The one-loop correction in Lehmann-Kallen form

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SUMMARY

The discussion centers on the one-loop correction in the Lehmann-Kallen form as presented in Chapter 15 of Srednicki's "Quantum Field Theory". The participants analyze the transition from equation (15.12) to equation (15.13), specifically addressing the disappearance of the term ##\pi \delta(k^2+m^2)##. It is concluded that the modified equation should include a delta function term for consistency, particularly at ##s=m^2##, where additional conditions on ##\mathrm{Re}\Pi(-m^2)## and ##\mathrm{Im}\Pi(-m^2)## are necessary to cancel the delta function. The discussion emphasizes the importance of understanding the behavior of ##\rho(s)## and ##\mathrm{Im}\Pi(-s)## in the context of the integral limits.

PREREQUISITES
  • Understanding of quantum field theory concepts, particularly the Lehmann-Kallen representation.
  • Familiarity with Srednicki's "Quantum Field Theory", especially Chapter 15.
  • Knowledge of complex analysis as it pertains to physical equations.
  • Ability to interpret mathematical expressions involving delta functions and imaginary parts of functions.
NEXT STEPS
  • Study the implications of the Lehmann-Kallen representation in quantum field theory.
  • Review the derivation and applications of the delta function in quantum mechanics.
  • Examine the role of the imaginary part of the self-energy function, ##\mathrm{Im}\Pi(k^2)##, in scattering theory.
  • Explore the conditions under which ##\rho(s)## vanishes for different values of ##s## in quantum field calculations.
USEFUL FOR

Researchers and students in theoretical physics, particularly those focusing on quantum field theory and particle physics, will benefit from this discussion. It is especially relevant for those analyzing one-loop corrections and the properties of self-energy functions.

JILIN
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Hi.
I would like to ask a question about Chapter 15 in Srednicki's QFT book.

In chapter 15, after eq. (15.12), he compares eq. (15.12)
## \mathrm{Im}\bm{\Delta}(k^2)=\frac{\mathrm{Im}\Pi (k^2)}{(k^2+m^2-\mathrm{Re}\Pi (k^2))^2 + (\mathrm{Im}\Pi (k^2))^2}##
with eq. (15.8)
##\mathrm{Im}\bm{\Delta}(k^2)=\pi \delta(k^2+m^2)+\pi\rho(-k^2).##
Then he gets eq. (15.13)
##\pi \rho(s)=\frac{\mathrm{Im}\Pi (-s)}{(-s+m^2-\mathrm{Re}\Pi (-s))^2 + (\mathrm{Im}\Pi (-s))^2}.##
Why does ##\pi \delta(k^2+m^2)## disappears?
 
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(15.12) only applies if ##{\rm Im}\Pi(k^2)\ne0##. If ##{\rm Im}\Pi(k^2)=0##, then (15.11) applies.
 
Thanks, Avodyne.
But my question is the following one.

I think that eqs. (15.12) and (15.8) give
##\pi \rho (s) = \frac{\mathrm{Im}\Pi(-s)}{(k^2+m^2-\mathrm{Re}\Pi(-s))^2 + (\mathrm{Im}\Pi(-s))^2} - \pi \delta(-s+m^2),##
instead of eq. (15.13) in his text.
 
That makes no difference in 15.8, because the integral over ##s## starts at ##4m^2##.
 
Integral over ##s## in eq. (15.8) does not necessarily need to start at ##4m^2##.
It starts at ##4m^2## just because we know ##\rho(s)=0## for ##s<4m^2## (this is clearly seen around eq. (13.11) in chapter 13).
Thus, eq. (15.8) and also eq. (15.13) is valid for any ##s## (or any ##-k^2##), although we already know ##\rho(s)=0## for ##s<4m^2##.

In fact, he used eq. (15.13) for ##s<4m^2## in the discussion below eq. (15.13).
Here, he combined eq. (15.13) for ##s<4m^2## with the fact ##\rho(s)=0## for ##s<4m^2##.

My understanding is the following.
Eq. (15.13) should be
##\pi \rho (s) = \frac{\mathrm{Im}\Pi(-s)}{(-s+m^2-\mathrm{Re}\Pi(-s))^2+(\mathrm{Im}\Pi(-s))^2} - \pi \delta(s-m^2)##
(this is valid for any ##s##).
Next, we consider the region ##s<4m^2##.
Combining my modified eq. (15.13) with \rho(s)=0 for ##s<4m^2##, we get ##\mathrm{Im}\Pi(-s)=0## for ##s<4m^2##, which is the same conclusion in the book.
(For ##s \ne m^2##, we can drop the delta-function and the modified eq. (15.13) becomes same as that in the book.
However, we have to be slightly careful at ##s=m^2##.)
 
If you agree that ##\rho(s)=0## and ##{\rm Im}\Pi(-s)=0## for ##s<4m^2##, then your modified eq.(15.13) is not consistent, because the delta function does not vanish at ##s=m^2##, which is less than ##4m^2##.
 
I appreciate your kind discussion (at the same time I'm sorry that I'm slow to understand).

I agree that ##\rho(s)=0## and ##\mathrm{Im}\Pi(-s)=0## for ##4m^2>s \ne m^2##.
But at ##s=m^2##, I think that an additional condition ##\mathrm{Re}\Pi(-m^2)=0## is needed; this condition and ##\mathrm{Im}\Pi(-m^2)=0## can cancel the delta-function ##-\pi\delta(s-m^2)##.
Actually, in Fig. 14.5, ##\mathrm{Re}\Pi(-m^2)## looks zero.
 
Oh, finally I understand!
Thank you very much, Avodyne!
 

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