Tensor Calculus General Theory of Relativity

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Homework Help Overview

The discussion revolves around finding the differential equations governing the paths of test particles in a specific space-time metric related to the general theory of relativity. The metric provided is expressed in terms of a constant \( k \) and involves a combination of spatial and temporal components.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the calculation of geodesics from the given metric and the application of the geodesic equation involving Christoffel symbols. Questions arise regarding the differentiation needed to compute these symbols and the interpretation of the metric tensor.

Discussion Status

Some participants have provided hints about calculating the Christoffel symbols and the relationship between the metric and the geodesic equation. There is an ongoing exploration of how to derive the necessary components from the metric, with no explicit consensus reached yet.

Contextual Notes

Participants express uncertainty about the differentiation process required for the metric and the Christoffel symbols, indicating a potential gap in understanding the underlying concepts from their lectures.

Sissy
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Hello

I have huge problems with the following exercise. Please give me some hints. No complete Solutions but a little bit help.


Find the differential equations of the paths of test particles in the space-time of which the metric ist

[tex]\mathrm{d}s^2 = e^{2kx} \left[- \left( \mathrm{d}x^2 + \mathrm{d}y^2 +\mathrm{d}z^2 \right) + \mathrm{d}t^2 \right][/tex],

where [tex]k[/tex] is a constant. If

[tex]v^2 = \left( \dfrac{\mathrm{d} x }{\mathrm{d} t } \right)^2 + \left( \dfrac{\mathrm{d}y }{\mathrm{d}t } \right)^2 + \left( \dfrac{ \mathrm{d} z }{\mathrm{d} t } \right)^2[/tex]

and if [tex]v=V[/tex] when [tex]x=0[/tex], show that

[tex]1-v^2 = \left( 1-V^2 \right) e^{2kx}[/tex].


Now I have no idea how to start. I do not want a solution. I will calculate it on my own but I need some assistance.

greetings
 
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Do you know how to calculate the equation for geodesics given a metric? Test particles will follow geodesics.
 
In the lecture we had this equation:

[tex]\dfrac{\mathrm{d}^2 x^i }{ \mathrm{d} s^2 } + \Gamma ^i _{kl} \dfrac{ \mathrm{d} x^k}{ \mathrm{d} s} ~ \dfrac{\mathrm{d} x^l}{ \mathrm{d} s} = 0[/tex]

But how to use this in my problem?

greetings
 
First calculate the [tex]\Gamma^i_{jk}[/tex] terms. Do you know how to do this? Then you have a set of differential equations for the 4-velocity components.
 
We introduced [tex]\Gamma ^m_{kl}[/tex] as

[tex]\Gamma ^m_{kl} = g^{im} \Gamma_{ikl}[/tex]

with

[tex]\Gamma_{ikl} = \dfrac{1}{2} \left( \dfrac{\partial g_{ik}}{\partial x^l} + \dfrac{\partial g_{li}}{\partial x^k} + \dfrac{\partial g_{kl}}{ \partial x^i} \right)[/tex]

and called [tex]\Gamma_{ikl}[/tex] Christoffel symbols of first kind and [tex]\Gamma ^m_{kl}[/tex] Christoffel symbols of second kind.

I think [tex]g[/tex] is the metric tensor coming from the Riemann-metric but how to calculate this [tex]g[/tex]? This is something I even did not understand it in the lecture. :frown::confused:

Also from lecture we know

[tex]\mathrm{d}s^2 = g_{lm} \mathrm{d}x^l \mathrm{d}x^m[/tex]

But I don't know how to work with this.

You said that I should calculate this christoffel symbols of second kind but what I have to differentiate in the exercise and why? I only have this metric and velocity square?

thanks for help
 
You have it right there. You've told me:
[tex] \mathrm{d}s^2 = g_{lm} \mathrm{d}x^l \mathrm{d}x^m [/tex]

and:

[tex] \mathrm{d}s^2 = e^{2kx} \left[- \left( \mathrm{d}x^2 + \mathrm{d}y^2 +\mathrm{d}z^2 \right) + \mathrm{d}t^2 \right][/tex]

So, remembering that

[tex]dx^i = (dt, dx, dy, dz)[/tex]

Can you tell me what [tex]g_{ij}[/tex] is? If not, you need to go back and review whatever textbook or reference materials you are using.
 

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