Solve Eq. (9.58) on Schutz Page 246 - A First Course in GR

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The discussion revolves around solving Equation (9.58) from "A First Course in GR" by Schutz, specifically in a vacuum region where the source term \( S_{\mu \nu} = 0 \). The equation can be approached using separation of variables, leading to a differential equation for \( f_k(r) \). The participants clarify that the appearance of the separation constant \( k \) in the resulting ordinary differential equation is a common occurrence in this method. The focus is on understanding how the separation constant influences the solution process.

PREREQUISITES
  • Familiarity with differential equations, particularly separation of variables.
  • Understanding of spherical harmonics, specifically \( Y_{km} \).
  • Knowledge of the concepts in general relativity as presented in Schutz's textbook.
  • Basic skills in mathematical notation and manipulation of equations.
NEXT STEPS
  • Study the method of separation of variables in partial differential equations.
  • Explore the properties and applications of spherical harmonics in physics.
  • Review the derivation and implications of separation constants in differential equations.
  • Examine the context and applications of Equation (9.58) in general relativity.
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Students and researchers in physics, particularly those studying general relativity, as well as mathematicians focusing on differential equations and their applications in theoretical physics.

Jimmy Snyder
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Here is a question from problem 26 part a on page 246 of "A First Course in GR" by Schutz. I doubt that it can be answered by someone without a copy of the book, but I have thought that before and been wrong. If someone without the book wants to help and needs more information then of course I would promptly provide it.

Eq. (9.58) in the vacuum region outside the source - i.e., where [itex]S_{\mu \nu} = 0[/itex] - can be solved by separation of variables.

Eq (9.58) (edited) follows:

[tex] (\nabla^2 + \Omega^2)(\bar{h}_{\mu \nu}e^{i\Omega t}) = 0[/tex]

Assume a solution for [itex]\bar{h}_{\mu \nu}[/itex] has the form

[tex] \Sigma_{km}A^{km}_{\mu \nu}f_k(r)Y_{km}(\theta, \phi)/\sqrt{r}[/tex]

where [itex]Y_{km}[/itex] is the spherical harmonic. (The book uses l as does everyone else on the planet, but I changed l to k so that this post would read more easily).

(a) Show that [itex]f_k(r)[/itex] satisfies the equation:

[tex] \ddot{f}_k + \frac{1}{r}\dot{f}_k + [\Omega^2 - \frac{(k+\frac{1}{2})^2}{r^2}]f_k = 0[/tex]

where dot means differentiation with respect to r. Without even trying to solve this problem, my question is simply this: how can k show up in the differential equation? Neither A nor Y are functions of r, and k is just a subscript on f.
 
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k is (related to) the separation constant. When solving partial differential equations by the technique of separation of variables, the separation constant often appears, after rearrangement, in the resulting ordinary differential equations.

Regards,
George
 
George Jones said:
k is (related to) the separation constant.
Thanks George, I got out a book on DiffEQs and looked up separation constant. It looks like I'll be spending some time on this.
 

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