Give mass to a massless scalar field in 1+1, Higgs like?

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SUMMARY

The discussion centers on the feasibility of introducing mass to a massless scalar field in 1+1 spacetime through interaction with another field, potentially invoking a Higgs-like mechanism. The Mermin-Wagner theorem is highlighted as a critical consideration, stating that continuous symmetries cannot be spontaneously broken at finite temperatures in dimensions of 2 or less. This theorem implies that massless Goldstone bosons would lead to infrared divergences, thus preventing spontaneous symmetry breaking in such low-dimensional systems.

PREREQUISITES
  • Understanding of quantum field theory principles
  • Familiarity with the Mermin-Wagner theorem
  • Knowledge of scalar fields and their properties
  • Basic concepts of symmetry breaking in physics
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  • Research the implications of the Mermin-Wagner theorem on field theories
  • Explore the characteristics of scalar fields in quantum field theory
  • Investigate Higgs mechanisms in higher-dimensional spacetimes
  • Study the role of Goldstone bosons in spontaneous symmetry breaking
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The discussion is beneficial for theoretical physicists, particularly those focusing on quantum field theory, symmetry breaking, and the implications of dimensionality in particle physics.

Spinnor
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Is it possible to have a free massless scalar field in 1+1 spacetime and then add another field of the right type which interacts with some adjustable strength with the massless field to give mass to the massless field? Is there a Higgs-like mechanism in 1+1 spacetime?

Thanks for any help!
 
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Have you looked at the Mermin Wagner theorem?
 
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thierrykauf said:
Have you looked at the Mermin Wagner theorem?

Thank you! From the wiki article,

"
In quantum field theory and statistical mechanics, the Mermin–Wagner theorem (also known as Mermin–Wagner–Hohenberg theorem or Coleman theorem) states that continuous symmetries cannot be spontaneously broken at finite temperature in systems with sufficiently short-range interactions in dimensions d ≤ 2. Intuitively, this means that long-range fluctuations can be created with little energy cost and since they increase the entropy they are favored.

This is because if such a spontaneous symmetry breaking occurred, then the corresponding Goldstone bosons, being massless, would have an infrared divergent correlation function.

The absence of spontaneous symmetry breaking in d ≤ 2 dimensional systems was rigorously proved by Sidney Coleman (1973) in quantum field theory and by David Mermin, Herbert Wagner and Pierre Hohenberg in statistical physics. That the theorem does not apply to discrete symmetries can be seen in the two-dimensional Ising model. "
 
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