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Under this transformation the wavefunction changes as <math>\psi\rightarrow e^{iq\theta}\psi</math> and <math>\bar{\psi}\rightarrow e^{-iq\theta}\bar{\psi}</math> and so clearly: | Under this transformation the wavefunction changes as <math>\psi\rightarrow e^{iq\theta}\psi</math> and <math>\bar{\psi}\rightarrow e^{-iq\theta}\bar{\psi}</math> and so clearly: | ||
::<math>\mathcal{L}\rightarrow\bar{\mathcal{L}}=e^{-iq\theta}\bar{\psi}\left(i\gamma^\mu \partial_\mu-m\right)e^{iq\theta}\psi=e^{-iq\theta}e^{iq\theta}\bar{\psi}\left(i\gamma^\mu \partial_\mu-m\right)=\mathcal{L}</math> | ::<math>\mathcal{L}\rightarrow\bar{\mathcal{L}}=e^{-iq\theta}\bar{\psi}\left(i\gamma^\mu \partial_\mu-m\right)e^{iq\theta}\psi=e^{-iq\theta}e^{iq\theta}\bar{\psi}\left(i\gamma^\mu \partial_\mu-m\right)\psi=\mathcal{L}</math> | ||
==See also== | ==See also== |
Revision as of 20:03, 25 July 2012
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A global symmetry is a symmetry that holds at all points in the spacetime under consideration, as opposed to a local symmetry which varies from point to point.
Global symmetries require conservation laws, but not forces, in physics.
An example of a global symmetry is the action of the (for a constant - making it a global transformation) group on the Dirac Lagrangian:
Under this transformation the wavefunction changes as and and so clearly:
See also
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