Understanding Spontaneous Symmetry Breaking in Quantum Field Theory

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Is there a reason why we have to expand a field ψ about the true vacuum |Ω>? Can't we just do field theory about ψ=0 instead of about ψ=<Ω|ψ|Ω>?

Also, I'm a bit confused about other fields. For the E&M potential, under the true vacuum, wouldn't we need to expand about A=<Ω|A|Ω> instead of A=0?

Also, how do we find the true vacuum anyhow? The way that it seems to be done is to take the derivative of the potential V, and set it equal to zero. The potential V usually has a negative mass or something shifting the true vacuum away from ψ=0. Is this an approximation? Don't we have to take the derivative of the effective potential Veff instead of V?

And how can one show that two derivatives of Veff gives the mass generated? I thought to get the mass generated, you have to shift the fields, and identify the coefficients of terms proportional to the square of the field. But a paper I'm reading claims you can just take two derivatives of Veff to get the mass generated?
 
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Yes, you have to use V_eff. "The way it seems to be done..." Are you referring to some specific book? There are presentations of varying level of precision.
 
DrDu said:
Yes, you have to use V_eff. "The way it seems to be done..." Are you referring to some specific book? There are presentations of varying level of precision.

Most textbooks just state V(\phi)=-\mu^2\phi^2+λ\phi^4 as the beginning potential which leads to spontaneous symmetry breaking.

V is not the effective potential, but the potential appearing in the Lagrangian, which is just the tree-level effective potential.

Something feels rotten about just stating that the potential is V(\phi)=-\mu^2\phi^2+\lambda \phi^4. Spontaneous symmetry breaking depends crucially on the sign of μ2, but how do we know the sign of μ2? Aren't these couplings supposed to depend on scale? Is there a scale where the coupling goes back to being negative?

I can see how λ must always be positive at any scale or else your theory doesn't have a ground state at all. But I'm not sure how we know the sign of μ2 by just looking at the bare Lagrangian.
 
I just now saw your reply.
Zee, Quantum field theory in a nutshell explains that the effective potential has to be used to determine whether a symmetry is broken or not.
 
Insights auto threads is broken atm, so I'm manually creating these for new Insight articles. Towards the end of the first lecture for the Qiskit Global Summer School 2025, Foundations of Quantum Mechanics, Olivia Lanes (Global Lead, Content and Education IBM) stated... Source: https://www.physicsforums.com/insights/quantum-entanglement-is-a-kinematic-fact-not-a-dynamical-effect/ by @RUTA
If we release an electron around a positively charged sphere, the initial state of electron is a linear combination of Hydrogen-like states. According to quantum mechanics, evolution of time would not change this initial state because the potential is time independent. However, classically we expect the electron to collide with the sphere. So, it seems that the quantum and classics predict different behaviours!
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