Scalar propagator for lightlike separation

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SUMMARY

The discussion centers on calculating the prefactor for the delta function in the context of a scalar propagator for lightlike separations in two-dimensional space. The integral presented, \(\int \frac{dk}{\sqrt{k^2+m^2}} e^{i k x - i \sqrt{k^2+m^2} t}+e^{i k x + i \sqrt{k^2+m^2} t}\), is crucial for deriving the propagator in position space. The challenge arises when determining the prefactor for \(\delta(t-x)\) specifically for lightlike separations, where traditional methods of setting either \(x\) or \(t\) to zero do not apply. The need for a clear approach to handle lightlike separation in this context is emphasized.

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  • Understanding of scalar field theory
  • Familiarity with propagators in quantum field theory
  • Knowledge of Lorentz invariance principles
  • Proficiency in evaluating integrals involving exponential functions
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  • Research the derivation of scalar propagators in quantum field theory
  • Learn about the treatment of lightlike separations in propagator calculations
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The discussion is beneficial for theoretical physicists, particularly those specializing in quantum field theory, as well as graduate students seeking to deepen their understanding of propagators and lightlike separations.

bnado
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Hello everybody.
I have a free scalar in two dimensions. I know that its propagator will diverge for lightlike separations, that is t= ±x. I have to find the prefactor for this delta function, and I don't know how to do this.
How do I see from, for example, \int \frac{dk}{\sqrt{k^2+m^2}} e^{i k x - i \sqrt{k^2+m^2} t}+e^{i k x + i \sqrt{k^2+m^2} t} what I get as a prefactor for my \delta (t-x)?

Normally when calculating this integral we set either x or t to 0, depending on whether the separation is timelike or spacelike, to then restore Lorentz invariance after the integral is solved. What can I do in the case of lightlike separation?
Thanks
 
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For some reason I can't see your formulas...
 
weird. The latex code for the first formula is
\int \frac{dk}{\sqrt{k^2+m^2}} e^{i k x - i \sqrt{k^2+m^2} t}+e^{i k x + i \sqrt{k^2+m^2} t}
and it's just the integral that gives you the propagator in position space.
the second one is just \delta (t-x)
 

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