Spectral weight function and the mass shift of a scalar field

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Discussion Overview

The discussion revolves around the application of the Kallen-Lehmann spectral representation to determine the mass shift of a scalar field, specifically exploring the relationship between the physical mass and the bare mass of a particle.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant suggests that the spectral representation could be used to find the mass shift \(\delta m^2 = m^2 - m_0^2\) of a scalar field.
  • Another participant expresses doubt, stating that deriving the spectral density function requires using the actual mass \(m\) rather than the bare mass \(m_0\), implying that the pole of the full propagator is determined by the free single-particle propagator's pole location.
  • A later reply indicates that it can indeed be done, referencing a specific page in a document.
  • One participant apologizes for potentially misleading the discussion but acknowledges their initial uncertainty.
  • Another participant clarifies that they were considering the same idea and found it unproductive, leading them to seek input from the forum.

Areas of Agreement / Disagreement

Participants express differing views on whether the spectral representation can be used to determine the mass shift, with some uncertainty and exploration of the topic evident in the responses.

Contextual Notes

The discussion includes assumptions about the relationship between physical and bare masses, and the implications of using different mass definitions in the spectral representation, which remain unresolved.

Rocky Raccoon
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In the Kallen-Lehmann spectral representation (http://en.wikipedia.org/wiki/Källén–Lehmann_spectral_representation) the interacting propagator is given as a weighted sum over free propagators. The pole of the integracting propagator is, of course, given by p^2=m^2, m being the physical mass of the particle.

Could this spectral representation be used to find the mass shift \delta m^2 = m^2 - m_0^2 of a scalar field (m_0 is the bare mass of the noninteracting particle)?

Thanks
 
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I think not but I'm not sure. In order to derive the spectral density function formula you are required to insert a basis of energy eigenstates which forces you to use the actual mass m and not the bare mass m_0. So that the free single particle propagator has the same pole location as the full propagator.

You might think that since the spectral density is a sum over poles you would find that taking this sum would yield a "total pole" and the location of the pole would be different from the single particle propagator. However the location of the pole of the full propagator is completely determined by the location of the pole of the free single-particle propagator (expressed in terms of the physical mass). Usually the full propagator is written in terms of the spectral density the following way to make this idea more explicit.

<br /> \Delta(k^2) = \frac{1}{k^2+m^2-i\epsilon}+\int^\infty_{(2m)^2}d\mu^2\rho(\mu^2) \frac{1}{k^2+\mu^2-i\epsilon}<br />

The integral of the poles gives something like a branch cut rather than contributing to the pole of the free propagator.
 
Interesting. Sorry I led you astray!
 
You didn't lead me astray, I was thinking the same thing as you and it got me nowhere so I tried PF :)
 

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