Parallel transport to explain motion of light near black hole?

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SUMMARY

This discussion centers on the application of parallel transport in explaining the behavior of light near black holes, particularly in relation to gravitational effects and the perception of speed by distant observers. The instructor, teaching a course on relativity, seeks to clarify how parallel transport can be used to illustrate concepts such as gravitational redshift and the apparent speed of light. Key references include Taylor and Wheeler's "Exploring Black Holes" and the pedagogical challenges of conveying complex ideas without delving into advanced mathematics. The consensus is that while parallel transport preserves the norm of lightlike vectors, it does not directly explain changes in the observed speed of light, but rather the frequency shifts due to gravitational effects.

PREREQUISITES
  • Understanding of General Relativity (GR) concepts
  • Familiarity with parallel transport and its mathematical implications
  • Knowledge of gravitational redshift and Doppler effect
  • Basic comprehension of Penrose diagrams and Schwarzschild coordinates
NEXT STEPS
  • Study the concept of gravitational redshift in detail
  • Explore the mathematical framework of parallel transport in curved spacetime
  • Investigate the implications of Schwarzschild coordinates on light behavior near black holes
  • Learn about energy-momentum vectors and their role in relativistic physics
USEFUL FOR

Students and educators in physics, particularly those teaching or learning about General Relativity, as well as anyone interested in the conceptual challenges of explaining complex relativistic phenomena to non-science majors.

  • #31
martinbn said:
If you parallel transport a vector around a loop you can end up with a vector with a diffrent orientation. Then why can't you end up with a vector at 180 degrees angle with the original i.e. a scalor multiple, where the scalor is -1? It seems quit possible. Start at the north pole facing south, walk along a meridian till you reach the equator, move along the equator for half of the circumference, then go back north to the pole. You end up facing the other way compare to you start.

You're right, that's a clear counterexample. I think the problem is my assertion that the result generalizes from infinitesimal parallelograms to larger paths. Now that I think more carefully about it, it's clearly wrong. If you add a bunch of vectors that are not parallel to a given line, you can still get a sum that's parallel to the line.
 
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  • #32
After posting a bunch of wrong stuff about the rescaling of null vectors, I think I finally understand it better. The antisymmetry of the Riemann tensor on its first two indices is exactly the condition needed so that parallel transport around an infinitesimal closed loop doesn't change inner products. For such a loop lying in a fixed plane, the set of possible actions by Riemann tensors are therefore the six-dimensional set of linear transformations that preserve inner products. In other words, they are the set of possible Lorentz transformations. Such a transformation can certainly take a null vector and rescale it.
 
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