Tensor Calculus General Theory of Relativity

AI Thread Summary
The discussion revolves around finding the differential equations for test particles in a specific space-time metric given by ds² = e²kx[-(dx² + dy² + dz²) + dt²]. Participants seek guidance on calculating the Christoffel symbols necessary for deriving geodesic equations, emphasizing the importance of understanding the metric tensor g and its components. There is confusion regarding the differentiation process required to compute the Christoffel symbols and how to apply them to the problem at hand. Clarifications are provided on the relationship between the metric and the Christoffel symbols, indicating that a solid grasp of the underlying concepts is essential for solving the exercise. The thread highlights the need for foundational knowledge in tensor calculus and general relativity to tackle such problems effectively.
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

\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],

where k is a constant. If

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

and if v=V when x=0, show that

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


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:

\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

But how to use this in my problem?

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

\Gamma ^m_{kl} = g^{im} \Gamma_{ikl}

with

\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)

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

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

Also from lecture we know

\mathrm{d}s^2 = g_{lm} \mathrm{d}x^l \mathrm{d}x^m

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:
<br /> \mathrm{d}s^2 = g_{lm} \mathrm{d}x^l \mathrm{d}x^m <br />

and:

<br /> \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]<br />

So, remembering that

dx^i = (dt, dx, dy, dz)

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