Locally inertial coordinates on geodesics

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Discussion Overview

The discussion revolves around the possibility of constructing a coordinate system in general relativity (GR) where the metric tensor is Minkowskian along an entire geodesic. The conversation explores the implications of the equivalence principle and the behavior of Christoffel symbols in relation to geodesics.

Discussion Character

  • Exploratory, Technical explanation, Conceptual clarification

Main Points Raised

  • One participant states that it is a standard fact in GR that at a point in spacetime, a coordinate system can be constructed such that the metric tensor resembles Minkowski spacetime and its first derivatives vanish, leading to vanishing Christoffel symbols.
  • The same participant questions whether it is possible to extend this to a coordinate system where the metric is Minkowskian along an entire geodesic, suggesting that this aligns with the equivalence principle.
  • Another participant references Fermi normal coordinates as a potential solution, noting that these were originally developed for Riemannian manifolds and later generalized to pseudo-Riemannian manifolds.
  • A later reply expresses appreciation for the reference provided.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the feasibility of constructing such a coordinate system along an entire geodesic, though there is acknowledgment of the relevance of Fermi normal coordinates.

Contextual Notes

The discussion does not resolve the mathematical details or assumptions underlying the construction of Fermi normal coordinates or their applicability to the problem posed.

VantagePoint72
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It's a standard fact of GR that at a given point in space-time, we can construct a coordinate system such that the metric tensor takes the form of Minkowski spacetime and its first derivatives vanish. Equivalently, we can make the Christoffel symbols vanish at point. Moreover, the fact that, in general, there's no coordinate system that let's us do this simultaneously for the entire manifold is the essence of curvature.

But, is it possible to construct a coordinate system such that the metric is Minkowskian along an entire geodesic? Since geodesics are the generalization in GR of inertial motion, it seems intuitively that it should be possible to do so. According to the equivalence principle, an arbitrarily small 'laboratory' falling along a geodesic should be unable to determine if its in an inertial (in the SR sense) frame in flat spacetime or falling along a geodesic in curved spacetime. It seems to me that finding a coordinate system in which the Christoffel symbols along the geodesic vanish would be mathematical realization of this.
 
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http://relativity.livingreviews.org/Articles/lrr-2011-7/fulltext.html

Try the section Fermi normal coordinates, and see the remarks after Eq 9.16.
 
Last edited by a moderator:
It sounds like you're describing Fermi coordinates. Fermi originally did this for a Riemannian manifold, but it was later generalized to pseudo-Riemannian manifolds.
 
Perfect, thank you!
 

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