Linearised Gravitational Waves Derivation

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SUMMARY

The discussion focuses on the derivation of linearised gravitational waves from the Einstein equations, specifically addressing the transition to a wave equation form. Key points include the confusion surrounding the manipulation of the trace-reversed metric, denoted as h-bar, and the application of the Minkowski metric to tensors. The participants clarify the steps involved in substituting and simplifying terms, particularly in Equations (2.6) and (2.7), and emphasize the importance of understanding covariant derivatives and perturbation theory in this context.

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  • Understanding of Einstein's field equations
  • Familiarity with linearised gravity concepts
  • Knowledge of tensor calculus and indices manipulation
  • Basic principles of perturbation theory in general relativity
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  • Study the derivation of linearised gravitational waves in detail
  • Learn about the properties of trace-reversed metrics in general relativity
  • Explore the implications of covariant derivatives on tensor equations
  • Investigate perturbation theory and its applications in gravitational physics
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Students and researchers in theoretical physics, particularly those focusing on general relativity, gravitational wave research, and advanced mathematical physics.

tomelwood
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Hi
A topic came up in a lecture the other day about how if certain simplifications are made, then the Einstein equation reduces to a form of the wave equation.
When I look at derivations of how this happens, I get a little confused as to how this happens.
I think I'm posting it in the right place putting it here, as it's not strictly a homework question, since it is only to help my understanding of the course so far...

Looking at the website http://iopscience.iop.org/1367-2630/7/1/204/fulltext/#nj192710s2
I don't understand why you are allowed to take the step made in Equation (2.9) - i.e. why does putting a prime on the LHS simply mean that you can go ahead and "prime" all of the h in the RHS? If this is allowed, then I can see how the rest of that equality works, no problem.

Secondly, taking a step or two back, where it says substituting "h-bar" into (2.6) "and expanding", how does this simplify down to (2.7)? Because I can see how the terms where both indices are "downstairs" are changed, but what about the h's in the form of a (1,1) tensor? That is one upstairs and one downstairs? I tried applying the Minkowski metric to the (1,1) h, to try and get into "downstairs format" for me to work with, but I was left with some delta's.. Specifically (apologies in advance for appalling Latex):

h^{c}_{a,bc}=\eta^{da}\bar{h}_{ab,bc}-\frac{1}{2}\eta_{ab}\eta^{ad}\bar{h}_{,bc}=\bar{h}^{d}_{b,bc}-\frac{1}{2}\delta\stackrel{d}{b}\bar{h}_{,bc}

and I don't understand how to move on from here?

Any observations would be greatly appreciated.
 
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tomelwood said:
Looking at the website http://iopscience.iop.org/1367-2630/7/1/204/fulltext/#nj192710s2
I don't understand why you are allowed to take the step made in Equation (2.9) - i.e. why does putting a prime on the LHS simply mean that you can go ahead and "prime" all of the h in the RHS? If this is allowed, then I can see how the rest of that equality works, no problem.
Why wouldn't it work? I mean, you just change the coordinates x'^{a} = x^{a} + \xi^{a}. h'_{ab} is the metric in the new gauge, so you just define your trace-reversed metric in the new gauge as \bar{h}'_{a b}= h'_{ab} - 1/2 \eta_{a b} h'

tomelwood said:
Secondly, taking a step or two back, where it says substituting "h-bar" into (2.6) "and expanding", how does this simplify down to (2.7)? Because I can see how the terms where both indices are "downstairs" are changed, but what about the h's in the form of a (1,1) tensor? That is one upstairs and one downstairs? I tried applying the Minkowski metric to the (1,1) h, to try and get into "downstairs format" for me to work with, but I was left with some delta's.. Specifically (apologies in advance for appalling Latex):

h^{c}_{a,bc}=\eta^{da}\bar{h}_{ab,bc}-\frac{1}{2}\eta_{ab}\eta^{ad}\bar{h}_{,bc}=\bar{h}^{d}_{b,bc}-\frac{1}{2}\delta\stackrel{d}{b}\bar{h}_{,bc}

and I don't understand how to move on from here?

Any observations would be greatly appreciated.

You are doing something very naughty there...

\partial_b \partial_c h^c_a = \partial_b \partial_c \bar{h}^c_a + \frac{1}{2} \partial_b \partial_c \delta^c_a h = \partial_b \partial_c \bar{h}^c_a + \frac{1}{2} \partial_b \partial_a h, right?
 
Oh of course. Thanks. OK. So now all that section makes sense, the final step is to show that the trace terms cancel out.
I've been trying to find out the intermediate steps going on, and have managed to solve the equation if I can show that:

h_{,ab}=\frac{1}{2}\eta_{ca}h_{,b}^{c}+\frac{1}{2}\eta_{cb}h_{,a}^{c}
where the superscript c's indicate partial differentiation with respect to c as well (I couldn't make the latex work for that bit)

The only problem is I can't do this, as I know you can't raise/lower indices of partials...
Thanks!
 
Remember two things:
1) what's the covariant derivative of a scalar?
2) in perturbation theory, you can drop everything 2nd order. How big is \Gamma^\mu_{\alpha \beta}?
 

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