Exterior derivative identity in vacuum space-time

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Discussion Overview

The discussion revolves around the exterior derivative identity in vacuum space-time, particularly focusing on the properties of a scalar field and a Killing vector field. Participants explore the implications of these properties in the context of general relativity, including the vanishing of certain derivatives and the existence of associated forms.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Conceptual clarification
  • Homework-related

Main Points Raised

  • One participant seeks clarification on why the expression ##\nabla_{[e}(2\lambda \nabla_{a}\xi_{b]} + \omega\epsilon_{ab]cd}\nabla^{c}\xi^{d}) = 0## holds in vacuum space-time.
  • Another participant proposes that showing ##\nabla_{[e}(\epsilon_{ab]cd}\nabla^{c}\xi^{d}) = 0## is a key step, leading to the conclusion that the exterior derivative of the 2-form vanishes.
  • It is noted that the Poincaré lemma implies the existence of a 1-form ##\alpha_{a}## such that ##\nabla_{[a}\alpha_{b]} = \frac{1}{2}\epsilon_{abcd}\nabla^{c}\xi^{d}## due to the vanishing of the exterior derivative of the 2-form associated with the Killing vector field.
  • Participants discuss the addition of a gradient to the 1-form to satisfy a specific condition involving the scalar field ##\omega##.
  • One participant asks about the exterior derivative of the twist of the Killing vector field and its vanishing in vacuum space-time, leading to a detailed explanation involving the Riemann curvature tensor.
  • Another participant inquires about the Lie derivative of the twist with respect to another Killing vector field, suggesting an intuitive geometric understanding of the preservation of volume along the flow.

Areas of Agreement / Disagreement

Participants generally agree on the mathematical properties discussed, but there are multiple competing views regarding the implications and specific proofs of the identities in question. The discussion remains unresolved on some aspects, particularly regarding the broader implications of the results.

Contextual Notes

Participants reference specific problems from Wald's general relativity textbook, indicating a shared context of study. The discussion includes complex mathematical expressions and assumptions that are not fully resolved, particularly regarding the implications of the results in broader contexts.

Who May Find This Useful

This discussion may be useful for students and researchers in general relativity, particularly those interested in the properties of Killing vector fields and their implications in vacuum space-time.

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I was reading a paper by Geroch and I was confused by the following: given a scalar field ##\omega## satisfying ##\nabla_{a}\omega = \omega_{a} = \epsilon_{abcd}\xi^{b}\nabla^{c}\xi^{d}## and the scalar ##\lambda = \xi^{a}\xi_{a}##, where ##\xi^{a}## is a killing vector field, can someone prove to me why ##\nabla_{[e}(2\lambda \nabla_{a}\xi_{b]} + \omega\epsilon_{ab]cd}\nabla^{c}\xi^{d}) = 0## if we are in vacuum i.e. ##R_{ab} = 0##? Thanks.
 
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First, it is easiest to show that ##\nabla_{[e}(\epsilon_{ab]cd}\nabla^{c}\xi^{d}) = 0##. Note that this is equivalent to showing ##\epsilon^{abef}\nabla_{e}(\epsilon_{abcd}\nabla^{c}\xi^{d}) = 0## since this then implies ##\epsilon_{ijkf}\epsilon^{abef}\nabla_{e}(\epsilon_{abcd}\nabla^{c}\xi^{d}) = -6\delta^{[a}_{i}\delta^{b}_{j}\delta^{e]}_{k}\nabla_{e}(\epsilon_{abcd}\nabla^{c}\xi^{d}) = -6\nabla_{[k}(\epsilon_{ij]cd}\nabla^{c}\xi^{d}) = 0## which is what we want. We have that ##\nabla_{e}(\epsilon_{abcd}\nabla^{c}\xi^{d}) = \nabla_{e}(\epsilon^{abef}\epsilon_{abcd}\nabla^{c}\xi^{d}) = -4\nabla_{e}(\delta^{[e}_{c}\delta^{f]}_{d}\nabla^{c}\xi^{d}) = -4\nabla_{e}\nabla^{e}\xi^{f} = 4R^{f}{}{}_{d}\xi^{d} = 0## where I have used the fact that ##\nabla^{c}\xi^{d} = \nabla^{[c}\xi^{d]} ## and that ##R_{ab} = 0## since we are in vacuum. Hence ##\nabla_{[e}(\epsilon_{ab]cd}\nabla^{c}\xi^{d}) = 0##. Now for the annoying part :smile:.

Note that by the same argument above, in order to show that the exterior derivative of the 2-form ##\alpha_{ab} = 2\lambda \nabla_{a}\xi_{b} + \omega \epsilon_{abcd}\nabla^{c}\xi^{d}## vanishes, it suffices to show that ##\epsilon^{abef}\nabla_{e}\alpha_{ab} = 0##. Expanding this out, and using the result from the previous paragraph, we get ##\epsilon^{abef}\nabla_{e}\alpha_{ab} = 2\xi^{c}\xi_{c}\epsilon^{abef}\nabla_{e}\nabla_{a}\xi_{b} + 4\epsilon^{abef}\xi_{c}\nabla_{e}\xi^{c}\nabla_{a}\xi_{b} - 4\nabla^{e}\xi^{f}\epsilon_{eabc}\xi^{a}\nabla^{b}\xi^{c}## where I have used the explicit form of the twist of ##\xi^{a}##.

Now, note that ##\epsilon^{abef}\nabla_{e}\nabla_{a}\xi_{b} = \epsilon^{ebaf}\nabla_{a}\nabla_{e}\xi_{b} = -\epsilon^{abef}\nabla_{a}\nabla_{e}\xi_{b}## where in the first equality I renamed the indices and in the second equality I used the antisymmetry of the volume form. Hence ##2\epsilon^{abef}\nabla_{e}\nabla_{a}\xi_{b} = \epsilon^{abef}R_{eab}{}{}^{d}\xi_{d} = \epsilon^{fbea}R^{d}{}{}_{bea}\xi_{d}##. Using the antisymmetry of the volume form and the Bianchi identity ##R_{a[bcd]} = 0##, we have that ##3\epsilon^{fbea}R^{d}{}{}_{bea}\xi_{d} = 3\epsilon^{fbea}R^{d}{}{}_{[bea]}\xi_{d} = 0## thus ##\epsilon^{abef}\nabla_{e}\nabla_{a}\xi_{b} = 0##.

All we're left with now is ##\epsilon^{abef}\nabla_{e}\alpha_{ab} = 4\epsilon^{abef}\xi_{c}\nabla_{e}\xi^{c}\nabla_{a}\xi_{b} - 4 \epsilon_{eabc}\xi^{a}\nabla^{b}\xi^{c}\nabla^{e}\xi^{f}##. Using again the antisymmetry of the volume form and permuting the indices around, we can express this as ##\epsilon^{abef}\nabla_{e}\alpha_{ab} = 8\xi_{c}\nabla^{a}\xi^{b}\epsilon_{abe}{}{}^{[c}\nabla^{f]}\xi^{e}##. As usual, in order to show that this vanishes all we have to show is that ##\epsilon^{klcf}(\nabla^{a}\xi^{b}\epsilon_{abec}\nabla_{f}\xi^{e}) = 0##. This can be easily done as ##\epsilon^{klcf}(\nabla^{a}\xi^{b}\epsilon_{abec}\nabla_{f}\xi^{e}) = \epsilon^{klfc}\epsilon_{abec}\nabla^{a}\xi^{b}\nabla^{e}\xi_{f} = -6\nabla^{[k}\xi^{l}\nabla^{f]}\xi_{f}##. Expanding this out, we have ##-6\nabla^{[k}\xi^{l}\nabla^{f]}\xi_{f} = -2(\nabla^{k}\xi^{l}\nabla^{f}\xi_{f} - \nabla^{k}\xi^{f}\nabla^{l}\xi_{f} + \nabla^{l}\xi^{f}\nabla^{k}\xi_{f}) = - \nabla^{k}\xi^{f}\nabla^{l}\xi_{f}+\nabla^{l}\xi_{f}\nabla^{k}\xi^{f} = 0## where I used the fact that ##\nabla^{f}\xi_{f} = 0## for killing vector fields.

So we finally have that ##\epsilon^{abef}\nabla_{e}\alpha_{ab} = 0## therefore ##\nabla_{[e}\alpha_{ab]} = 0## as desired.
 
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Thank you WannabeNewton, this was very clarifying
 
Yep anytime. I should probably note that this is also problem 5 of chapter 7 in Wald's general relativity text, for future reference.
 
I have another question to ask: in the paper Geroch then says that since ##\nabla_{[e}(\epsilon_{ab]cd}\nabla^{c}\xi^{d}) = 0##, there exists an ##\alpha_{a}## such that ##\nabla_{[a}\alpha_{b]} = \frac{1}{2}\epsilon_{abcd}\nabla^{c}\xi^{d}## and that we can "add a gradient" to make it so that ##\xi^{a}\alpha_{a} = \omega## but why is any of this true?
 
Well ##\omega_{ab} = \epsilon_{abcd}\nabla^{c}\xi^{d}## is just a 2-form so the statement ##\nabla_{[e}\omega_{ab]} = \nabla_{[e}\{\epsilon_{ab]cd}\nabla^{c}\xi^{d}\} = 0## is equivalent to saying that ##d\boldsymbol{\omega} = 0##. By the Poincare lemma, this then implies that locally there exists a 1-form ##\boldsymbol{\alpha}## such that ##\boldsymbol{\omega} = d\boldsymbol{\alpha}## i.e. ##\nabla_{[a}\alpha_{b]} = \frac{1}{2}\epsilon_{abcd}\nabla^{c}\xi^{d}##.

As for your second question, note that if we take an arbitrary smooth scalar field ##\varphi ## and consider ##\alpha_{b} + \nabla_{b}\varphi ## then ##\nabla_{[e}\{\alpha_{b]} + \nabla_{b]}\varphi \} = \nabla_{[e}\alpha_{b]}## since ##\nabla_{a}## is torsion free. So consider ##\tilde{\alpha}_{b} = \alpha_{b} + \nabla_{b}\varphi## such that ##\xi^{b}\tilde{\alpha}_{b} = \omega = \xi^{b}\alpha_{b} + \xi^{b}\nabla_{b}\varphi##. Then all you have to do is, in principle, find a ##\varphi## solving ## \omega = \xi^{b}\alpha_{b} + \xi^{b}\nabla_{b}\varphi## and you can then just use ##\tilde{\alpha}_{b}## as the 1-form that solves ##\nabla_{[a}\tilde{\alpha}_{b]} = \frac{1}{2}\epsilon_{abcd}\nabla^{c}\xi^{d}##.

A similar argument holds for ##\nabla_{[e}\{2\lambda \nabla_{a}\xi_{b]} + \omega\epsilon_{ab]cd}\nabla^{c}\xi^{d}\} = 0##.
 
Thanks. One last question (hopefully): can you explain why the exterior derivative of the twist of the killing vector field identically vanishes in vacuum space-time because Geroch just mentions it, he doesn't prove it.
 
Last edited:
Sure! It is actually quite easy to show that ##\nabla_{[a}\omega_{b]} = 0##. As usual we just have to show that ##\epsilon^{abcd}\nabla_{c}\omega_{d} = \epsilon^{abcd}\epsilon_{defg}\nabla_{c}(\xi^{e}\nabla^{f}\xi^{g}) = 6
\nabla_{c}(\xi^{[b}\nabla^{c}\xi^{d]})## vanishes. Expanding this out we find that ##6\nabla_{c}(\xi^{[b}\nabla^{c}\xi^{d]}) = 2\nabla_{c}(\xi^{b}\nabla^{c}\xi^{d}- \xi^{c}\nabla^{b}\xi^{d} + \xi^{d}\nabla^{b}\xi^{c}) \\ = 2( \xi^{b}\nabla_{c}\nabla^{c}\xi^{d} - \xi^{c}\nabla_{c}\nabla^{b}\xi^{d} - \xi^{d}\nabla_{c}\nabla^{c}\xi^{b} + \nabla_{c}\xi^{b}\nabla^{c}\xi^{d} - \nabla_{c}\xi^{c}\nabla^{b}\xi^{d} + \nabla_{c}\xi^{d}\nabla^{b}\xi^{c}) \\= 2( \xi^{b}\nabla_{c}\nabla^{c}\xi^{d} - \xi^{c}\nabla_{c}\nabla^{b}\xi^{d} - \xi^{d}\nabla_{c}\nabla^{c}\xi^{b} + \nabla_{c}\xi^{b}\nabla^{c}\xi^{d} - \nabla^{c}\xi^{d}\nabla_{c}\xi^{b})\\ = 2(R^{d}{}{}_{e}\xi^{e}\xi^{b} - R^{b}{}{}_{e}\xi^{e}\xi^{d} - \xi^{c}\nabla_{c}\nabla^{b}\xi^{d}) = -2R^{db}{}{}_{ce}\xi^{c}\xi^{e} = 0##

where I used the fact that ##R_{ab} = 0## in vacuum space-time. Hence ##\nabla_{[a}\omega_{b]} = 0##.
 
Is it also true that ##\mathcal{L}_{\psi}\omega_{a} = 0## where ##\psi^{a}## is another killing vector field which is lie transported by ##\xi^{a}##? I ask because geometrically it seems like it should: because one killing vector field is lie transported along the other and the metric tensor is lie transported along any killing vector field (hence intuitively the volume should be preserved along the flow as well), the twist should then be lie transported since it is constructed only out of those quantities.
 
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Yes that is true and your intuition is exactly correct; proving that ##\mathcal{L}_{\psi}\omega_{a} = 0## is also problem 1 of chapter 7 in Wald's general relativity textbook. What has to be shown is that ##\mathcal{L}_{\psi}(\epsilon_{abcd}\xi^{b}\nabla^{c}\xi^{d}) = \xi^{b}\nabla^{c}\xi^{d}\mathcal{L}_{\psi}\epsilon_{abcd} + \xi^{c}\epsilon_{abcd}\mathcal{L}_{\psi}(\nabla^{c}\xi^{d}) = 0## since ##\mathcal{L}_{\psi}\xi^{a} = 0##.

Proceeding, we have that ##\mathcal{L}_{\psi}(\nabla^{a}\xi^{b}) = \psi^{c}\nabla_{c}\nabla^{a}\xi^{b} - \nabla^{c}\xi^{b}\nabla_{c}\psi^{a} - \nabla^{a}\xi^{c}\nabla_{c}\psi^{b}\\ = -R^{abcd}\psi_{c}\xi_{d} +\nabla^{b}\xi^{c}\nabla_{c}\psi^{a} - \nabla^{c}\xi^{a}\nabla^{b}\psi_{c}##.

Now note that ##\nabla^{b}\xi^{c}\nabla_{c}\psi^{a} - \nabla^{c}\xi^{a}\nabla^{b}\psi_{c}\\ = \nabla^{b}(\xi^{c}\nabla_{c}\psi^{a}) - \xi_{c}\nabla^{b}\nabla^{c}\psi^{a} - \nabla^{b}(\psi^{c}\nabla_{c}\xi^{a}) + \psi_{c}\nabla^{b}\nabla^{c}\xi^{a} \\= \nabla^{b}\mathcal{L}_{\xi}\psi^{a} + R^{cabd}\xi_{c}\psi_{d} - R^{dabc}\xi_{c}\psi_{d}##.

Since ##\mathcal{L}_{\xi}\psi^{a}= 0## everywhere in space-time, ##\nabla^{b}\mathcal{L}_{\xi}\psi^{a}= 0## everywhere in space-time as well.
Thus, ##\mathcal{L}_{\psi}(\nabla^{a}\xi^{b}) = \xi_{c}\psi_{d}(R^{dcba}- R^{dbca}+R^{dacb} ) = 0## where in that last line the first Bianchi identity was used.

I personally know of two potential ways to show that ##\mathcal{L}_{\psi}\epsilon_{abcd} = 0## although they both come down to the same final equation. The formulaic way would be to make use of the fact that the volume form ##\epsilon_{abcd}## is totally antisymmetric. Evaluating the lie derivative and using the fact that ##\nabla_{e}\epsilon_{abcd} = 0## (as well as renaming the indices to something more convenient), we have ##\mathcal{L}_{\psi}\epsilon_{a_1a_2a_3a_4} = \epsilon_{ca_2a_3a_4}\nabla_{a_1}\psi^{c} + \epsilon_{a_1ca_3a_4}\nabla_{a_2}\psi^{c} + \epsilon_{a_1a_2ca_4}\nabla_{a_3}\psi^{c} + \epsilon_{a_1a_2a_3c}\nabla_{a_4}\psi^{c}##. Now note that for each term in the RHS, the only index that survives after the sum over ##c## is the one that is not equal to the other three free indices because the volume form is totally antisymmetric i.e. it vanishes when two or more indices are equal. Therefore, ##\mathcal{L}_{\psi}\epsilon_{a_1a_2a_3a_4} = \epsilon_{a_1a_2a_3a_4}\nabla_{c}\psi^{c} = 0## because ##\nabla_{c}\psi^{c} = 0## for a killing vector field. Thus ##\mathcal{L}_{\psi}\omega_{a} = 0##.

As a side note, another way to show that ##\mathcal{L}_{X}\epsilon_{abcd} = \epsilon_{abcd}\nabla_{c}X^{c}## for any vector field ##X^{a}## is to take an infinitesimal 4-parallelepiped in space-time spanned by ##X^{a}## and three infinitesimal connecting vectors ##W^{a},Y^{a},Z^{a}## (infinitesimal connecting vectors are always lie transported along a congruence) and consider the change in the volume ##\epsilon_{abcd}X^{a}W^{a}Y^{a}Z^{a}## of this infinitesimal 4-parallelepiped along the flow of ##X^{a}##. Essentially what's going is that the change in the volume of the 4-parallelepiped along the flow of ##X^{a}## is given by the divergence of ##X^{a}## multiplied by the volume form. Since killing vector fields has vanishing divergence, they preserve the volume as you would expect since killing vector fields lie transport the metric tensor. Many smooth manifolds texts will in fact define the divergence of a vector field in this way.
 

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