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Quantum Field Theory I

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1.2. MANY-BODY QUANTUM MECHANICS 25<br />

Remark: Even if it is not necessary for our purposes, it is hard to resist<br />

the temptation to discuss perhaps the most important pair interaction in the<br />

non-relativistic quantum physics, namely the Coulomb interaction. This is of<br />

general interest not only because of the vast amount of applications, but also<br />

due to the fact that the standard way of dealing with the Coulomb potential in<br />

the p-representation involves a mathematical inconsistency. The way in which<br />

this inconsistency is treated is in a sense generic, and therefore quite instructive.<br />

1<br />

|⃗x−⃗y|<br />

In the x-representation V Coulomb (⃗x,⃗y) = e2<br />

4π<br />

(which is relevant in the case with no external field)<br />

V Coulomb (⃗p 1 ,⃗p 2 ,⃗p 3 ,⃗p 4 ) = e2<br />

4π<br />

∫<br />

, i.e. in the p-representation<br />

d 3 x<br />

(2π) 3 d 3 y<br />

(2π) 3 1<br />

|⃗x−⃗y| ei(⃗p4−⃗p1).⃗x e i(⃗p3−⃗p2).⃗y<br />

(for the sake of brevity, we use the Heaviside-Lorentz convention in electrodynamics<br />

and = 1 units in QM). This integral, however, is badly divergent. The<br />

integrand simply does not drop out fast enough for |⃗x| → ∞ and |⃗y| → ∞.<br />

Instead of giving up the use of the p-representation for the Coulomb potential<br />

energy, it is a common habit to use a dirty trick. It starts by considering the<br />

Yukawa (or Debey) potential energy V Debey (⃗x,⃗y) = e2 1<br />

4π |⃗x−⃗y| e−µ|⃗x−⃗y| , for which<br />

the p-representation is well defined and can be evaluated readily 34<br />

V Debey (⃗p 1 ,⃗p 2 ,⃗p 3 ,⃗p 4 ) = e2 1 1<br />

4π 2π 2 µ 2 +(⃗p 4 −⃗p 1 ) 2δ(⃗p 1 +⃗p 2 −⃗p 3 −⃗p 4 )<br />

Now comes the dirty part. It is based on two simple (almost trivial) observations:<br />

the first is that V Coulomb (⃗x,⃗y) = lim µ→0 V Debey (⃗x,⃗y), and the second is that the<br />

limit lim µ→0 V Debey (⃗p 1 ,⃗p 2 ,⃗p 3 ,⃗p 4 ) is well defined. From this, a brave heart can<br />

easily conclude that V Coulomb (⃗p 1 ,⃗p 2 ,⃗p 3 ,⃗p 4 ) = e2 1<br />

8π<br />

δ(⃗p 3 (⃗p 4−⃗p 1) 2 1 +⃗p 2 −⃗p 3 −⃗p 4 ).<br />

And, believe it or not, this is indeed what is commonly used as the Coulomb<br />

potential energy in the p-representation.<br />

Needless to say, from the mathematical point of view, this is an awful heresy<br />

(called illegal change of order of a limit and an integral). How does it come<br />

about that physicists are working happily with something so unlawful<br />

The most popular answer is that the Debey is nothing else butascreenedCoulomb,<br />

and that in most systems this is more realistic than the pure Coulomb. This is<br />

a reasonable answer, with a slight off-taste of a cheat (the limit µ → 0 convicts<br />

us that we are nevertheless interested in the pure Coulomb).<br />

Perhaps a bit more fair answer is this one: For µ small enough, one cannot say<br />

experimentally the difference between the Debey and Coulomb. And the common<br />

plausible belief is that measurable outputs should not depend on immeasurable<br />

inputs (if this was not typically true, the whole science would hardly be possible).<br />

If the mathematics nevertheless reveals inconsistencies for some values of<br />

a immeasurable parameter, one should feel free to choose another value, which<br />

allows for mathematically sound treatment.<br />

34 ∫<br />

For⃗r = ⃗x−⃗y, V Yukawa (⃗p 1 ,⃗p 2 ,⃗p 3 ,⃗p 4 ) = e2 d<br />

3 r d 3 y 1<br />

4π (2π) 3 (2π) 3 r e−µr e i(⃗p 4−⃗p 1 ).⃗r e i(⃗p 3−⃗p 2 +⃗p 4 −⃗p 1 ).⃗y<br />

= e2<br />

4π δ(⃗p 1 +⃗p 2 − ⃗p 3 −⃗p 4 ) ∫ d 3 r e −µr<br />

(2π) 3 e r i⃗q.⃗r , where ⃗q = ⃗p 4 − ⃗p 1 . The remaining integral in<br />

∫ 1<br />

the spherical coordinates: ∞<br />

(2π) 2 0 dr r ∫ e−µr 1<br />

−1 dcosϑ eiqrcosϑ = 1 ∫ 1 ∞<br />

2π 2 q 0 dr e−µr sinqr.<br />

For the integral I = ∫ ∞<br />

0 dr e−µr sinqr one obtains by double partial integration the relation<br />

I = q<br />

µ 2 − q2<br />

µ 2 I, and putting everything together, one comes to the quoted result.

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