Conventional renormalization to order in the coupling or loops?

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SUMMARY

Conventional renormalization requires computing scattering amplitudes using bare quantities such as ##\lambda_0## and ##m_0##, followed by expressing these in terms of physical quantities like ##m## and ##\lambda##. When calculating the scattering amplitude to ##O(\lambda_0^2)## and first order in loops, it is essential to determine whether to compute mass and coupling to second order in the coupling or first order in loop corrections. This process is governed by the perturbation theory's order, ensuring that divergences are managed through renormalization conditions, leveraging the graph theoretic structure of Feynman integrals. For further insights, refer to Zimmerman's Forest formula and the introductory lecture notes available at the provided arXiv link.

PREREQUISITES
  • Understanding of conventional renormalization techniques
  • Familiarity with scattering amplitudes and perturbation theory
  • Knowledge of Feynman integrals and their graph theoretic structure
  • Basic grasp of loop corrections in quantum field theory
NEXT STEPS
  • Study Zimmerman's Forest formula for deeper insights into renormalization
  • Explore advanced topics in perturbation theory and their applications
  • Learn about the implications of loop corrections on scattering amplitudes
  • Review Part 1 of the lecture notes on arXiv for foundational concepts
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Quantum field theorists, physicists specializing in particle physics, and researchers interested in advanced renormalization techniques and scattering amplitude calculations.

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In conventional renormalization one is first supposed to compute a scattering amplitude of interest in terms of bare quantities ##\lambda_0, m_0...##, then compute these bare quantities in terms of physical quantities, i.e. ##m(m_0,\lambda_0,...), \lambda(m_0, \lambda_0,...)## and substitute these back into the scattering amplitude. The amplitude should now be finite.

That is all nice, but suppose one computes the scattering amplitude to ##O(\lambda_0^2 )## and to first order in loops. To be consistent, should one now compute the mass and coupling to second order in the coupling or first order in loop corrections?

And why?
 
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At each order in perturbation theory you make the bare/physical replacement to the order previously computed. These should leave diveregences at the current order that can be absorbed by invoking the renormalization conditions.

It works because of the graph theoretic structure of Feynman integrals. Look for explanations of Zimmerman's Forest formula.

Part 1 of these lecture notes gives an nice intro and some references: https://arxiv.org/abs/1004.3462
 

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