Given the Klein Gordon equation (◻+m2)ϕ(t,x)=0
From this we can calculate the required evolution of the Fourier modes ˜ϕ(t,k) such that at each instant in time t, ϕ(t,x) is a solution to the Klein Gordon equation. This can be done, following on from the above, as follows: (◻+m2)ϕ(t,x)=(◻+m2)∫d3x(2π)3˜ϕ(t,k)eik⋅x=∫d3x(2π)3[(∂2t+k2+m2)˜ϕ(t,k)]eik⋅x=0⇒(∂2t+k2+m2)˜ϕ(t,k)=0
Question: This is all well and good, but why is it that in this case we only perform a Fourier decomposition of the spatial part only, whereas in other cases, such as for finding solutions for propagators (Green's functions), we perform a Fourier decomposition over all 4 spacetime coordinates? [e.g. G(x−y)=∫d4x(2π)4˜G(t,k)eik⋅x
Is it simply because when we construct the appropriate QFT for a scalar field we do so in the Heisenberg picture, or is there something else to it?
Apologies if this is a really dumb question but it's really been bugging me for a while and I want to get the reasoning straight in my mind!
Answer
Notation: x=(t,x); k=(k0,k); kx=k0t−k⋅x; dx=dtd3x; etc.
You can in principle perform the Fourier decomposition on both space and time variables, but to do so you'll need several properties of the Dirac's delta funciton:
The first one is: let ξ∈R; then δ(f(ξ))=∑f(ξi)=0δ(ξ−ξi)|f′(ξi)|
The second one is that, given g(ξ) a known function, the distributional solution of g(ξ)f(ξ)=0 is f(ξ)=h(ξ)δ(g(ξ)) for an arbitrary function h(ξ). If you believe these, then the Fourier decomposition is as follows:
Let ϕ(x) be the solution of (∂2+m2)ϕ(x)=0
Take the Fourier transform of the equation to find (k2−m2)ϕ(k)=0
As ϕ(x) is a distribution, the solution of (2) is ϕ(k)=h(k)δ(k2−m2) for an arbitrary function h(k). Inverting the Fourier Transform, we find ϕ(x)=∫dk e−ikxh(k)δ(k2−m2)
Next, use (1) to expand the delta over the roots of k2−m2. These roots are easily found to be k0=±ω(k), where ω(k)=+(k2+m2)1/2. Therefore, it is immediate to get ϕ(x)=∫dk e−ikxh(k)12ω[δ(k0−ω)+δ(k0+ω)]
Finally, make the change of variable k→−k in the second term, which yeilds the usual expansion ϕ(x)=∫dk2ω [e−ikxa(a)+e+ikxb†(k)]
As you can see, the solution is the same as yours (modulo some irrelevant prefactor that can be reabsorbed into the definition of h(k)), though the algebraic procedure to find it is a bit harder.
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