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GaugeFixing

Gauge fixing is a procedure in gauge theories to remove redundant degrees of freedom associated with gauge invariance. In many theories, fields are defined up to a gauge transformation, so many field configurations describe the same physical situation. To perform calculations, one imposes a gauge condition that selects a unique representative from each equivalence class of gauge-related configurations.

Common gauges include the Lorenz gauge ∂^μ A_μ = 0, the Coulomb gauge ∇·A = 0, and the temporal

In the quantization of gauge theories, gauge fixing is essential for defining the path integral and propagators.

A significant complication is the Gribov problem: in non-Abelian theories, a given gauge condition can intersect

In lattice gauge theory, gauge invariance is maintained exactly, and gauge fixing is optional; it is commonly

See also: Faddeev–Popov procedure, BRST symmetry, Gribov ambiguity, lattice gauge theory, Dirac's constrained quantization.

gauge
A^0
=
0.
In
non-Abelian
gauge
theories,
gauge
fixing
is
more
subtle
because
the
space
of
gauge
orbits
is
more
intricate.
The
Faddeev-Popov
procedure
inserts
a
delta
function
enforcing
the
gauge
condition
and
a
determinant
to
compensate
for
overcounting.
This
leads
to
the
introduction
of
ghost
fields,
which
are
needed
to
preserve
unitarity
and
gauge
invariance
of
physical
observables,
at
least
perturbatively.
BRST
symmetry
provides
a
formal
framework
for
these
structures.
Observables
that
are
gauge
invariant
do
not
depend
on
the
choice
of
gauge,
but
gauge-dependent
quantities
such
as
propagators
do.
the
same
gauge
orbit
multiple
times,
making
global
gauge
fixing
ambiguous
and
affecting
nonperturbative
results.
used
to
study
gauge-variant
quantities
and
to
define
certain
correlators,
with
Landau
or
Coulomb
gauges
among
popular
choices.