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Vacuum expectation value: Wikis


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Quantum field theory
Feynmann Diagram Gluon Radiation.svg
Feynman diagram
History of...
Effective field theory
Expectation value
Faddeev–Popov ghosts
Feynman diagram
LSZ reduction formula
Partition function
Vacuum state
Wick's theorem
Wightman axioms

In quantum field theory the vacuum expectation value (also called condensate or simply VEV) of an operator is its average, expected value in the vacuum. The vacuum expectation value of an operator O is usually denoted by \langle O\rangle. One of the best known examples of the vacuum expectation value of an operator leading to a physical effect is the Casimir effect.

This concept is important for working with correlation functions in quantum field theory. It is also important in spontaneous symmetry breaking. Examples are:

The observed Lorentz invariance of space-time allows only the formation of condensates which are Lorentz scalars and have vanishing charge. Thus fermion condensates must be of the form \langle\overline\psi\psi\rangle, where ψ is the fermion field. Similarly a tensor field, Gμν, can only have a scalar expectation value such as \langle G_{\mu\nu}G^{\mu\nu}\rangle.

In some vacua of string theory, however, non-scalar condensates are found. If these describe our universe, then Lorentz symmetry violation may be observable.

See also

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