Solving a 2nd order ODE using Green's Function

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SUMMARY

The discussion focuses on solving the homogeneous Helmholtz equation using Green's function methodology. The Green's function is expressed as G(𝑟₁, 𝑟₂) = ∑(𝑖=1 to ∞) (ψᵢ(𝑟₁)ψᵢ(𝑟₂) / (λ²ᵢ - λ²)), where λ²ᵢ are the eigenvalues and ψᵢ are the eigenfunctions. The participants emphasize the importance of understanding the definition and properties of Green's functions, particularly in relation to linear, nonhomogeneous differential equations. Additionally, the lack of specified boundary conditions raises questions about assumptions in the problem-solving process.

PREREQUISITES
  • Understanding of the Helmholtz equation and its eigenvalues and eigenfunctions.
  • Familiarity with Green's function theory in the context of differential equations.
  • Knowledge of boundary conditions in mathematical physics.
  • Proficiency in mathematical methods for physicists, particularly Arfken's textbook.
NEXT STEPS
  • Study the derivation and applications of Green's functions in solving differential equations.
  • Learn about boundary value problems and how to determine boundary conditions.
  • Explore the mathematical properties of eigenfunctions and eigenvalues in the context of the Helmholtz equation.
  • Review examples of Green's functions in various physical contexts to solidify understanding.
USEFUL FOR

This discussion is beneficial for physics students, mathematicians, and researchers working with differential equations, particularly those interested in mathematical methods for solving boundary value problems in physics.

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Homework Statement


The homogeneous Helmholtz equation

[tex]\bigtriangledown^2\psi+\lambda^2\psi=0[/tex]

has eigenvalues [tex]\lambda^2_i[/tex] and eigenfunctions [tex]\psi_i[/tex]. Show that the corresponding Green's function that satisfies

[tex]\bigtriangledown^2 G(\vec{r}_1, \vec{r}_2)+\lambda^2 G(\vec{r}_1, \vec{r}_2)=-\delta(\vec{r}_1-\vec{r}_2)[/tex]

may be written as

[tex]G(\vec{r}_1, \vec{r}_2)=\sum_{i=1}^{\infty}\frac{\psi_i(\vec{r}_1)\psi_i(\vec{r}_2)}{\lambda^2_i-\lambda^2}[/tex]

Homework Equations



[tex]\int(\psi \bigtriangledown^2 G-G\bigtriangledown^2 \psi) d\tau_2=\int(\psi \bigtriangledown G-G\bigtriangledown\psi) d\sigma[/tex]

The Attempt at a Solution



I'm using Arfken's Mathematical methods for physicists, and it isn't very good at explaining the examples it uses. I just need some kind of jump start to get me going. Do I need to use the equation in the relevant equations section?
 
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You might want to start by writing out the definition of "Green's function"- that's far more important than examples.

Green's function for a linear, nonhomogeneous, differential equation, L(Y)=f(x), where L( ) is a linear differential operator, with given boundary conditions, is a function G(r, r') such that
1) L(G(r,r'))= 0 for all r not equal to r'
2) limit as r->r' from the right of L(G(r, r')) minus the limit as r->r' from the left of L(G(r,r'))= 1.
3) G(r, r') satisfies the boundary conditions.
2)
 
How do I know the boundary conditions? The problem doesn't state any. Do I just assume there aren't any?
 

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