Weak Interactions — Howard Georgi — draft - March 25, 2010 —
22
well, as follows:
s
→
D
φ
(
g
-
1
)
s ,
η
R
→
D
L
(
g
-
1
)
η
R
,
η
L
→
D
R
(
g
-
1
)
η
L
.
(1b.1.3)
Note the switching of
L
↔
R
for the fermion sources, because the fermions source terms are like
mass terms that couple fields of opposite chirality. Now if the regularization and renormalization
respect the symmetry, the vacuum amplitude,
Z
(
s, η,
η
) will also be invariant under (1b.1.3).
Generators —
T
a
It is often convenient to use the infinitesimal version of (1b.1.2) and (1b.1.3), in terms of the
generators,
T
a
,
δφ
=
i
a
T
a
φ
φ ,
δψ
L
=
i
a
T
a
L
ψ
L
,
δψ
R
=
i
a
T
a
R
ψ
R
,
δs
=
i
a
T
a
φ
s ,
δη
R
=
i
a
T
a
L
η
R
,
δη
L
=
i
a
T
a
R
η
L
.
(1b.1.4)
The
T
a
j
for
j
=
φ
,
L
and
R
, are generators of the representation of the Lie algebra of
G
, corre-
sponding to the representations,
D
j
(
g
-
1
) =
e
i
a
T
a
j
.
(1b.1.5)
A sum over repeated
a
indices is assumed. Often we will drop the subscript, and let the reader
figure out from the context which representation we are discussing.
Gauge Symmetry
In order to discuss the conserved Noether currents associated with a symmetry of the quantum
field theory as composite operators, it is useful to convert the global symmetry, (1b.1.4), into a
gauge symmetry, that is a symmetry in which the parameters can depend on space-time,
a
→
a
(
x
)
.
(1b.1.6)
To do this, we must introduce a set of “gauge fields”, which in this case will be classical fields, like
the other sources. Call these fields,
