Christoffel symbols for gravitational waves

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SUMMARY

The discussion focuses on calculating the Christoffel symbol \(\Gamma^{t}_{xx}\) for the metric \(ds^2 = -c^2dt^2 + (1+h\sin(\omega t))dx^2 + (1-h\sin(\omega t))dy^2 + dz^2\). The correct answer is established as \(\frac{h\omega}{2} \cos(\omega t)\). Participants highlight the importance of using natural units and the potential confusion between using \(t\) and \(ct\) as coordinates. The discussion emphasizes the utility of the equation for Christoffel symbols derived from the metric's first derivatives for simplifying calculations.

PREREQUISITES
  • Understanding of general relativity concepts, particularly Christoffel symbols.
  • Familiarity with metric tensors and their derivatives.
  • Knowledge of Lagrangian mechanics and the Euler-Lagrange equation.
  • Proficiency in using natural units in physics calculations.
NEXT STEPS
  • Study the derivation and application of Christoffel symbols in general relativity.
  • Learn about the implications of using natural units in gravitational wave physics.
  • Explore the Euler-Lagrange equation in the context of curved spacetime.
  • Investigate the relationship between metric tensors and geodesic equations.
USEFUL FOR

This discussion is beneficial for physicists, particularly those specializing in general relativity, gravitational wave research, and advanced mechanics. It is also useful for students seeking to deepen their understanding of Christoffel symbols and their applications in theoretical physics.

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Homework Statement


Determine the Christoffel symbol [tex]\Gamma^{t}_{xx}[/tex] for the metric [tex]ds^2 = -c^2dt^2 + (1+h\sin(\omega t))dx^2 + (1-h\sin(\omega t))dy^2 + dz^2[/tex]

The answer should be: [tex]\frac{h\omega}{2} \cos(\omega t)[/tex]

Homework Equations


For the evaluation we have to use [tex]\frac{d^2x^\alpha}{d\tau^2}+\Gamma^\alpha_{\mu\nu}\frac{dx^\mu}{d\tau}\frac{dx^\nu}{d\tau}[/tex]


The Attempt at a Solution


I keep getting c's where they shouldn't be. I calculated the Euler Lagrange Equation for the time to be:
[tex]-2\frac{d^2(ct)}{d\tau^2}-c^{-1}\omega h\cos(\omega t)((\frac{dx}{d\tau})^2 - (\frac{dy}{d\tau})^2) = 0[/tex]
Which leaves us with the equation of motion
[tex]\frac{d^2 t}{d\tau^2}+\frac{1}{2c^2}\omega h\cos(\omega t)((\frac{dx}{d\tau})^2 - (\frac{dy}{d\tau})^2) =0[/tex]
So the answer is:
[tex]\Gamma^{t}_{xx}=\frac{h\omega}{2c^2} \cos(\omega t)[/tex]
Where have I gone wrong? Also, I don't understand whether you are supposed to take t or ct as the zero'th coordinate and whether it gives a different answer.
 
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are you sure you're not working in natural units because I get the same answer as you. i don't think it cancels. you could redefine t' = ct but that still gives you factors of c
 
Don't know if you already figured it out but the problem probably wanted it in natural units. Also, when you only have one specific Christoffel symbol to calculate it is much easier to just use the equation for the Christoffel symbols in terms of permutations of first derivatives of the metric; I am sure you know which one this is (too lazy to do all the latex business).
 

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