Symmetry breaking with Lagrangian

Question

I have been studying the spontaneous symmetry braking from Zee (Quantum Field theory ) and found in the page 224, he wrote the lagrangian as
$$\mathcal{L}= \frac{1}{2}\{ λ (∂φ)^2 + μ^2φ^ 2\} − \frac{\lambda}{4}(φ^4)$$

But according to sclar field theory I got from Ryder $$\mathcal{L}=\frac{1}{2}\{ λ (∂φ)^2 + μ^2φ^ 2\} − \frac{\lambda}{4!}(φ^4)$$ Am I doing wrong?

My another question is, the potential we have inserted in the Lagrangian is look like Mexican hat. What conditions will change the shape of the potential? Symmetry breaking means ,changing the Lagrangian with kinetic energy terms?

Answer 1

The difference between the two is in the potential term (Ryder divides by 4! whereas Zee divides by 4). The physics doesn't change, provided the potential term has a nonzero minima. Really, that's where spontaneous symmetry breaking happens for a scalar field.

You have your Lagrangian $$ \mathcal{L} = \frac{1}{2}\left(\partial^{\mu}\varphi\partial_{\mu}\varphi-\mu^{2}\varphi^{2}\right)-V(\varphi). $$ If it has a nonzero vacuum energy, then $V(\varphi)\not=0$ for any $\varphi$. If this happens, it breaks symmetry since the vacuum is nonunique (egads!).

We find this happening if $\varphi_{0}$ satisfies $V'(\varphi_{0})=0$ but $V(\varphi_{0})\not=0$.

Addendum: The potential $V(\varphi)=c_{1}\varphi^{2}+c_{2}\varphi^{4}$ would experience spontaneous symmetry breaking, for nonzero constants $c_{1}$, $c_{2}$...but if $c_{1}=0$ -- as your model has -- there is no symmetry breaking.