# How to obtain the explicit form of Green's function of the Klein-Gordon equation?

The definition of the green's function for the Klein-Gordon equation reads: $$(\partial_t^2-\nabla^2+m^2)G(\vec{x},t)=-\delta(t)\delta(\vec{x})$$ According to these resources:

1. Green's function for the inhomogenous Klein-Gordon equation , the green's function looks like this:

$$G(\vec{x},t) = \frac {\theta(t)} {2 \pi} \delta\Big( t^2 - |\vec{x}|^2 \Big) - \frac {m} {2 \pi} \theta(t - |\vec{x}|) \frac {J_{1}\left(m \sqrt{t^2 - |\mathbf{x}|^2}\right)} {m\sqrt{t^2 - |\mathbf{x}|^2}}$$

1. From the wikipedia, there are several kinds of propagator, which depends on the choice of contour. They looks very like the above one, but still not identical to me. For example, the advanced and retarded green's function looks very similar to the above expression.

I want to derive the explicit form of the above listed green's function, here is what I tried:

Assume: $$G(\vec{x},t)=\int~\mathrm{d}^3p~\mathrm{d}\omega \,e^{i(\vec{p}\cdot\vec{x}-\omega t)}G(\vec{p},\omega)$$

Substitute to Klein-Gordon equation one gets:

$$G(\vec{p},\omega)=\frac{1}{(2\pi)^4}\frac{1}{\omega^2-p^2-m^2}$$

Then: $$G(\vec{x},t)=\frac{1}{(2\pi)^4}\int~\mathrm{d}^3p~\mathrm{d}\omega \,e^{i(\vec{p}\cdot\vec{x}-\omega t)}\frac{1}{\omega^2-p^2-m^2}$$

In the above formula, the pole are on real axis, to get a finite answer, one need manipulate the pole slightly away from the real axis. In Feynman's choice, one has the left pole slightly above and right pole slightly down, like this:

Then we have: \begin{align} G(\vec{x},t)&=\frac{1}{(2\pi)^4}\int~\mathrm{d}^3p~\mathrm{d}\omega \,e^{i(\vec{p}\cdot\vec{x}-\omega t)}\frac{1}{\omega^2-p^2-m^2+i\epsilon} \\ &\text{integrate over $\omega$} \\ &=\theta(t)\frac{-i}{(2\pi)^3}\int~\mathrm{d}^3\vec{p}\frac{e^{i\vec{p}\cdot{x}}e^{-i\sqrt{p^2+m^2}t}}{2\sqrt{p^2+m^2}}+\theta(-t)\frac{-i}{(2\pi)^3}\int~\mathrm{d}^3\vec{p}\frac{e^{i\vec{p}\cdot{x}}e^{i\sqrt{p^2+m^2}t}}{2\sqrt{p^2+m^2}} \\ &\text{integrate over $\phi$ and $\theta$} \\ &=\frac{-i}{(2\pi)^2}\frac{\theta(t)}{|\vec{x}|}\int_0^\infty\frac{p\sin(p|\vec{x}|)e^{-i\sqrt{p^2+m^2}t}}{\sqrt{p^2+m^2}} + \frac{-i}{(2\pi)^2}\frac{\theta(-t)}{|\vec{x}|}\int_0^\infty\frac{p\sin(p|\vec{x}|)e^{i\sqrt{p^2+m^2}t}}{\sqrt{p^2+m^2}} \end{align}

The above derivation seems has no flaw and I don't know how to proceed the $p$ integral, and I can't see the resemblance of the current formula to the closed formula given in resources 1 and 2.

To integrate $p$, I found this integral from the book might help: $$\int_0^\infty e^{-\beta\sqrt{\gamma^2+x^2}} \cos bx =\frac{\beta\gamma}{\sqrt{\gamma^2+\beta^2}}K_1\left(\gamma\sqrt{\beta^2+b^2}\right), \text{ with: \mathrm{Re}\beta>0, \mathrm{Re}\gamma>0}$$

## Edit2

The answer suggested to rotate the contour counter-clockwise ($\omega=i\omega'$), therefore: \begin{align} G_F(\vec{p},\omega)&=\frac{1}{-\omega'^2-|\vec{p}|^2-m^2+i\epsilon} \\ &=-\int_0^\infty \mathrm{d} L\,e^{-L(\omega'^2+|\vec{p}|^2+m^2-i\epsilon)} \end{align}

Plug the above $G_F(\vec{p},\omega)$ into the integral of four momentum: \begin{align} G_F(\vec{x},t)&=\frac{-i}{(2\pi)^4}\int_0^\infty~\mathrm{d}L\,e^{-(m^2-i\epsilon)L}\int\mathrm{d}\omega'\mathrm{d}^3\vec{p}\,e^{-L\omega'^2+t\omega'}e^{-Lp^2+i\vec{x}\cdot\vec{p}} \\ &=\frac{-i}{16\pi^2}\int_0^\infty~\mathrm{d}L\,e^{-(m^2-i\epsilon)L}\frac{1}{L^2}e^{\frac{\tau^2}{4L}}\quad\text{ with $\tau^2=t^2-|\vec{x}|^2$} \end{align}

Since now $\epsilon$ is unimportant to conduct the above integral, just omit it. \begin{align} G_F(\vec{x},t)&=\frac{-i}{16\pi^2}\int_0^\infty\mathrm{d}L\,e^{-m^2L}\frac{1}{L^2}e^{\frac{\tau^2}{4L}} \\ &=\frac{-im^2}{16\pi^2}\int_0^\infty\mathrm{d}\xi\,e^{-\xi}e^{\frac{m^2\tau^2}{4\xi}}\frac{1}{\xi^2} \end{align} When $\tau^2>0$, the integrand diverges at $\xi\to0$, the integral can't be conducted.

When $\tau^2<0$, we have: $$-\frac{im}{4\pi^2\sqrt{-\tau^2}}K_1\left(m\sqrt{-\tau^2}\right)$$ where $K_1$ is modified Bessel function, this is exactly form of the Feynmann propagator when $\tau^2<0$.

Question: Although our result triumphs on one side, what about the other side( $\tau^2>0$)? How can we get it from the above procedure? In which step did we exclude this possibility?

Green's functions are not unique. Any solution of that satisfies the homogeneous equation, $$(\partial_t^2 - \nabla^2 + m^2)f = 0$$ in the region of interest can be added to the Green's function without spoiling the inhomogeneous equation. The homogeneous part must, therefore, be set by boundary conditions. You can get the Bessel function part of the Feynman version of the Green's function by solving for the stationary Green's function with a 4-dimensional space, that is: $$\left(-\frac{1}{r^3} \frac{\partial }{\partial r} \left[r^3 \frac{\partial}{\partial r}\right] + m^2\right)G(r) = \frac{i}{\Omega_4 r^3}\delta(r)$$ and analytically continuing to imaginary time. Inside of the forward light cone, where the argument of $K$ is imaginary, gives a Hankel function of the first kind: \begin{align}\frac{m}{4\pi^2\sqrt{\tau^2}}K_1\left(im\sqrt{\tau^2}\right) &= -\frac{m}{8\pi\sqrt{\tau^2}} H_1^{(2)}\left(m\sqrt{\tau^2}\right) \\ & = -\frac{m}{8\pi\sqrt{\tau^2}} \left[J_1\left(m\sqrt{\tau^2}\right) - i Y_1\left(m\sqrt{\tau^2}\right)\right],\end{align} with $J_a$ and $Y_a$ the Bessel functions of the first and second kind, respectively.

Because both the operator and the inhomogeneous part are real, the imaginary part of the Green's function must be a solution to the homogeneous equation and the real part must solve the inhomogeneous. That is: $$\left(\frac{\partial}{\partial t}^2 - \nabla^2 + m^2\right) \operatorname{Im}\left\{\frac{m}{4\pi^2\sqrt{\tau^2}}K_1\left(im\sqrt{\tau^2}\right)\right\} = 0,\ \mathrm{and} \\ \left(\frac{\partial}{\partial t}^2 - \nabla^2 + m^2\right) \operatorname{Re}\left\{\frac{m}{4\pi^2\sqrt{\tau^2}}K_1\left(im\sqrt{\tau^2}\right)\right\} = -\delta^4(x),$$ so the Green's function is the real part of that expression.

Features that remain to be shown at this point in this post: that the split into retarded and advanced propagators is valid (needed to preserve causality), and the zero mass limit of the propagator gives the correct limit. The energy injected by the impulse cannot be tracked because it is infinite.

• Maybe the second equation should be written as: $$\left[-\frac{1}{r^3} \frac{\partial }{\partial r} r^3 \frac{\partial}{\partial r} + m^2\right]G(r) =\delta(r)$$ ? Sep 14, 2016 at 7:27
• Good catch on the misplaced parentheses. The right hand side, though, only needed a sign correction. It's a 4-dimensional delta function, so it needs to have the 4-dimensional solid angle and the factor of $r^{-3}$. Sep 14, 2016 at 9:25
• I still think the right hand side should change, the original equation is: $$(\partial_t^2-\nabla^2+m^2)G(\vec{x},t)=-\delta(t)\delta(\vec{x})$$ You want to make a substitution $t\to iw$, the above equation becomes: $$(-\nabla_4^2+m^2)G(\vec{r})=-\delta(iw)\delta(\vec{x})$$ Now $\nabla_4^2=\frac{1}{r^3}\partial_r(r^3\partial_r)+\frac{L^2}{r^2}$, where $L^2$ is the operator that differentiate the angular part. If we assume $G(\vec{r})=G(r)$, $L^2$ act on it just gives zero. Therefore, the equation becomes: Sep 15, 2016 at 2:27
• $$(-\frac{1}{r^3}\partial_r(r^3\partial_r)+m^2)G(r)=-\delta(iw)\delta(\vec{x})$$ A question, at this stage, I think we are considering $w$ to be a real variable. However, when comes to $\delta(iw)$(well defined?), do we have the identity that $\delta(iw)=-i\delta(w)$? therefore the right hand side should probably be changed as $i\delta(r)$? Sep 15, 2016 at 2:27
• Indeed, I missed the $i$ in the changeover to Euclidean 4-dimensional space. And, yes, we have $\delta(iw) = -i\delta(w)$. Sep 15, 2016 at 2:30

You could try using the proper time method:

$$\frac{1}{p^2 - m^2 + i \varepsilon} = \intop_0^{\infty} dL \, \exp \left[ -L \left( p^2 - m^2 + i \varepsilon \right) \right].$$

The trick is to do the (Gaussian) momentum integrals first, and then proceed with the integral over $L$. This should give the Bessel function. Let me know in the comments if you have further questions.

UPDATE: How to handle the Lorentz signature in the propagator?

We are interested in the following integral: $$D(x) = \int \frac{d^4 p}{(2\pi)^4} \frac{e^{i p_{\mu} x^{\mu}}}{p^2 - m^2 + i \varepsilon} = \int \frac{d\omega}{2\pi} \: \int \frac{d^3 \vec{p}}{(2\pi)^3} \, \frac{e^{i \omega t} e^{- i \vec{p} \vec{x}}}{\omega^2 - p^2 - m^2 + i \varepsilon}.$$

Now we can rotate the contour of integration in the complex plane in such a way that no pole transits it. I shall rotate the contour from your original post 90 degrees counterclockwise:

$$D(x) = \int \frac{i d\omega'}{2\pi} \: \int \frac{d^3 \vec{p}}{(2\pi)^3} \, \frac{- e^{- \omega' t} e^{- i \vec{p} \vec{x}}}{\omega'^2 + p^2 + m^2}.$$

I have also passed to the new integration variable: $\omega = i \omega'$. Now the denominator is always positive and you can use the proper time method. All integrals will be Gaussian and convergent.

UPDATE 2: The $i \varepsilon$ allows us to rotate the contour counterclockwise, but forbids other (similar) transformation, e.g. rotating it clockwise, like you did. This is because no pole must transit the contour during its deformation. Hence, $\omega = i \omega'$, not $-i \omega'$. Smooth transformations of the contour do not change the integral as long as no pole transits it.

So, the role played by $i \varepsilon$ is to determine how the integral is going to be transformed into the Euclidean integral. In the Euclidean case (after you rotate the contour), you can omit the $i \varepsilon$.

UPDATE 3: since we have rotated the contour, $\omega$ becomes imaginary and $\omega' = - i \omega$ is real (the whole point of introducing ω′ actually). Hence, $\omega'^2 + \vec{p}^2 + m^2$ can not be less than zero!

UPDATE 4: regarding your final answer, I suspect that if you take $\omega = i \omega'$ and not $- i \omega'$ (you are not allowed to pass through the pole, remember?) then you will get the correct answer. I am not sure, of course, but that what I would do.

You do get different Green's functions. It all depends on how where contour walks round the poles, really. Or on where to plug the $i \varepsilon$, if you wish.

UPDATE 5: How to handle the $\tau^2 > 0$ case?

Well, here is what I came up with. You could rotate the contours of the three integrals over $\vec{p}$ instead of the one over $\omega$. After similar calculations, you will arrive at the second Hankel function $H_1^{(2)}$. Alternatively, since we use complex numbers everywhere, we could just do the analytical continuation of the result for $\tau^2 < 0$, which would give us exactly the same Hankel function.

I am still struggling to find a clear explanation of why an additional delta symbol appears (its not like it can not appear, since we have only calculated our propagator for $\tau^2 > 0$ and $\tau^2 < 0$ by now).

• Have you assumed that $p^2-m^2>0$? If written like yours, when doing integral over momentum, the coefficients in front of the $\vec{p}^2$ should be at least negative in the real part. Sep 13, 2016 at 1:13
• since the $\omega^2-\vec{p}^2$ always persist, integrate out the four momentum seems impossible using gaussian integral. Sep 13, 2016 at 1:40
• @buzhidao in my notation, $p^2 = p_0^2 - \vec{p}^{\, 2}$. No, $p^2 - m^2$ is not always greater than zero. You can use the analytical continuation of the Gausian intrgral. Sep 13, 2016 at 11:33
• See my first comment, I think the gaussian integral can be proper defined only if the real part of the coefficient of the square is less than zero. Other wise, you just can't do that, it is divergent. Sep 13, 2016 at 11:43
• @buzhidao if you consider the Euclidean case, the (Euclidean) propagator is proportional to $(p^2 + m^2)^{-1}$ and all Gaussian integrals are well defined. Then, you can obtain the Lorentzian propagator by the analytical continuation (passing to the imaginary time intervals) just as you explained in your question. Alternatively, you can think of the Gaussian integrals to be defined by analytical continuation even when the coefficient in front of the square term is positive. Sep 13, 2016 at 12:31