Spontaneous symmetry breaking
Suppose we generalise the Klein-Gordon Lagrangian density to the case where the scalar field

is complex, or equivalently is a pair of real scalar fields

and

such that

or

The Lagrangian density would then be

We can take

and

a.s independent, just as easily as

and

.
The state of lowest energy of a system is known as the ground state, or in field theory terminology, the vacuum.
In the above Lagrangian the
potential energy density

is a minimum when

But suppose we modify it to (

a real constant)
![LaTeX Code: <BR>\\begin{array}{l}<BR> V\\left( {\\Phi ,\\Phi ^+} \\right)=\\frac{m^2}{2\\phi _0^2 }\\left[ {\\Phi ^+\\Phi <BR>-\\phi _0^2 } \\right]^2=V\\left( {\\Phi ,\\Phi ^+} \\right)= \\\\ <BR> =\\frac{m^2}{2\\phi _0^2 }\\left( {\\Phi ^+\\Phi } \\right)^2-m^2\\Phi ^+\\Phi <BR>+\\frac{1}{2}m^2\\phi _0^2 \\\\ <BR> \\end{array}<BR>](latex_images/16/1664113-13.png)
The vacuum state

now occurs when

, which defines a
circle in

space, i.e. there are an infinity of vacuums. The Lagrangian density has a U(1) symmetry.
Nature chooses one of these as the physical vacuum and "breaks'" this symmetry. This phenomenon is known as spontaneous symmetry breaking.
How does spontaneous symmetry breaking help? Suppose we expand the field

around the chosen vacuum state, by writing

Substituting into
![LaTeX Code: <BR>L\\left( {\\Phi ,\\Phi ^+} \\right)=\\partial _\\mu \\Phi ^+\\partial ^\\mu \\Phi <BR>-\\frac{m^2}{2\\phi _0^2 }\\left[ {\\Phi ^+\\Phi -\\phi _0^2 } \\right]^2<BR>](latex_images/16/1664113-19.png)
and doing the algebra, the Lagrangian density now becomes
![LaTeX Code: <BR>L\\left( {\\Phi ,\\Phi ^+} \\right)=\\partial _\\mu \\chi ^+\\partial ^\\mu \\chi <BR>+\\partial _\\mu \\psi ^+\\partial ^\\mu \\psi -\\frac{m^2}{2\\phi _0^2 }\\left[ <BR>{\\sqrt 2 \\phi _0 \\chi +\\frac{\\chi ^2}{2}+\\frac{\\psi ^2}{2}} \\right]^2<BR>](latex_images/16/1664113-20.png)
Pick out the "free particle" pieces by writing

we have

is a complicated ''self" interaction amongst the fields, which we will leave aside.
We can interpret

by comparing with the Klein-Gordon Lagrangian density
![LaTeX Code: <BR><BR>L=\\frac{1}{2}\\left[ {\\partial _\\mu \\phi \\partial ^\\mu \\phi -m^2\\phi ^2} <BR>\\right]<BR>](latex_images/16/1664113-25.png)
We can see that we have a massive, spinless scalar boson field

of mass

. This is called a Higgs boson.
A massless, spinless scalar boson field

. This is called a Goldstone boson.
The Higgs boson is like a fluctuation around the vacuum point in the direction in which the potential density increases. The Goldstone boson is like a fluctuation in the direction in winch the potential density is flat.
At this point, we seem to have introduced new fields into our toy theory and not gained a lot. However, the full theory mast be locally gauge invariant, which is not yet the case.
For local
gauge invariance we require invariance under

and the introduction of a gauge field

, transforming as

with the Lagrangian looking like
where as before
Again the vacuum state is when

, and since

is arbitrary, we can choose it so that

is real, breaking the symmetry.