Vector Supermultiplet

In theoretical physics, a supermultiplet is a representation of a supersymmetry algebra.

Then a superfield is a field on superspace which is valued in such a representation. Naïvely, or when considering flat superspace, a superfield can simply be viewed as a function on superspace. Formally, it is a section of an associated supermultiplet bundle.

Phenomenologically, superfields are used to describe particles. It is a feature of supersymmetric field theories that particles form pairs, called superpartners where bosons are paired with fermions.

These supersymmetric fields are used to build supersymmetric quantum field theories, where the fields are promoted to operators.

History

Superfields were introduced by Abdus Salam and J. A. Strathdee in their 1974 articl
Supergauge Transformations
Operations on superfields and a partial classification were presented a few months later by Sergio Ferrara, Julius Wess and Bruno Zumino i
Supergauge Multiplets and Superfields

Naming and classification

The most commonly used supermultiplets are vector multiplets, chiral multiplets (in 4D N=1 supersymmetry for example), hypermultiplets (in 4D N=2 supersymmetry for example), tensor multiplets and gravity multiplets. The highest component of a vector multiplet is a gauge boson, the highest component of a chiral or hypermultiplet is a spinor, the highest component of a gravity multiplet is a graviton. The names are defined so as to be invariant under dimensional reduction, although the organization of the fields as representations of the Lorentz group changes.

The use of these names for the different multiplets can vary in literature. A chiral multiplet (whose highest component is a spinor) may sometimes be referred to as a ''scalar multiplet'', and in N=2 SUSY, a vector multiplet (whose highest component is a vector) can sometimes be referred to as a chiral multiplet.

Superfield in d = 4, N = 1 supersymmetry

A general complex superfield $\Phi(x, \theta, \bar \theta)$ in $d = 4, \mathcal = 1$ supersymmetry can be expanded as

:$\Phi(x, \theta, \bar\theta) = \phi(x) + \theta\chi(x) + \bar\theta \bar\chi'(x) + \bar \theta \sigma^\mu \theta V_\mu(x) + \theta^2 F(x) + \bar \theta^2 \bar F'(x) + \bar\theta^2 \theta\xi(x) + \theta^2 \bar\theta \bar \xi' (x) + \theta^2 \bar\theta^2 D(x)$,

where $\phi, \chi, \bar \chi' , V_\mu, F, \bar F', \xi, \bar \xi', D$ are different complex fields. This is not an irreducible supermultiplet, and so different constraints are needed to isolate irreducible representations.

Chiral superfield

A (anti-)chiral superfield is a supermultiplet of $d=4, \mathcal = 1$ supersymmetry.

In four dimensions, the minimal $\mathcal=1$ supersymmetry may be written using the notion of superspace. Superspace contains the usual space-time coordinates $x^$, $\mu=0,\ldots,3$, and four extra fermionic coordinates $\theta_\alpha,\bar\theta^\dot\alpha$ with $\alpha, \dot\alpha = 1,2$, transforming as a two-component (Weyl) spinor and its conjugate.

In N=1 supersymmetry in 3+1D, a chiral superfield is a function over chiral superspace. There exists a projection from the (full) superspace to chiral superspace. So, a function over chiral
superspace can be pulled back to the full superspace. Such a function $\Phi(x, \theta, \bar\theta)$ satisfies the covariant constraint $\overline\Phi=0$, where $\bar D$ is the covariant derivative, given in index notation as
:$\bar D_\dot\alpha = -\bar\partial_\dot\alpha - i\theta^\alpha \sigma^\mu_\partial_\mu.$

A chiral superfield $\Phi(x, \theta, \bar\theta)$ can then be expanded as

:$\Phi (y , \theta ) = \phi(y) + \sqrt \theta \psi (y) + \theta^2 F(y),$
where $y^\mu = x^\mu + i \theta \sigma^\mu \bar$. The superfield is independent of the 'conjugate spin coordinates' $\bar\theta$ in the sense that it depends on $\bar\theta$ only through $y^\mu$. It can be checked that $\bar D_\dot\alpha y^\mu = 0.$

The expansion has the interpretation that $\phi$ is a complex scalar field, $\psi$ is a Weyl spinor. There is also the auxiliary complex scalar field $F$, named $F$ by convention: this is the F-term which plays an important role in some theories.

The field can then be expressed in terms of the original coordinates $(x,\theta, \bar \theta)$ by substituting the expression for $y$:
:$\Phi(x, \theta, \bar\theta) = \phi(x) + \sqrt \theta \psi (x) + \theta^2 F(x) + i\theta\sigma^\mu\bar\theta\partial_\mu\phi(x) - \frac\theta^2\partial_\mu\psi(x)\sigma^\mu\bar\theta - \frac\theta^2\bar\theta^2\square\phi(x).$

Antichiral superfields

Similarly, there is also antichiral superspace, which is the complex conjugate of chiral superspace, and antichiral superfields.

An antichiral superfield $\Phi^\dagger$ satisfies $D \Phi^\dagger = 0,$ where
:$D_\alpha = \partial_\alpha + i\sigma^\mu_\bar\theta^\dot\alpha\partial_\mu.$

An antichiral superfield can be constructed as the complex conjugate of a chiral superfield.

Actions from chiral superfields

For an action which can be defined from a single chiral superfield, see Wess-Zumino model.

Vector superfield

The vector superfield is a supermultiplet of $\mathcal = 1$ supersymmetry.

A vector superfield (also known as a real superfield) is a function $V(x,\theta,\bar\theta)$ which satisfies the reality condition $V = V^\dagger$. Such a field admits the expansion

:$V = C + i\theta\chi - i \overline\overline + \tfrac\theta^2(M+iN)-\tfrac\overline(M-iN) - \theta \sigma^\mu \overline A_\mu +i\theta^2 \overline \left( \overline + \tfrac\overline^\mu \partial_\mu \chi \right) -i\overline^2 \theta \left(\lambda + \tfrac\sigma^\mu \partial_\mu \overline \right) + \tfrac\theta^2 \overline^2 \left(D + \tfrac\Box C\right).$

The constituent fields are
* Two real scalar fields $C$ and $D$
* A complex scalar field $M + iN$
* Two Weyl spinor fields $\chi_\alpha$ and $\lambda^\alpha$
* A real vector field (gauge field) $A_\mu$

Their transformation properties and uses are further discussed in supersymmetric gauge theory.

Using gauge transformations, the fields $C, \chi$ and $M + iN$ can be set to zero. This is known as Wess-Zumino gauge. In this gauge, the expansion takes on the much simpler form
:$V_ = \theta\sigma^\mu\bar\theta A_\mu + \theta^2 \bar\theta \bar\lambda + \bar\theta^2 \theta \lambda + \frac\theta^2\bar\theta^2 D.$
Then $\lambda$ is the superpartner of $A_\mu$, while $D$ is an auxiliary scalar field. It is conventionally called $D$, and is known as the D-term.

Scalars

A scalar is never the highest component of a superfield; whether it appears in a superfield at all depends on the dimension of the spacetime. For example, in a 10-dimensional N=1 theory the vector multiplet contains only a vector and a Majorana–Weyl spinor, while its dimensional reduction on a d-dimensional torus is a vector multiplet containing d real scalars. Similarly, in an 11-dimensional theory there is only one supermultiplet with a finite number of fields, the gravity multiplet, and it contains no scalars. However again its dimensional reduction on a d-torus to a maximal gravity multiplet does contain scalars.

Hypermultiplet

A hypermultiplet is a type of representation of an extended supersymmetry algebra, in particular the matter multiplet of ''N''=2 supersymmetry in 4 dimensions, containing two complex scalars ''A''_''i'', a Dirac spinor ψ, and two further auxiliary complex scalars ''F''_''i''.

The name "hypermultiplet" comes from old term "hypersymmetry" for ''N''=2 supersymmetry used by ; this term has been abandoned, but the name "hypermultiplet" for some of its representations is still used.

See also

* Supersymmetric gauge theory
* D-term
* F-term

References

*
* Stephen P. Martin. ''A Supersymmetry Primer'', arXiv:hep-ph/9709356 .
* Yuji Tachikawa. ''N=2 supersymmetric dynamics for pedestrians'', arXiv:1312.2684.
*

{{Supersymmetry topics
Supersymmetry