex]([itex]\frac{dL}{d\dot{x^{a}}}[/itex]) = [itex]\frac{dL}{dx}[/itex]


The Attempt at a Solution


Lagrangian:
L = −(1+2ϕ)[itex]\dot{t}[/itex]2+(1−2ϕ)([itex]\dot{x}[/itex]2+[itex]\dot{y}[/itex]2+[itex]\dot{z}[/itex]2)

using EL:[itex]\frac{d}{d\tau}[/itex]([itex]\frac{dL}{d\dot{t}}[/itex]) = [itex]\frac{dL}{dx}[/itex]


−(1+2ϕ)[itex]\ddot{t}[/itex]= 0

I repeated the similar process for x, y, and z and I got zero for all. Can someone please help me?

Answer should be:

Γtti=ϕ,i

Γi00=ϕ,iijk=δjkϕ,i−δijϕ,k−δikϕ,j
 
Last edited:
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You are taking phi to be constant in your calculation. The Christoffel symbols are indeed zero if phi is constant, but not if it's not.
 
I know that phi is function of r and I am having hard time to differentiate it. I just got stuck. Since r = sqrt (x^2 + y^2+ z^2) . How can it depend on t. The way it can depend on t by using the definition of proper time. Sorry, I am just lost.
 
Last edited:
So you just use chain rule:

[itex]\frac{d}{d\tau} \frac{\partial L}{\partial \dot{x}_i} = 2\frac{d}{d\tau} [(1+2\phi) \dot{x}_i] = 2((1+2\phi)\ddot{x}_i + 2\dot{x}_i \phi_{,\mu} \dot{x}^{\mu})[/itex]

and as usual,

[itex]\frac{\partial L}{\partial x_i}= 2 \phi_{,i} ( \dot{t}^2 +\dot{x}_j \dot{x}^j)[/itex]

Note that I can be careless with my index notation here, because the errors I'm making would be proportional to phi squared, which I can drop in first order perturbation theory. You should probably be more careful though, it's very easy to make stupid mistakes with this kind of calculations
 
I didn't get how you get [itex]{\mu}[/itex]...why are you using lower index [itex]\dot{x}_i[/itex]


[itex]\frac{d}{d\tau} \frac{\partial L}{\partial \dot{x}_i} = 2\frac{d}{d\tau} [(1+2\phi) \dot{x}_i] = 2((1+2\phi)\ddot{x}_i + 2\dot{x}_i \phi_{,\mu} \dot{x}^{\mu})[/itex]


What is [itex]\dot{x}_j \dot{x}^j[/itex]?


[itex]\frac{\partial L}{\partial x_i}= 2 \phi_{,i} ( \dot{t}^2 +\dot{x}_j \dot{x}^j)[/itex]
 
Last edited:
psimeson said:
I didn't get how you get [itex]{\mu}[/itex]

What is [itex]\dot{x}_j \dot{x}^j[/itex]?

Suppose I have a function f(t,x) and t and x depend on the proper time, t=t(λ) and x=x(λ) along my path. Then

df/dλ = ∂f/∂x dx/dλ + ∂f/∂t dt/dλ.

The Einstein summing convention is just my shorthand way of writing this for all 4 indices. So I would write x,y,z,t as a 4-vector xμ and sum over repeating indices.

It's just a shorthand notation. So latin indices get values 1,2,3 (x,y,z) and greek indices get values 0,1,2,3 (t,x,y,z). I also use Einstein summation convention, so for example
[itex]\dot{x}_j \dot{x}^j = \sum_{j} g_{jj} \dot{x}^j \dot{x}^j = \dot{x}^2+\dot{y}^2+\dot{z}^2 + O(\phi)[/itex]


psimeson said:
...why are you using lower index [itex]\dot{x}_i[/itex]

You're right, my indices are all over the place in that equation :-) You should really do the calculation more carefully.
 
For time, Christoffel Symbol should be:
[itex]{\Gamma^t}_{it}[/itex] = [itex]x_i\frac{\phi'(r)}{r}[/itex]

But by doing the way you suggest I didn't get the answer:

[itex]\frac{d}{d\tau} \frac{\partial L}{\partial \dot{t}} = -2\frac{d}{d\tau} [(1+2\phi) \dot{t}] = -2((1+2\phi)\ddot{t} + 2\dot{t} \phi_{,\mu} \dot{x}^{\mu})[/itex]

[itex]\frac{\partial L}{\partial t}= 0[/itex]

[itex](1+2\phi)\ddot{t} + 2\dot{t} \phi_{,\mu} \dot{x}^{\mu}=0[/itex]

The μ does not really fit, why do you used μ..can't we use {i,j,k}?
 
psimeson said:
For time, Christoffel Symbol should be:
[itex]{\Gamma^t}_{it}[/itex] = [itex]x_i\frac{\phi'(r)}{r}[/itex]

But by doing the way you suggest I didn't get the answer

The μ does not really fit, why do you used μ..can't we use {i,j,k}?

My formula gives the same result, so you must be doing something wrong.

You can use absolutely whatever notation you like, as long as you calculate the derivatives right.
 
I have my solution in the above post I am getting

[itex]\frac{1}{(1+2ϕ)}[/itex]ϕ,μ[itex]\dot{x}[/itex]μ=0

I think my derivatives are correct
 
  • #10
psimeson said:
I have my solution in the above post I am getting

[itex]\frac{1}{(1+2ϕ)}[/itex]ϕ,μ[itex]\dot{x}[/itex]μ=0

I think my derivatives are correct

[itex]\frac{1}{1+2\phi} \phi_{,\mu} x^{\mu} = -\frac{\partial \phi}{\partial t} \dot{t} + \frac{\partial \phi}{\partial x} \dot{x} + \frac{\partial \phi}{\partial y} \dot{y} + \frac{\partial \phi}{\partial x} \dot{y} + O(\phi^2)[/itex]
 

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