How does a virtual particle becomes a point interaction?

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SUMMARY

The discussion centers on the mathematical justification for the Taylor expansion of a propagator of a heavy particle, specifically in the context of quantum field theory. The propagator is expressed as an integral involving the mass M of the particle, and the expansion is valid for distances greater than the inverse mass (x > M-1). The first term of the expansion yields a delta function point interaction, while subsequent terms represent derivatives of the delta function. The participants emphasize the need for a rigorous mathematical foundation for this expansion, particularly when considering contributions from high-energy virtual modes.

PREREQUISITES
  • Understanding of quantum field theory concepts
  • Familiarity with propagators and their mathematical representations
  • Knowledge of Taylor series expansions in mathematical physics
  • Experience with integrals in the context of Fourier transforms
NEXT STEPS
  • Study the derivation of propagators in quantum field theory textbooks such as "Schweber" and "Pauli Lectures"
  • Investigate the mathematical foundations of delta functions and their derivatives
  • Learn about the implications of high-energy virtual particles in quantum field interactions
  • Explore the role of the mass parameter in propagator behavior and its physical significance
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This discussion is beneficial for physicists, particularly those specializing in quantum field theory, as well as graduate students seeking to deepen their understanding of propagators and point interactions in theoretical physics.

jim burns
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If you want to show that a propagator of a heavy particle reduces to a point interaction at distances large compared to the inverse mass of the particle by Taylor expanding the propagator (for simplicity take 1-dimension):

$$G(x)=\int^\infty_{-\infty} \frac{dk}{2\pi} \frac{e^{-ikx}}{k^2+M^2}=
\int^\infty_{-\infty} \frac{dk}{2\pi} \frac{e^{-ikx}}{M^2(1+\frac{k^2}{M^2})}=
\int^\infty_{-\infty} \frac{dk}{2\pi} \frac{e^{-ikx}}{M^2} (1-\frac{k^2}{M^2}+...(-1)^n\left(\frac{k^2}{M^2}\right)^n)
$$

then how does one justify this expansion when k>M? The first term gives the δ(x) point interaction, and the rest give derivatives of δ(x). But how is the Taylor expansion in the integrand justified?

It seems that the answer must have to do with the fact that x>M-1 in the exponential?

Also, a related question: if you have an arbitrary function

$$f(x)=\int^\infty_{-\infty} \frac{dk}{2\pi} e^{-ikx} f(k)$$

and specify that x>M-1, does that tell you anything about the contribution of f(k) for k>M to f(x)?
 
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Why are you doing the expansion in the first place? You can just calculate the propagator in position representation. You find it explicitly done in older textbooks on quantum field theory like Schweber or in the Pauli Lectures.
 
I was following some lectures (McGreevy's notes - if anyone's interested it's page 16 of http://physics.ucsd.edu/~mcgreevy/s15/215C-2015-lectures.pdf ) and they showed the expansion so I thought it was important to understand why it could be done mathematically.

I was thinking that physically high energy virtual modes don't contribute to the propagator at long time scales, so that you should be able to ignore the integral at high k when your time argument of the propagator in position space is long (>M-1). However, I don't see the justification mathematically.
 

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