Linearising the Geodesic Deviation Equation

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SUMMARY

The discussion focuses on the linearization of the geodesic deviation equation, specifically addressing the relationship between covariant derivatives and partial derivatives in the context of general relativity. The participant highlights the approximation of the particle 4-velocity, Vμ ≈ (1,0,0,0), and the metric perturbation, gμν = ημν + hμν. A key point of contention is the transition from D2Yμ to ∂t2Yμ, questioning the omission of Christoffel symbols and the order of perturbation terms. The participant also corrects the equation D2Yμ = Rμρλν to include the appropriate indices, suggesting it should be D2Yμ = RμρλνVρVλYν.

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  • Understanding of general relativity concepts, particularly geodesics and deviation vectors.
  • Familiarity with covariant and partial derivatives in the context of curved spacetime.
  • Knowledge of the Riemann curvature tensor and its role in geodesic deviation.
  • Basic grasp of metric perturbations and their implications in Einstein's field equations.
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  • Study the derivation of the geodesic deviation equation in general relativity.
  • Learn about the role of Christoffel symbols in relating covariant and partial derivatives.
  • Explore the implications of metric perturbations in gravitational wave theory.
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Xander314
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Homework Statement


Write down the Newtonian approximation to the geodesic deviation equation for a family of geodesics. ##V^\mu## is the particle 4-velocity and ##Y^\mu## is the deviation vector.

Homework Equations


<br /> D = V^\mu\nabla_\mu \\<br /> V^\mu\approx(1,0,0,0) \\<br /> g_{\mu\nu}=\eta_{\mu\nu}+h_{\mu\nu}<br />[/B]
The geodesic deviation equation and the desired linearisation are
<br /> D^2 Y^\mu = R^\mu{}_{\rho\lambda\nu} \\<br /> \partial_t^2 Y^i = -\partial_i\partial_j\phi Y^j<br />

The Attempt at a Solution


Apologies if this is not the correct way to post in this subforum, but I'm not going to write up all of what I have so far as I don't think it's relevant to my question. My issue is with the left hand side, which with the approximation for the 4-velocity becomes
<br /> D^2 Y^\mu = V^\mu\nabla_\mu V^\nu\nabla_\nu Y^\mu = \nabla_t^2 Y^\mu<br />
Everywhere I have looked, the next step is to replace this by ##\partial_t^2 Y^\mu##, but I don't follow this logic. As far as I can see, the covariant and partial derivatives differ by Christoffel symbols containing terms O(h), which should enter into the linearisation. What am I missing? Is Y also O(h)?
 
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Xander314 said:

Homework Statement


Write down the Newtonian approximation to the geodesic deviation equation for a family of geodesics. ##V^\mu## is the particle 4-velocity and ##Y^\mu## is the deviation vector.

Homework Equations


<br /> D = V^\mu\nabla_\mu \\<br /> V^\mu\approx(1,0,0,0) \\<br /> g_{\mu\nu}=\eta_{\mu\nu}+h_{\mu\nu}<br />[/B]
The geodesic deviation equation and the desired linearisation are
<br /> D^2 Y^\mu = R^\mu{}_{\rho\lambda\nu} \\<br /> \partial_t^2 Y^i = -\partial_i\partial_j\phi Y^j<br />

That equation D^2 Y^\mu = R^\mu{}_{\rho\lambda\nu} can't possibly be right, because the left-hand side has only one index, \mu, while the right side has indices \mu, \rho, \lambda, \nu. I think it's supposed to be something like:

D^2 Y^\mu = R^\mu{}_{\rho\lambda\nu} V^\rho V^\lambda Y^\nu
 

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