Linear FE for static, spherical body

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Discussion Overview

The discussion revolves around the linear vacuum field equations for the external gravitational field of a static, spherical body. Participants explore the mathematical formulation and implications of these equations, particularly in the context of spherical symmetry and coordinate systems.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant inquires about finding the components of h_{ab} and suggests that since the body is static at x = y = z = 0, all spatial derivatives of h_{ab} vanish from the Riemann tensor.
  • Another participant proposes using spherical polar coordinates and letting h_{ab} be a function of r only to maintain spherical symmetry.
  • A different participant expresses confusion regarding the application of the linear field equations, specifically the equation \nabla_{\alpha }\nabla_{\alpha }h_{\mu \nu }= 0, and questions whether to set up a generalized metric similar to full field equations.
  • One participant acknowledges the complexity of deriving the linearized field equations and suggests consulting a textbook for clarification.
  • Another participant states that the linearized field behaves like the electrostatic potential for a Coulomb field, indicating that solutions should satisfy a gauge condition.
  • A participant mentions being comfortable with the derivation but expresses confusion about applying the field equations and Lorentz gauge in curvilinear coordinates.

Areas of Agreement / Disagreement

Participants express varying levels of understanding and confusion regarding the application of the linear vacuum field equations and the implications of spherical symmetry. There is no consensus on the best approach to take in this context.

Contextual Notes

Some participants note the challenges of applying linearized field equations in curvilinear coordinates and the assumptions involved in using Cartesian coordinates. The discussion highlights the need for clarity on gauge conditions and the nature of solutions in spherical symmetry.

WannabeNewton
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How exactly would I go about finding the components of [tex]h_{ab}[/tex] of the linear vacuum field equations for the external gravitational field of a static, spherical body situated at x = y = z = 0 for all t? I assumed since x = y = z = 0 for all t all [tex]h_{ab}[/tex],x and ,y and ,z terms vanish from the Riemann tensor. Do I go about solving [tex]R_{ab}[/tex] = 0 for [tex]h_{ab}[/tex] because I can't really see where the spherical part comes in.
 
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WannabeNewton said:
How exactly would I go about finding the components of [tex]h_{ab}[/tex] of the linear vacuum field equations for the external gravitational field of a static, spherical body situated at x = y = z = 0 for all t? I assumed since x = y = z = 0 for all t all [tex]h_{ab}[/tex],x and ,y and ,z terms vanish from the Riemann tensor. Do I go about solving [tex]R_{ab}[/tex] = 0 for [tex]h_{ab}[/tex] because I can't really see where the spherical part comes in.

Use spherical polar coordinates and let hab=hab(r) be a function of r only. Then you'll have spherical symmetry.
 
I just don't get what to do with the linear field equations in this case: [tex]\nabla[/tex][tex]_{\alpha }[/tex][tex]\nabla[/tex][tex]_{\alpha }[/tex][tex]h_{\mu \nu }[/tex]= 0
([tex]\alpha[/tex]s should be lower indexes sorry)
with [tex]g_{\mu \nu }[/tex] = diag(-1, 1, r[tex]^{2}[/tex], r[tex]^{2}[/tex]sin[tex]^{2}\theta[/tex])

Do I set up a generalized metric like one would for the full field equations?
 
The linear theory is a sort of local theory and assumes we can use approximately Cartesian coords, so my first post is wrong.

It's a tricky business deriving the linearized field equations. I recommend you look it up in a textbook,
or have a look at this

http://www.lehigh.edu/~kdw5/project/howto1.pdf
 
Last edited by a moderator:
The linearized field obeys the linear wave equation, or in this time-independent case Laplace's equation. With spherical symmetry it's just like the electrostatic potential for the Coulomb field of a charge, h ~ m/r. Put together solutions of this form that satisfy your gauge condition.
 
I'm actually fine on the derivation. The subsequent solution for the plane gravitational wave was pretty straight forward too. I'm just confused with what to do with the field equations and the Lorentz gauge in the case of curvilinear coordinates like in this situation.
 

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