Spontaneous symmetry breaking in the SM

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SUMMARY

The discussion centers on spontaneous symmetry breaking in the Standard Model (SM) using a specific Lagrangian, \(\mathcal{L} = \frac{1}{2}(\partial_{\mu}\underline{\phi}).(\partial^{\mu}\underline{\phi}) + \frac{1}{2}\mu^{2}\underline{\phi}.\underline{\phi} - \frac{\lambda}{4}(\underline{\phi}.\underline{\phi})^{2} + \bar{\psi}(i\gamma . \partial )\phi - g\bar{\psi}(\phi_{1}+i\gamma^{5}\phi_{2})\psi\). The goal is to demonstrate that the classical equations of motion yield a vacuum that breaks symmetry spontaneously, leading to fermion mass proportional to coupling constant \(g\). Constructing the Hamiltonian from the Lagrangian is essential for identifying the lowest energy field configuration, which simplifies the solution process.

PREREQUISITES
  • Understanding of Lagrangian mechanics in quantum field theory
  • Familiarity with the concepts of spontaneous symmetry breaking
  • Knowledge of Hamiltonian formulation in field theory
  • Basic understanding of fermion fields and mass generation
NEXT STEPS
  • Study the Hamiltonian formulation of field theories
  • Research spontaneous symmetry breaking in the context of the Standard Model
  • Examine the derivation of mass terms for fermions in quantum field theory
  • Explore the role of the Higgs mechanism in mass generation
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The discussion is beneficial for theoretical physicists, graduate students in particle physics, and researchers focusing on quantum field theory and the Standard Model, particularly those interested in symmetry breaking and mass generation mechanisms.

AlphaNumeric
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[tex]\mathcal{L} = \frac{1}{2}(\partial_{\mu}\underline{\phi}).(\partial^{\mu}\underline{\phi}) + \frac{1}{2}\mu^{2}\underline{\phi}.\underline{\phi} - \frac{\lambda}{4}(\underline{\phi}.\underline{\phi})^{2} + \bar{\psi}(i\gamma . \partial )\phi - g\bar{\psi}(\phi_{1}+i\gamma^{5}\phi_{2})\psi[/tex]

where [tex]\underline{\phi} = \left( \begin{array}{c} \phi_{1} \\ \phi_{2} \end{array} \right)[/tex]

I've shown this Lagrangian is invariant under [tex]\phi_{1} \to \cos \alpha \phi_{1} - \sin \alpha \phi_{2}[/tex] [tex]\phi_{2} \to \sin \alpha \phi_{1} + \cos \alpha \phi_{2}[/tex] [tex]\psi \to \exp\left( -\frac{i \alpha \gamma^{5}}{2} \right)\psi[/tex]

The question then asks to show that the solution to the classical equations of motion with minimal energy lead to a vacuum which breaks the symmetry spontaneously. Then, to pick a suitable vacuum solution, and use it to show the fermion field acquires a mass proportional to g.

If someone could give me pointers in the right direction I've be very grateful. I've tried mucking about with the equations of motion for the phi's and psi's, but seem to going round in circles. Thanks :smile:
 
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Hi AlphaNumeric,

Since you are asked to find the classical lowest energy field configuration it makes sense to construct the Hamiltonian for your system. This step is essentially trivial since your Lagrangian is nice and simple in its time derivatives (note that I think you have a typo in the kinetic term for the dirac field, that [tex]\phi[/tex] should be a [tex]\psi[/tex]). I won't spoil it for you, but you will find that some terms in the Hamiltonian should obviously be zero in the lowest energy configuration. Once you set these terms to zero in your classical field equations, everything becomes simple and the solution will pop right out.
 

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