In
quantum field theory, the vacuum expectation value (VEV) of an
operator is its average or
expectation value in the
vacuum. The vacuum expectation value of an operator
O is usually denoted by
One of the most widely used examples of an observable physical effect that results from the vacuum expectation value of an operator is the
Casimir effect.
This concept is important for working with
correlation functions in
quantum field theory. In the context of
spontaneous symmetry breaking, an operator that has a vanishing expectation value due to symmetry can acquire a nonzero vacuum expectation value during a
phase transition
In physics, chemistry, and other related fields like biology, a phase transition (or phase change) is the physical process of transition between one state of a medium and another. Commonly the term is used to refer to changes among the basic Sta ...
. Examples are:
*The
Higgs field has a vacuum expectation value of 246
GeV.
This nonzero value underlies the
Higgs mechanism of the
Standard Model. This value is given by
, where ''M
W'' is the mass of the W Boson,
the reduced
Fermi constant, and the weak isospin coupling, in natural units. It is also near the limit of the most massive nuclei, at v = 264.3
Da.
*The
chiral condensate in
quantum chromodynamics, about a factor of a thousand smaller than the above, gives a large effective mass to
quarks, and distinguishes between phases of
quark matter. This underlies the bulk of the mass of most hadrons.
*The
gluon condensate in
quantum chromodynamics may also be partly responsible for masses of hadrons.
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
, where
ψ is the fermion field. Similarly a
tensor field,
Gμν, can only have a scalar expectation value such as
.
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
*
Correlation function (quantum field theory)
*
Dark energy
*
Spontaneous symmetry breaking
*
Vacuum energy
*
Wightman axioms
References
External links
*
Quantum field theory
Standard Model
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