Undergrad Check for geodesically-followed path in a coordinate-free way

Click For Summary
SUMMARY

The discussion centers on determining whether a body in flat spacetime follows a geodesic path without relying on a reference frame. It is established that an accelerometer reading zero indicates a geodesic path. Additionally, participants explore alternative methods for verifying geodesic paths, such as measuring distances between points along the path to confirm collinearity. The conversation emphasizes the importance of local criteria for assessing geodesics, particularly through the use of concepts like the Euler-Lagrange equations and the Levi-Civita connection.

PREREQUISITES
  • Understanding of Special Relativity (SR) and flat spacetime concepts
  • Familiarity with accelerometers and their role in measuring proper acceleration
  • Knowledge of Euclidean geometry and properties of straight lines
  • Basic grasp of differential geometry, including connections and parallel transport
NEXT STEPS
  • Research the role of the Levi-Civita connection in defining geodesics in differential geometry
  • Explore the Euler-Lagrange equations and their application in determining geodesic paths
  • Study the implications of curvature in manifolds and its effect on local measurements
  • Investigate alternative methods for measuring proper acceleration beyond traditional accelerometers
USEFUL FOR

Physicists, mathematicians, and students of general relativity interested in the geometric interpretation of motion and the criteria for identifying geodesic paths in spacetime.

  • #91
cianfa72 said:
Thus, sticking at that given non-metric connection, the sentence "walking in the direction you are facing" actually means "keep walking forward step-by-step in the direction at a given fixed angle to the direction shown locally by the compass needle"
which is the way you would be facing at any moment ... you choose to be always facing, e.g. east.
 
Physics news on Phys.org
  • #92
PAllen said:
which is the way you would be facing at any moment ... you choose to be always facing, e.g.east.
But to do that you would have to turn the direction you are facing relative to a gyroscope or to a great circle path.
 
  • Like
Likes cianfa72
  • #93
Dale said:
But to do that you would have to turn the direction you are facing relative to a gyroscope or to a great circle path.
Yes, relative to those. And those would be turning relative to constant bearing.

Let me recap what I consider important points to understand:

1) There is a metric extremal definition of a geodesic. This doesn't explicitly use a connection or any definition of straightness. In the case of Riemannian metric (positive definite), you are requiring that between any two nearby points on a geodesic, there is no shorter path.

2) There is a parallel transport definition of a geodesic as a "straightest possible line". Per a connection, it says the direction of the tangent doesn't change. You need not even have a metric defined to use this definition.

3) For the unique metric compatible connection without torsion (and only for this case), the two geodesic definitions are shown to be equivalent. For any other connection, straightest path geodesics and metric extremal geodesics may be different.

4) There is at least one gravitational theory matching all current observation where there a physically significant connection is used that has torsion that defines straightest lines that are different from geodesics defined by the metric extremal definition. This is Einstein-Cartan theory. Note, the connection has no torsion in vacuum regions, thus replicating all GR vacuum predictions exactly.

5) As an analogy for this not so easy to understand situation, I proposed (not having realized @pervect had used the same example much earlier in the thread) the idea that on a sphere, constant bearing defines non-metric compatible connection and alternate notion of straightness compared to the metric compatible connection. As with Einstein-Cartan theory, each corresponds to a physical observable. Which one you sense (in either example) depends what you measure.
 
Last edited:
  • Informative
Likes Dale
  • #94
PAllen said:
4) There is at least one gravitational theory matching all current observation where there a physically significant connection is used that has torsion that defines straightest lines that are different from geodesics defined by the metric extremal definition. This is Einstein-Cartan theory. Note, the connection has no torsion in vacuum regions, thus replicating all GR vacuum predictions exactly.
Oh cool, I didn't know that. (I agree with your recap on the others)
 
  • #95
Nikodem Popławski has a number of technical and popularized writings about Einstein-Cartan theory. Einstein Cartan theory is able to handle spin 1/2 particles, where GR is either unable to handle them at all, or only handles them with great difficulty. (I'm not sure which is correct.)

Wikipedia has an article on Poplawski's papers, the implications for black holes are especially interesting. Using Einstein-Cartan theory, Poplawski theorizes that black hole collapse doesn't end in a singularity, but that due to the presence of spin 1/2 fermions in the collapsing matter and the extra torsion turns, under the extremely high density conditions during the collapse, cause the torsion terms to halt the collapse. The result, according to Poplawski's analysis, is the creation of a new universe rather than the creation of a singularity.

See for instance https://en.wikipedia.org/w/index.php?title=Nikodem_Popławski&oldid=977163437#Black_holes_as_doorways

Under normal conditions, though, the effect of torsion is unmeasurable. So the theory makes definite physical predictions that are different than GR, but it requires extreme conditions to test.

This lack of testability under normal conditions also implies that even if Einstein-Cartan theory were to be 100 % correct, we could use GR for most things. And the lack of torsion makes the math considerably simpler.
 
  • Informative
Likes Dale
  • #96
Thanks all for support :wink:
 
Last edited:

Similar threads

  • · Replies 3 ·
Replies
3
Views
836
  • · Replies 76 ·
3
Replies
76
Views
4K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 78 ·
3
Replies
78
Views
7K
  • · Replies 17 ·
Replies
17
Views
2K
  • · Replies 22 ·
Replies
22
Views
1K
  • · Replies 16 ·
Replies
16
Views
2K
  • · Replies 27 ·
Replies
27
Views
7K
  • · Replies 9 ·
Replies
9
Views
1K
  • · Replies 11 ·
Replies
11
Views
2K