Graduate Validity of Scalar Field Lagrangian with Linear and Quadratic Terms

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SUMMARY

The discussion centers on the validity of a scalar field Lagrangian with linear and quadratic terms, specifically the form $$\mathscr{L} = \phi \square \phi + c_1 \phi + c_2 \phi^2$$. It is established that the inclusion of a linear term, represented by $$c_1 \phi$$, results in an unbounded energy from below, making it unsuitable for perturbation theory. To resolve this issue, a shift in the field configuration, $$\phi \rightarrow \phi - \frac{c_1}{2c_2}$$, is proposed, effectively eliminating the linear term and reverting to a stable free theory. The discussion highlights that the quadratic term's coefficient, $$c_2$$, must maintain the correct sign to ensure bounded energy.

PREREQUISITES
  • Understanding of scalar field theory
  • Familiarity with Lagrangian mechanics
  • Knowledge of perturbation theory in quantum field theory
  • Basic concepts of Hamiltonian stability
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  • Study the implications of linear terms in scalar field Lagrangians
  • Learn about the Klein-Gordon Lagrangian and its applications
  • Research perturbation theory and its requirements for stable vacuum states
  • Examine the role of potential densities in quantum field theory
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The discussion is beneficial for theoretical physicists, particularly those specializing in quantum field theory, as well as students seeking to understand the implications of scalar field Lagrangians and their stability conditions.

Gaussian97
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TL;DR
Is a term proportional to ##\phi## valid in a scalar Lagrangian?
Hi, if I want to construct the most general Lagrangian of a single scalar field up to two fields and two derivatives, I usually see that is
$$\mathscr{L} = \phi \square \phi + c_2 \phi^2$$ i.e. the Klein-Gordon Lagrangian.
My question is, would be valid the Lagrangian
$$\mathscr{L} = \phi \square \phi + c_1 \phi + c_2 \phi^2$$
?
 
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With a linear term, the energy is not bounded from below. So this is usually not considered. This is a problem for applying perturbation theory, this indicates that one is expanding around a field configuration that cannot be used as a vacuum. So one then shifts ## \phi \rightarrow \phi - \frac{c_1}{2c_2} ## which gets rid of the linear term.
 
nrqed said:
With a linear term, the energy is not bounded from below.
A linear term shifts the location of the minimum of the potential and shifts the overall potential by a finite constant. (speaking loosely about potential densities as potentials)
 
With the linear term and the quadratic term the energy is still bounded from below provided ##c_2## has the "right sign". So it's a fine theory (as ##\phi^3## theory is not though it's treated at length in some textbooks to have a simple model to explain perturbative renormalization theory, e.g., in Collin's Renormalization; adding a ##\phi^4## term makes it again a theory with the Hamiltonian bounded from below).

For the free field here you can just introduce a new field shifted field as explained in #2, and you are back at the usual free theory.
 
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Likes dextercioby
Ok! Thank you!
 

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