Why Shift ##z_0## by ##-i\epsilon## in Non-Convergent Integrals?

  • Thread starter Thread starter Jufa
  • Start date Start date
  • Tags Tags
    Integral
Click For Summary
SUMMARY

The discussion centers on the computation of the commutator ##[\phi(x), \phi^\dagger(y)]## for a non-relativistic field, specifically with the expression involving a spacelike vector ##z=x-y##. The integral derived from this computation does not converge, prompting the suggestion to shift ##z_0## by adding ##-i\epsilon## to ensure convergence. This technique allows for the limit ##\epsilon \rightarrow 0## to be taken, facilitating the calculation. The justification for this approach is rooted in Distribution theory, as established by Laurent Schwartz.

PREREQUISITES
  • Understanding of quantum field theory concepts, particularly commutators.
  • Familiarity with non-relativistic quantum mechanics, specifically the energy-momentum relation ##p^0 = \frac{\vec{p}^2}{2m}##.
  • Knowledge of complex analysis, particularly the handling of divergent integrals.
  • Basic principles of Distribution theory as formulated by Laurent Schwartz.
NEXT STEPS
  • Study the principles of Distribution theory to understand the justification for shifting integrals.
  • Learn about the implications of non-convergent integrals in quantum field theory.
  • Explore the mathematical techniques for regularization of divergent integrals.
  • Investigate the role of causality in quantum field theories and its violation in non-relativistic contexts.
USEFUL FOR

Physicists, particularly those specializing in quantum field theory, mathematicians interested in Distribution theory, and researchers dealing with non-convergent integrals in theoretical physics.

Jufa
Messages
101
Reaction score
15
Homework Statement
I encounter a divergent integral when computing a commutator of two fields in quantum field theory homework
Relevant Equations
##\phi = \int \frac{dp^3}{(2\pi)^3}e^{-ipx}\hat{a}(\vec{p})##
I am asked to compute ##[\phi(x), \phi^\dagger(y)]## , with
##\phi = \int \frac{dp^3}{(2\pi)^3}e^{-ipx}\hat{a}(\vec{p})## and with z=x-y a spacelike vector. And show that this commutator does not vanish, which means that for this non-relativsitic field i.e. with ##p^0 = \frac{\vec{p}^2}{2m}## causality is violated.

After two straightforward steps I get to this

##[\phi(x), \phi^\dagger(y)] = \int \frac{dp^3}{(2\pi)^3}e^{-i \frac{\vec{p}^2}{2m}z_0}e^{i\vec{p}\cdot\vec{z}} ##

It is self-evident that this integral does not converge and, therefore, I have been suggested to shift ##z_0## by adding to it a quantity ##-i\epsilon##. This makes the integral convergent and allows one to take the limit ##\epsilon \rightarrow 0## in the end, which works perfectly.
But why are we allowed to do this? To me it seems that the integral I am asked to compute is just (I would end the problem here and say that it is not zero, just what I was demanded to prove) divergent and that this trick allows to compute not the requested integral but a different one.

I need some help on this.

Thanks in advance.
 
Physics news on Phys.org

Similar threads

Replies
4
Views
665
  • · Replies 2 ·
Replies
2
Views
2K
Replies
27
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
Replies
1
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K