A physical description of some GR concepts

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Discussion Overview

The discussion centers on the physical interpretation of expansion, rotation, and shear in the context of time-like congruences in general relativity. Participants explore both mathematical formulations and intuitive analogies to clarify these concepts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant describes the mathematical framework for expansion, rotation, and shear, using the metric tensor and properties of time-like congruences.
  • Another participant offers a physical analogy involving a ball of coffee grounds to illustrate how these concepts manifest in a more intuitive manner.
  • There is a discussion on the condition under which the rotation tensor vanishes and its relation to hypersurface orthogonality, with one participant providing a detailed explanation based on the twist of the congruence.
  • Some participants express appreciation for both the intuitive and mathematical explanations provided, indicating a recognition of the value in both approaches.

Areas of Agreement / Disagreement

While there is a general understanding of the concepts being discussed, the discussion includes both mathematical and intuitive perspectives, suggesting that multiple views remain on how best to convey these ideas. No consensus is reached on a singular explanation or interpretation.

Contextual Notes

Participants rely on specific mathematical definitions and properties, such as the use of the metric tensor and the implications of Frobenius' theorem, which may not be universally understood without further context.

Who May Find This Useful

This discussion may be useful for students and researchers in physics, particularly those interested in general relativity, as well as educators seeking to convey complex concepts in both rigorous and intuitive ways.

R136a1
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Can someone explain what the expansion, rotation, and shear of a time-like congruence are physically?
 
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Sure. Let ##\xi^{a}## be a time-like congruence and ##\gamma## an integral curve of ##\xi^a##; let ##p\in \gamma(I)##. Take an orthonormal basis ##\{\xi^{a},\eta^{a}_{1},\eta^{a}_{2},\eta^{a}_{3}\}## for ##T_p M## such that ##\mathcal{L}_{\xi}\eta^{a}_{i} = 0,\forall i## (i.e. the ##\eta^{a}_{i}## are infinitesimal connecting vectors). The metric tensor can be written in this basis as ##g_{ab} = -\xi_{a}\xi_{b} + \eta^{1}_{a}\eta^{1}_{b} + \eta^{2}_{a}\eta^{2}_{b} + \eta^{3}_{a}\eta^{3}_{b}## so the spatial metric ##h_{ab}## is given by ##h_{ab} = g_{ab} + \xi_{a}\xi_{b} = \eta^{1}_{a}\eta^{1}_{b} + \eta^{2}_{a}\eta^{2}_{b} + \eta^{3}_{a}\eta^{3}_{b} ##. I now claim that the expansion ##\theta = \nabla_{a}\xi^{a}## represents the expansion of the infinitesimal space-time volume ##V = \epsilon_{abcd}\xi^{a}\eta^{b}_{1}\eta^{c}_{2}\eta^{d}_{3}## carried along ##\gamma##. We have that ##\xi^{n}\nabla_{n}\eta^{b}_{i} = \eta_{i}^{n}\nabla_{n}\xi^{b}## so ##\xi^{a}\nabla_{a}V = \epsilon_{abcd}\{(\xi^{n}\nabla_{n}\xi^{a})\eta^{b}_{1}\eta^{c}_{2}\eta^{d}_{3} + ...+(\eta_{3}^{n}\nabla_{n}\xi^{d})\xi^{a}\eta^{b}_{1}\eta^{c}_{2}\}##. Note that ##\epsilon_{abcd}\eta^{b}_{1}\eta^{c}_{2}\eta^{d}_{3}## must be parallel to ##\xi^{a}## at ##p## hence ##\epsilon_{abcd}\eta^{b}_{1}\eta^{c}_{2}\eta^{d}_{3} = \alpha \xi^{a}\Rightarrow \alpha = -V## at ##p##. As a result, ##\epsilon_{abcd}(\xi^{n}\nabla_{n}\xi^{a})\eta^{b}_{1}\eta^{c}_{2}\eta^{d}_{3} = -V\xi^{n}\xi_{a}\nabla_{n}\xi^{a} = 0## at ##p##. Handling the other terms in a similar manner, we end up with ##\xi^{n}\nabla_{n}V = V(g_{r}^{n} + \xi_{r}\xi^{n})\nabla_{n}\xi^{r} = V\nabla_{n}\xi^{n} = V\theta## as desired. If we imagine a small ball centered at ##p##, ##\theta## tells us how its volume changes instantaneously.

As for the shear ##\sigma_{ab}##, note that because it is symmetric we can find an orthonormal basis for ##T_p M## that orthogonally diagonalizes ##\sigma_{ab}## on top of the spatial basis vectors being lie transported along the integral curve of the time-like basis vector ##\xi^{a}## and as a result write ##\sigma_{ab} = k_{1}\eta^{1}_{a}\eta^{1}_{b} + k_{2}\eta^{2}_{a}\eta^{2}_{b} + k_{3}\eta^{3}_{a}\eta^{3}_{b}##. ##\sigma_{ab}## is also traceless so that places a constraint on the eigenvalues ##k_{i}##. Now assume that at ##p##, the expansion and rotation vanish so that at ##p## we have ##\xi^{n}\nabla_{n}\eta_{i}^{a} = k_{i}\eta^{a}_{i}## after using the various conditions above. Now if we imagine a reference observer ##O##, an infinitesimally nearby observer ##O'##, and think of ##\eta^{a}_{i}## as a connecting vector between the two then the above tells us that ##O'## has an instantaneous velocity at ##p## relative to ##O## that is directed along ##\eta^{a}_{i}## so each ##\eta^{a}_{i}## defines an axis of instantaneous expansion/contraction with value ##k_{i}##. Because of the trace constraint, expansion along one such axis must be sufficiently compensated for by contractions along the other axes so if we imagine a small ball centered at ##p##, this ball will get distorted into an ellipse.

Rotation is the obvious one in the kinematical decomposition. It simply measures the extent to which the congruence fails to be hypersurface orthogonal i.e. ##\omega_{ab} = 0## if and only if ##\xi_{[a}\nabla_{b}\xi_{c]} = 0##. Geroch gives a nice pictorial interpretation of this as follows: picture a normal twisted rope and note that there is no way you can slice the rope using a plane such that all the fibers of the twisted rope intersecting the plane are orthogonal to the plane.
 
R136a1 said:
Can someone explain what the expansion, rotation, and shear of a time-like congruence are physically?

I'll try a more "physical" and less rigorous description than Wanabee Newton's.

Consider a ball of coffee grounds - ala Baez, http://math.ucr.edu/home/baez/einstein/ "The meaning of Einstein's equation".

The worldlines of the individual grounds will trace out a time-like congruence. (The worldlines must be time like, and we'll assume the rest of the properties needed).

Then the ball can change it's volume. That's expansion. It can get squashed into an ellipsoid. That's shear. And, of course, it can rotate.
 
Thanks a lot pervect for giving a great intuition. And thanks miss wbn for giving a very neat mathematical derivation for the intuition!
 
May I ask why why ##\omega_{ab} = 0## if and only if ##\xi^{a}## is hypersurface orthogonal?
 
Well first consider the twist ##\omega_{a} = \epsilon_{abcd}\xi^{b}\nabla^{c}\xi^{d}## of the time-like congruence. The rotation will be given in terms of the twist by ##\omega_{ab} = \epsilon_{abcd}\xi^{c}\omega^{d}##. Hence if ##\omega_{ab} = 0## then ##\xi^{c}\omega^{d} - \xi^{d}\omega^{c} = 0## so ##\omega_{a} = 0##. This then implies that ##\xi^{[b}\nabla^{c}\xi^{d]} = 0## so ##\xi^{a}## is hypersurface orthogonal by Frobenius' theorem. As for the converse, if ##\xi^{a}## is hypersurface orthogonal then ##\xi^{a} = f\nabla^{a}g## for smooth scalar fields ##f,g##
so ##\omega_{ab} = h_{[a}{}{}^{m}h_{b]}{}{}^{n}\nabla_{m}\xi_{n} = fh_{a}{}{}^{m}h_{b}{}{}^{n}\nabla_{[m}\nabla_{n]}g + h_{a}{}{}^{m}h_{b}{}{}^{n}\nabla_{[m}f\nabla_{n]}g = 0## because ##\nabla_{a}## is torsion free (i.e. it commutes on smooth scalar fields) and ##h_{a}{}{}^{m}\nabla_{m}g = f^{-1}h_{a}{}{}^{m}\xi_{m} = 0##.
 
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Thank you, that was a very good explanation!
 

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