Saturday, 30 August 2014

quantum field theory - Complex integration by shifting the contour


In section 12.11 of Jackson's Classical Electrodynamics, he evaluates an integral involved in the Green function solution to the 4-potential wave equation. Here it is:


dk0eik0z0k20κ2



where k and z0 are real constants.


Jackson considers two open contours: one above and one below the real axis. I understand that in order to use Jordan's lemma, when z0<0 we have to close the contour in the upper half of the complex plane whereas if z0>0 we have to close the contour in the lower half plane.


What I don't understand is why it's OK to consider contours above and below the real axis when the original integral is along the real axis. As I understand it, the necessity to deal with poles like this also arises a lot in QFT, so perhaps it is well understood from that point of view.



Answer




Suppose we want to analyse the problem of a forced harmonic oscillator. Denote as ϕ(t) the time dependent position of the oscillator. The oscillator experiences two forces, the spring force kϕ(t) and an external force Fext(t). Newton's law says


F(t)=ma(t)kϕ(t)+Fext(t)=m¨ϕ(t)Fext(t)/m=¨ϕ(t)+(k/m)ϕ(t)j(t)=¨ϕ(t)+ω20ϕ(t)


where ω0 is the free oscillation frequency and j(t)Fext/m. We use the following Fourier transform convention: f(t)=ω˜f(ω)eiωtdω2π˜f(ω)=tf(t)eiωt dt.


With this convention on Eq. (1), and defining ω±±ω0, we find ˜ϕ(ω)=˜j(ω)ω20ω2=˜j(ω)(ωω+)(ωω). From Eq. (2) we see that the Green's function is ˜G(ω)=1(ωω+)(ωω) which has poles on the real axis. If we want to compute ϕ(t) we do a Fourier transform


ϕ(t)=ω˜j(ω)eiωt(ωω+)(ωω)dω2π=ωeiωt˜j(ω)˜G(ω)dω2π.



This integral is tricky because of the poles on the axis. The solution everyone knows is to push the poles off the axis by adding an imaginary part to ω±, or by moving the contour above or below the real axis, but what does this actually mean physically? How do we choose which direction to push the poles or move the contour?



In a real system, we always have some damping. In our oscillator model, this could come in the form of a velocity dependent friction Ffriction=μ˙ϕ(t). Defining 2β=μ/m, the equation of motion becomes


¨ϕ(t)+2β˙ϕ(t)+ω20ϕ(t)=j(t).


Fourier transforming everything again leads to Eq. (2) but now with ω±=±ω0+iβ where ω0=ω01(β/ω0)2.


Therefore, we see that adding damping moves the poles a bit toward the origin along the real axis, but also gives them a positive imaginary component. In the limit of small damping (i.e. βω0), we find ω0ω0. In other words, the frequency shift of the poles due to the damping is small. So let's ignore that and focus on the added imaginary part.


Ok, suppose we want to do the integral () in the case that j(t) is a delta function at t=0. In that case, ˜j=1 (I'm ignoring units) and we have ϕ(t)=ωeiωt(ωω+)(ωω)dω2π As you noted, for t<0 you have to close the contour in the lower plane in order to use Jordan's lemma. There aren't any poles in the lower half plane, so we get ϕ(t<0)=0. This makes complete sense: the driving force is a delta function at t=0 and there shouldn't be any response of the system before the driving happens. This means that our introduction of friction imposed a causal boundary condition to the system! For t>0, you close in the upper half plane where there are poles, and so you get some response out of the integral.



In many cases, you don't naturally have damping in the system. For example, the Green's function from the question,  dk0eik0z0k20κ2 doesn't have any damping and thus the poles sit on the real axis. So what you do is just bump the contour a bit up or down, or equivalently add ±iβ to the poles (most people write iϵ instead of iβ), then do the integral, and finally take β0. In doing this, you're solving the problem in the presence of damping (or anti-damping), and then taking the damping to zero in the end to recover the no-damping case.


Choosing to push the contour up or down, or equivalently choosing the sign of ±iβ, corresponds to imposing either friction or anti-friction, causal or anti-causal boundary conditions. If you pick the "causal" boundary condition, you find that the response of the system to a delta function in time and space is an outgoing spherical wave which starts at the delta function source. This gives you the so-called "retarded Green's function". If you pick the other condition, you find that the solution for a point source is actually an incoming spherical wave which converges right onto the point of the source. This gives you the so-called "Advanced Green's function".



The thing is, you can solve a problem using either Green's function. You're "allowed" to push the contour up or down (or add +iβ or iβ to the poles) because you invented that as a trick to do the integral; it's not representing a real factor in your physical system. Of course, in problems where there is damping, the choice is made for you. When you have damping, you can't have fields at infinity; they'd be damped away by the time they interact with your sources.


I hope this was helpful, and I really hope if someone finds mistakes they'll jump in and fix 'em.


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