Tortoise-like coordinate transform for interior metric

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SUMMARY

The discussion centers on the application of the tortoise coordinate transformation to the Schwarzschild exterior metric within the Klein-Gordon equation. The primary goal of this transformation is to eliminate the coordinate singularity at the event horizon. The challenge arises when attempting to derive a wave equation from the Schwarzschild interior metric, particularly in the context of a fluid sphere, where no singularity exists at the horizon. The conversation highlights the difficulty in achieving a Schrödinger-like form without coupling the effective potential to the energy term.

PREREQUISITES
  • Understanding of the Schwarzschild metric and its properties
  • Familiarity with the Klein-Gordon equation
  • Knowledge of coordinate transformations in general relativity
  • Basic principles of wave equations and effective potentials
NEXT STEPS
  • Research the derivation of the tortoise coordinate transformation for various metrics
  • Study the implications of the Eddington-Finkelstein coordinates in general relativity
  • Explore the relationship between fluid spheres and interior metrics in gravitational theory
  • Investigate methods to decouple energy terms from effective potentials in wave equations
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The discussion is beneficial for theoretical physicists, particularly those specializing in general relativity, quantum field theory, and gravitational wave research.

FunkyDwarf
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Hello!

When using the Schwarzschild exterior metric in the klein-gordon equation one can perform the standard tortoise(E-F) coordinate transform to yield a wave equation which has a well defined potential that is independent of the energy term. My understanding is that the motivation for this coordinate transform was the removal of the coordinate singularity at the horizon of this metric. If one wanted to generate a wave equation from an INTERIOR metric, say the Schwarzschild interior, that also had a well defined potential independent of energy, on what premise would one start, given that if we want to consider a fluid sphere there is no singularity at the horizon?

Certainly i can take the wave equation and put it in a Schrödinger-like form but this yields an effective potential with the energy term coupled to coordinate terms which I must admit i don't know how to transform away without re-instating the first derivative (ie no longer in Schrödinger form).

Hope that makes sense!
 
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Don't know if it's what you want, but one way of arriving at Eddington-Finkelstein coordinates is to find a retarded time that serves to eliminate the dr2 term in the metric. This can be done in general. For

ds2 = A(r)2 dt2 - B(r)2 dr2 + ...

just let u = t ± integral(B/A dr)
 

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