In theoretical physics, more specifically in quantum field theory and supersymmetry, supersymmetric Yang–Mills, also known as super Yang–Mills and abbreviated to SYM, is a supersymmetric generalization of Yang–Mills theory, which is a gauge theory that plays an important part in the mathematical formulation of forces in particle physics. It is a special case of 4D N = 1 global supersymmetry.
Super Yang–Mills was studied by Julius Wess and Bruno Zumino in which they demonstrated the supergauge-invariance of the theory and wrote down its action,[1] alongside the action of the Wess–Zumino model, another early supersymmetric field theory.
The treatment in this article largely follows that of Figueroa-O'Farrill's lectures on supersymmetry[2] and of Tong.[3]
While N = 4 supersymmetric Yang–Mills theory is also a supersymmetric Yang–Mills theory, it has very different properties to
l{N}=1
l{N}=2
d=4
A first treatment can be done without defining superspace, instead defining the theory in terms of familiar fields in non-supersymmetric quantum field theory.
The base spacetime is flat spacetime (Minkowski space).
G
ak{g}
The field content then consists of
ak{g}
A\mu
ak{g}
\Psi
ak{g}
D
For gauge-invariance, the gauge field
A\mu
\Psi
\Psi
\Psi=(λ,\barλ)
λ
\Psi
When
G=U(1)
A\mu
\Phi
D
The field strength tensor is defined as usual as
F\mu\nu:=\partial\muA\nu-\partial\nuA\mu
The Lagrangian written down by Wess and Zumino is then
l{L}=-
1 | |
4 |
F\mu\nuF\mu\nu-
i | |
2 |
\bar\Psi\gamma\mu\partial\mu\Psi+
1 | |
2 |
D2.
This can be generalized to include a coupling constant
e
\propto\varthetaF\mu\nu*F\mu\nu
*F\mu\nu
*F\mu\nu=
1 | |
2 |
\epsilon\mu\nu\rho\sigmaF\rho\sigma.
\epsilon\mu\nu\rho\sigma
\Psi
λ
This can be viewed as a supersymmetric generalization of a pure
U(1)
In full generality, we must define the gluon field strength tensor,
F\mu\nu=\partial\muA\nu-\partial\nuA\mu-i[A\mu,A\nu]
D\muλ=\partial\muλ-i[A\mu,λ].
To write down the action, an invariant inner product on
ak{g}
B( ⋅ , ⋅ )
B
Tr
ak{g}
Supersymmetric Yang–Mills then readily generalizes from supersymmetric Maxwell theory. A simple version is
SSYM=\intd4xTr\left[-
1 | |
4 |
F\mu\nuF\mu\nu-
1 | |
2 |
\bar\Psi\gamma\muD\mu\Psi\right]
while a more general version is given by
The base superspace is
l{N}=1
V
The theory is defined in terms of a superfield arising from taking covariant derivatives of
V
W\alpha=-
1 | |
4 |
2}l{D} | |
l{\barD | |
\alpha |
V
\tau=
\vartheta | |
2\pi |
+
4\pii | |
e |
where h.c. indicates the Hermitian conjugate of the preceding term.
For non-abelian gauge theory, instead define
W\alpha=-
1 | |
8 |
\barl{D}2(e-2Vl{D}\alphae2V)
\tau=
\vartheta | |
2\pi |
+
4\pii | |
g |
For the simplified Yang–Mills action on Minkowski space (not on superspace), the supersymmetry transformations are
\delta\epsilonA\mu=\bar\epsilon\gamma\mu\Psi
\delta\epsilon\Psi=-
1 | |
2 |
F\mu\nu\gamma\mu\nu\epsilon
\gamma\mu\nu=
1 | |
2 |
(\gamma\mu\gamma\nu-\gamma\nu\gamma\mu)
For the Yang–Mills action on superspace, since
W\alpha
W\alpha
\intd2\theta
An important observation is that the Wess–Zumino gauge is not a supersymmetric gauge, that is, it is not preserved by supersymmetry. However, it is possible to do a compensating gauge transformation to return to Wess–Zumino gauge. Then, after a supersymmetry transformation and the compensating gauge transformation, the superfields transform as
\deltaA\mu=\epsilon\sigma\mu\barλ+λ\sigma\mu\bar\epsilon,
\deltaλ=\epsilonD+(\sigma\mu\nu\epsilon)F\mu\nu
\deltaD=i\epsilon
\mu\partial | |
\sigma | |
\mu |
\barλ-i\partial\muλ\bar\sigma\mu\bar\epsilon.
See also: supersymmetric gauge theory.
The preliminary theory defined on spacetime is manifestly gauge invariant as it is built from terms studied in non-supersymmetric gauge theory which are gauge invariant.
The superfield formulation requires a theory of generalized gauge transformations. (Not supergauge transformations, which would be transformations in a theory with local supersymmetry).
Such a transformation is parametrized by a chiral superfield
\Omega
V\mapstoV+i(\Omega-\Omega\dagger).
V
\Omega
V
A\mu
\Omega
\omega
A\mu\mapstoA\mu-2\partial\mu(Re\omega)=:A\mu+\partial\mu\alpha.
W\alpha=-
1 | |
4 |
\barl{D}2l{D}\alphaV,
The chiral superfield is adjoint valued. The transformation of
V
e2V\mapsto
-2i\Omega\dagger | |
e |
e2Ve2i\Omega
V
The chiral superfield
W\alpha=-
1 | |
8 |
\barl{D}2(e-2Vl{D}\alphae2V)
W\alpha\mapstoe2i\OmegaW\alphae-2i\Omega
As a classical theory, supersymmetric Yang–Mills theory admits a larger set of symmetries, described at the algebra level by the superconformal algebra. Just as the super Poincaré algebra is a supersymmetric extension of the Poincaré algebra, the superconformal algebra is a supersymmetric extension of the conformal algebra which also contains a spinorial generator of conformal supersymmetry
S\alpha
Conformal invariance is broken in the quantum theory by trace and conformal anomalies.
While the quantum
l{N}=1
The
U(1)
l{N}=1
See also: Super QCD.
Matter can be added in the form of Wess–Zumino model type superfields
\Phi
\Phi\mapsto\exp(-2iq\Omega)\Phi
\Phi\dagger\Phi
\Phi\daggere2q\Phi.
This gives a supersymmetric analogue to QED. The action can be written
SSMaxwell+\intd4x\intd4\theta\Phi\daggere2qV\Phi.
For
Nf
Nf
\Phii
SSMaxwell+\intd4x\intd4\theta
\dagger | |
\Phi | |
i |
2qiV | |
e |
\Phii.
However, for a well-defined quantum theory, a theory such as that defined above suffers a gauge anomaly. We are obliged to add a partner
\tilde\Phi
\Phi
SSQED=SSMaxwell+\intd4x\intd4\theta
\dagger | |
\Phi | |
i |
2qiV | |
e |
\Phii+
\dagger | |
\tilde\Phi | |
i |
-2qiV | |
e |
\tilde\Phii.
For non-abelian gauge, matter chiral superfields
\Phi
R
\Phi\mapsto\exp(-2i\Omega)\Phi
The Wess–Zumino kinetic term must be adjusted to
\Phi\daggere2V\Phi
Then a simple SQCD action would be to take
R
SSYM+\intd4xd4\theta\Phi\daggere2V\Phi
More general and detailed forms of the super QCD action are given in that article.
See also: Fayet–Iliopoulos D-term.
When the center of the Lie algebra
ak{g}