4
$\begingroup$

Assuming we are given a Lagrangian \begin{equation} \mathcal{L}(\phi(r),\partial^i\phi(r)) = \frac{1}{2} \partial_i\phi \partial^i\phi + \frac{m^2}{2} \phi^2 + \lambda \phi, \end{equation} the equations of motion obtained from the Euler-Lagrange equations are \begin{equation} (\Delta-m^2) \phi = \lambda. \end{equation} In order to find the Green's function for this system, the standard procedure would be to impose $(\Delta-m^2)G(r) = \delta(r)$, going to Fourier space in order to get an algrbraic equation ($\Delta \rightarrow k^2$) and get $G(r)$ by performing the inverse Fourier transform.

However, assuming we know that $G \propto r^{-1}e^{-mr}$, is there a way to find the proper normalization for the Green's function directly from the equations of motion, without using the above procedure?

$\endgroup$
3
  • 1
    $\begingroup$ The normalization constant, $1/4\pi$ is the same as for the unscreened Poisson equation, for the very same reason. Do you remember how to get that by integrating both sides (perhaps from EM)? The $\delta$ on the r.h.s. is a 3 dimensional one! $\endgroup$ Commented Feb 5, 2020 at 15:55
  • $\begingroup$ In the unscreened case I can integrate over both sides and apply the divergence theorem, but I am having trouble to do the same thing here, as $\int_0^R m^2 r^{-1}\exp(-mr) \mathrm{d}r$ diverges. $\endgroup$
    – scaphys
    Commented Feb 5, 2020 at 18:06
  • $\begingroup$ Update: I missed the Jacobian. The question is therefore solved. I will write it up as an answer. $\endgroup$
    – scaphys
    Commented Feb 5, 2020 at 18:23

1 Answer 1

0
$\begingroup$

Integrating $(\Delta-m)G(\mathbf{r}) = \delta(\mathbf{r})$ with the ansatz $G(r) = A r^{-1} \exp(-mr)$ over a sphere of radius R yields \begin{align} 1 &= A\int_V \Delta\Big(\frac{e^{-mr}}{r}\Big)-m^2\frac{e^{-mr}}{r} \;\mathrm{d}V\\ &= A\int_V \partial_r\left[r^2\partial_r\Big(\frac{e^{-mr}}{r}\Big)\right]-m^2re^{-mr} \;\mathrm{d}r\mathrm{d}\Omega\\ &= 4\pi A\int_0^R \partial_r\left[r^2\partial_r\Big(\frac{e^{-mr}}{r}\Big)\right]-m^2re^{-mr} \;\mathrm{d}r\\ &= -4\pi A \left[(1+mR)e^{-mR}\right]+\left[1-(1+mR)e^{-mr}\right] \\ &= -4 \pi A. \end{align} Therefore, $A = -\frac{1}{4\pi}$.

$\endgroup$

Your Answer

By clicking “Post Your Answer”, you agree to our terms of service and acknowledge you have read our privacy policy.

Not the answer you're looking for? Browse other questions tagged or ask your own question.