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In particle and condensed matter physics, Nambu-Goldstone bosons are bosons that appear in models with spontaneously broken symmetry.

In certain supersymmetric models, "Goldstone fermions," or "Goldstinos" also appear. So do sgoldstinos. The simplest model with a Goldstone boson is as follows:

We have a complex scalar field φ (phi), with the constraint that φ*φ=k2. One way to get a constraint of that sort is by including a potential

\lambda^2(\phi^*\phi - k^2)^2 \,

and taking the limit as λ goes to infinity. The field can be redefined to give a real scalar, θ, without a constraint by using

\phi = k e^{i\theta} \,

where θ is the Goldstone boson (actually kθ is) with the Lagrangian density given by:

{\mathcal L}=-\frac{1}{2}(\partial^\mu \phi^*)\partial_\mu \phi +m^2 \phi^* \phi = -\frac{1}{2}(-ik e^{-i\theta} \partial^\mu \theta)(ik e^{i\theta} \partial_\mu \theta) + m^2 k^2=-\frac{k^2}{2}(\partial^\mu \theta)(\partial_\mu \theta) + m^2 k^2.

Note that the constant term m2k2 has no physical significance and the other term is simply the kinetic term for a massless scalar. In general the Goldstone boson is always massless, and parametrises the curve of possible vacuum states.

A somewhat simpler but more detailed presentation of the same concepts is presented in the article on the Yukawa interaction.

See also


Bosons | Quantum field theory

 

This article is licensed under the GNU Free Documentation License. It uses material from the "Nambu-Goldstone boson".

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