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Supersymmetry. Theory, Experiment, and Cosmology

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Example of supersymmetric SU(Nc) with Nf flavors. The rˆole of R-symmetries 209

We take this opportunity to note that, in order to integrate out a heavy degree of freedom in a supersymmetric way, one has to work at the level of the superpotential, and not at the level of the Lagrangian (potential).

8.4Example of supersymmetric SU (Nc) with Nf flavors. The rˆole of R-symmetries

We use the methods introduced in the preceding sections to study the case of supersymmetric QCD, or more generally of a SU (Nc) gauge theory with Nf flavors of quarks and antiquarks. As we will see, the discussion depends on whether the number of flavors Nc is smaller or larger than the number of colors.

8.4.1Nf < Nc

If at some large scale M0, the gauge coupling has a perturbative value g, then the running coupling g(µ) evolves, at one loop, as

1

=

 

1

+

 

b

ln

 

µ

(8.45)

g2(µ)

g2

8π2

M0

 

 

 

 

where b = 3Nc − Nf is the coe cient of the one-loop beta function (see Chapter 9). Due to asymptotic freedom, or rather asymptotic slavery (b > 0), it explodes at a scale

Λ = M0 e8π2/(bg2).

(8.46)

Above the scale Λ, we have a theory of elementary excitations, the quarks and antiquarks, whereas, below, the e ective theory is a theory of mesons. We wish to study the symmetries of the original theory in order to identify the dynamical interactions of the meson fields. Under independent global rotations of left and right chiralities, SU (Nf )L × SU (Nf )R, the quark superfields Q transform as (Nf , 1) (since they

¯

include the left-handed quark field), whereas the antiquark superfields Q transform

¯

as (1, Nf ) (they include the right-handed chirality). Similarly, baryon number con-

¯

servation is associated with a global U (1)B symmetry: Q (resp. Q) has charge +1 (resp. 1).

We now identify a R-symmetry which is nonanomalous. We have seen in (8.7) that the fermionic component of a superfield of R-charge r (the charge of its scalar

 

¯

 

component) transforms with charge r − 1. Thus if Q and Q transform with same

R-charge r, then the quark and antiquark fields transform as:

 

ψQ

= ei(r−1)α ψQ

 

ψ ¯

= ei(r−1)α ψ ¯ .

(8.47)

Q

Q

 

Also gaugino fields transform with charge +1 (see equation (C.77) of Appendix C):

λ = eλ.

(8.48)

Nf )C

210 Dynamical breaking. Duality

One computes the mixed U (1) − SU (Nc) − SU (Nc) triangle anomalies. The goal is to choose r in order to cancel these mixed anomalies. Writing T a (resp. ta) the generators of SU (Nc) in the adjoint (resp. fundamental) representation, we have:

Tr T aT b = C2(G) δab

C2(G) = Nc,

(8.49)

Tr tatb = T (R) δab

T (R) =

1

.

(8.50)

2

 

 

 

 

Then the condition of anomaly cancellation reads:

Nc + 12 (r − 1)Nf + 12 (r − 1)Nf = 0.

Hence

r =

Nf − Nc

.

(8.51)

 

Nf

 

The meson superfields Mij of the e ective theory transform under the nonanomalous U (1)R symmetry as:

j

¯

αj

→ e

2i

Nf −Nc

α

j

 

(8.52)

Nf

.

Mi

≡ Qαi Q

 

 

 

 

Mi

We now use the full symmetries in order to extract the dynamical interactions of these e ective mesonic degrees of freedom. They are described by a superpotential Wdyn(Mij ). Since this superpotential cannot have a matrix structure – indeed it must be invariant under SU (Nf )L × SU (Nf )R – it must depend on det(M ). We summarize in Table 8.2 the transformation properties of the di erent, fundamental or e ective, fields.

Since Wdyn(M ) must have R-charge +2, we conclude that it must be proportional to (det M )1/(Nf −Nc). Using dimensional analysis ([W ] = 3 and [det M ] = 2Nf ) and the fact that the only dynamical scale available is the scale Λ, we conclude that the dynamical e ective potential is

Wdyn(M ) = CNc,Nf

1

 

Λ3Nc−Nf

Nc−Nf

(8.53)

det M

 

 

where CNc,Nf is a dimensionless constant. This result may be tested in several di erent regimes and the constant computed to depend on Nc and Nf as CNc,Nf = (Nc

1/(Nc−Nf ), with C constant (see Exercise 3).

Table 8.2

 

SU (Nf )L

SU (Nf )R

U (1)B

U (1)R

Q

Nf

1

+1

(Nf − Nc)/Nf

¯

1

¯

1

(Nf − Nc)/Nf

Q

Nf

M

Nf

¯

0

2(Nf − Nc)/Nf

Nf

det M

1

1

0

2(Nf − Nc)

Example of supersymmetric SU(Nc) with Nf flavors. The rˆole of R-symmetries 211

In the special case Nf = Nc 1, we may then write (8.53) as

Wdyn(M ) = C

Λ

b

 

b

 

 

 

 

 

CM0

2

2

 

 

=

 

e8π

/g ,

(8.54)

det M

det M

where we have used (8.46). We recognize in the last factor the standard one-instanton contribution. Indeed, a direct instanton calculation provides the same answer and allows us to compute the remaining constant: C = 1 in the DR scheme [163].

Finally, taking Nf = 0 yields Wdyn(M ) = Λ3. This is obviously related to gaugino condensation: the dynamical potential being a function of λλ alone, dimensional

analysis imposes that Wdyn(M ) λλ3 . It

follows from (8.27) and the remark below

8π

2

 

2

(M0) , i.e. Λ

3

 

it that Wdyn(M ) is proportional to M0 exp

 

/Ncg

 

 

.

8.4.2 Nf = Nc or Nc + 1

Let us start with Nf = Nc. Then, according to Table 8.2, the quark superfields Q

¯

and Q have vanishing R-charge and it is not possible to use them only to write a superpotential of R-charge 2. However, there are now enough flavors to be able to form baryonic states:

B = α1···αNc Qα11 · · · QαNc Nc

 

 

 

 

¯

 

 

¯α11

¯αNc Nc

.

 

 

 

B = α1

···αNc Q

 

 

· · · Q

 

 

 

Since we may write in shortened

notation B = det[Q

], where [Q ] is a N

c ×

N

 

 

¯

αi

 

 

 

αi

αi

 

f

¯

 

 

 

 

 

 

 

 

 

 

square matrix and similarly B = det[Q ], we see that the low energy fields are not

independent:

 

 

 

 

 

 

 

 

 

 

 

¯

 

 

 

¯

αj

 

j

].

(8.55)

BB = det[QαiQ

 

] = det[Mi

[335] has, however, argued that this relation is only valid at the classical level. At the quantum level, he proposes to include a nonperturbative contribution:

j

¯

2Nc

,

(8.56)

det[Mi

] − BB = Λ

 

where Λ is the dynamical scale.

One may first check that the new term Λ2Nc has the right dimension (2Nc) and R-charge (0). But the main argument in favour of this addition is that it yields the right theory when one flavor decouples. Let us see this in detail. As discussed above in Section 8.3.4, we make the Nf th flavor decouple by introducing the following tree level term in the superpotential:

¯

αNf

.

(8.57)

Wtree = m QαNf Q

 

212 Dynamical breaking. Duality

We expect that the theory at scales much below m is supersymmetric SU (Nc) with Nc 1 flavors. Thus the low energy superpotential should simply read, according to (8.53),

˜2Nc+1

 

 

Λ

 

(8.58)

W detNc1 M

,

˜

 

 

 

 

 

 

where Λ is the dynamical scale of this e ective theory with Nc 1 flavors. It can be

easily related to Λ by matching the two theories at scale m: since

0 =

1

+

b

ln

Λ

,

g2(m)

8π2

m

 

 

 

 

 

1

 

˜

 

˜

 

0 =

+

b

ln

Λ

,

g2(m)

8π2

m

 

 

 

 

where b = 2Nc is the one-loop beta function coe cient of the theory with Nc fla-

˜

 

for the theory with Nc 1 flavors,

vors and b = 2Nc + 1 is the same coe cient

we have

 

 

 

 

˜2Nc+1

= mΛ

2Nc

.

(8.59)

Λ

 

To extract the low energy theory, we must place ourselves in the F -flat direction cor-

responding to QαNf

 

¯

αNf

 

 

 

 

 

 

 

 

¯αNf

 

= mQαNf , this di-

and Q

 

. Since for example dWtree/dQ

 

 

 

 

 

 

¯αNf

 

 

 

possibly

 

Q

 

 

¯

αNf

= 0). Hence

rection correspondsj to QαNf = Q = 0 (but

 

αNf

Q

 

 

N

 

 

 

 

 

¯

= 0 and det M = detNc1 M × MNf

f

. Then, the quantum con-

B = B = MNf

 

straint (8.56) yields M

Nf

= Λ2Nc / det

Nc1

M and we obtain from (8.57) and (8.59)

 

 

Nf

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

mΛ

2Nc

 

˜2Nc+1

 

 

 

 

Wtree = mMNf Nf =

 

=

Λ

 

 

 

 

,

 

(8.60)

detNc1 M

detNc1

M

 

 

 

 

 

 

 

 

 

 

 

in agreement with (8.58).

Another nontrivial check is provided by the ’t Hooft anomaly condition (see Section 8.3.3 above). The complete global symmetry SU (Nf = Nc)L × SU (Nf = Nc)R × U (1)B × U (1)R is partially broken by the vacua which satisfy the quantum constraint (8.56). The ’t Hooft consistency condition is all the more useful that the residual

j

2

j

 

 

 

 

 

=

 

¯

 

= 0,

 

 

B

B

symmetry is richer. One may for example consider the vacuum

 

 

 

 

Mi

= Λ δi . The symmetry is then SU (Nf = Nc)V × U (1)B × U (1)R. The quantum

numbers of the fundamental fermion fields (quarks ψ

Q

, antiquarks ψ ¯

and gauginos

 

 

 

 

 

Q

 

 

 

 

 

λ) as well as composite fermion fields (supersymmetric partners of the meson scalars

ψ

M

, baryons ψ

B

and antibaryons ψ ¯ ) are given in Table 8.3.

 

 

B

We note that among the e ective degrees of freedom, the mesons form an adjoint representation of dimension Nf2 1 of SU (Nf = Nc)V : one component of the matrix Mij is not independent because of the quantum constraint (8.56) which fixes det M .

Example of supersymmetric SU(Nc) with Nf flavors. The rˆole of R-symmetries 213

Table 8.3

 

SU (Nf = Nc)V

U (1)B

U (1)R

ψQ

Nf

+1

1

ψQ¯

Nf

1

1

λ

1

0

+1

ψM

Nf2 1

0

1

ψB

1

Nf

1

ψB¯

1

−Nf

1

One may then compute (see Exercise 4) the following mixed anomalies using either the fundamental degrees of freedom or the composite degrees of freedom of the low energy theory. The two results coincide:

SU (Nf ) − SU (Nf ) − U (1)R

−Nf

 

U (1)B − U (1)B − U (1)R

2Nf2

(8.61)

U (1)R − U (1)R − U (1)R

− Nf2 + 1 .

 

In the case where Nf = Nc + 1, the (anti)baryon fields carry a flavor index:

Bi = ij1···jNc α1

¯

Bi = ij1···jNc α1

···αNc Qα1j1

· · · QαNc jNc

 

¯α1j1

¯

αNc jNc

.

···αNc Q

· · · Q

 

The following superpotential

 

 

 

W =

1

det M − BiMij B¯j

(8.62)

Λb

allows us to recover the quantum constraint (8.56) when decoupling one flavor: it corresponds to the F -flatness condition for the decoupled flavor. Again, one may check in this case the ’t Hooft consistency conditions.

8.4.3Nf > Nc + 1: nonabelian electric–magnetic duality

When one reaches the value Nf = Nc + 2 and beyond, one encounters a growing disagreement between the computation of anomalies from the fundamental fields and from the system of baryons and mesons. This is a sign that one is misidentifying the e ective theory.

214 Dynamical breaking. Duality

 

˜

= Nf − Nc indices could be

We note, however, that baryon fields, having Nc

˜

 

interpreted as bound states of Nc component fields which we note q:

 

Bi1···iN˜c α1···αN˜c qα1i1 · · · qαN˜c iN˜c ,

(8.63)

 

¯

and similarly for B. This has led [336] to propose that supersymmetric QCD with Nc

colors and Nf

flavors could be described, for Nf ≥ Nc + 2 as supersymmetric QCD

˜

j

with Nc colors, Nf flavors of quark and antiquark supermultiplets and a field Mi

() which is a gauge singlet coupling to the quarks throughQαiQ¯αj

W =

1

 

µ q¯αiMij qαj .

(8.64)

As we will see, the relation between these two theories is somewhat reminiscent of the electric–magnetic duality discussed in Section 4.5.2 of Chapter 4: the original SU (Nc)

˜

theory provides the electric description whereas the SU (Nc) theory is the equivalent magnetic formulation. This is why Seiberg has called this relation the nonabelian electric–magnetic duality.

One may first check that this is indeed a duality. If we start with the latter theory and perform another duality transformation, one obtains supersymmetric QCD with

˜

 

 

¯αi

, and the singlet fields Mi

j

and Mi

j

Nf − Nc = Nc colors, Nf flavors Qαi and Q

 

 

( qαiq¯αj ) with superpotential

 

 

 

 

 

 

 

 

 

 

,

 

1

 

j

 

i 1 ¯αi

 

j

 

 

 

 

W =

 

 

 

M

 

 

 

 

M

 

 

 

 

 

µ Mi

 

+ µ˜ Q

 

Qαj .

 

(8.65)

 

 

,j

,i

 

,

The F -flatness condition for M ensures that M = 0 and thus a vanishing superpotential. We recover the original theory.

Again, ’t Hooft consistency condition provides a highly nontrivial check on the conjecture. The quantum numbers of the various superfields are given in Table 8.46. Using this information, on may for example compute the U (1)R3 anomaly in the

original picture (Nc2 1 gauginos of charge +1, Nf quarks ψQ and antiquarks ψQ¯

˜

˜ 2

1 gauginos of charge

of charge Nc/Nf 1 = −Nc/Nf ) or in the dual picture (Nc

˜

2

fermions ψM of charge

+1, Nf quarks ψq and antiquarks ψq¯ of charge −Nc/Nf , Nf

1 2Nc/Nf ). In both cases one finds Nc2 1 2Nc4/Nf2.

Let us complicate somewhat the picture by noting that, for Nf 3Nc, the original “electric” theory is no longer asymptotically free: as one goes deeper into the infrared (i.e. to larger distances), the coupling becomes smaller. The infrared regime is thus one of weakly coupled massless quarks and gluons: it is a free electric phase. On the other hand, we have seen in Section 8.3.2 that, for Nf just below 3Nc, appears a nontrivial infrared fixed point: the coupling tends in the infrared to the finite value g given in (8.42).

6The U (1) quantum numbers of q and q¯ are obtained by noting that baryons can be made with

˜

Nc quarks Q or, in the dual picture, Nc quarks q.

N = 2 supersymmetry and the Seiberg–Witten model 215

Table 8.4

 

SU (Nf )L

SU (Nf )R

U (1)B

U (1)R

Q

Nf

1

+1

˜

Nc/Nf

¯

1

¯

1

˜

Q

Nf

Nc/Nf

q

Nf

1

˜

Nc/Nf

Nc/Nc

q¯

1

¯

˜

Nc/Nf

Nf

−Nc/Nc

M

Nf

¯

0

˜

Nf

2Nc/Nf

Similarly, on the “magnetic side”, for Nf

˜

3Nc/2, the theory

3Nc, i.e. Nf

becomes free in the infrared: we are in the free magnetic phase. And for Nf just above 3Nc/2, we identify a nontrivial infrared fixed point.

One can show that nontrivial infrared fixed points may only appear for values of Nf larger than 3Nc/2. Indeed, let us suppose that we have such a fixed point: as we have seen in Section 8.3.2, the theory has superconformal invariance. The corresponding R symmetry is nothing but the nonanomalous one that we identified in Table 8.4. Since the field Mij of the magnetic theory has R-charge 2(Nf − Nc)/Nf and is in a chiral multiplet, we conclude from (8.44) that its scaling dimension is7 d = 3(Nf − Nc)/Nf . The condition d ≥ 1 imposes Nf 3Nc/2.

These considerations have led Seiberg to conjecture the existence of a nontrivial infrared fixed point for 3Nc/2 < Nf < 3Nc. The corresponding theory has superconformal invariance. Quarks and gluons are not confined but appear as interacting massless particles: this is referred to as the nonabelian Coulomb phase.

8.5N = 2 supersymmetry and the Seiberg–Witten model

We consider in this section a N = 2 supersymmetric SU (2) gauge theory. The fundamental fields in the ultraviolet limit are the fields of a N = 2 vector supermultiplet. We study the infrared regime of this theory.

As we have seen in Section 4.4.1 of Chapter 4, the fundamental fields of this theory can be arranged into a N = 1 vector supermultiplet (Aµ, λα) and a N = 1 chiral supermultiplet (φ, ψα) in the adjoint representation. The action can then be written as a sum of the relevant N = 1 actions with adequate normalizations. We will

 

 

 

 

 

 

 

 

˜µν

term. We thus

slightly generalize the case studied in Chapter 4 by allowing a θFµν F

write the full N = 2 action

 

 

 

 

 

 

 

 

1

Im τ

 

d4xd2θW αWα

1

 

d4xd4 θΦe2V Φ,

 

S =

 

+

 

(8.66)

16π

g2

7Note that, for Nf = 3Nc/2, d = 1. In other words, the field Mij is free.

216 Dynamical breaking. Duality

where Wα and Φ are respectively the gauge and chiral superfields and τ has been defined in (8.24) as

τ =

θ

+ i

4π

.

(8.67)

2 π

 

 

 

g2

 

The normalization of the chiral action is di erent from the one chosen in equation (4.28) of Chapter 4 because the normalization of the gauge fields is di erent (Aµ has been rescaled by 1/g). This can be checked on the Lagrangian written in terms of the component fields, which is obtained as in Chapter 4 using (C.81) of Appendix C:

L = Tr

1

 

 

 

θ

 

 

 

 

i

1

 

 

Fµν F µν

 

 

 

Fµν F˜µν +

 

 

 

λσµDµλ¯ +

 

D2

4g2

32π2

g2

2g2

+

 

1

DµφDµφ +

i

 

ψσµDµψ¯ +

1

F F

 

 

g2

g2

g2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Tr D φ, φ +

2ψ λ, φ2ψ¯ λ,¯ φ ,

 

 

g2

 

 

where the covariant derivatives are defined as:

Dµλ = µλ − i [Aµ, λ] ,

Dµφ = µφ − i [Aµ, φ] ,

Dµψ = µψ − i [Aµ, ψ] ,

Fµν = µAν − ∂ν Aµ − i [Aµ, Aν ] .

(8.68)

(8.69)

(8.70)

Solving for the auxiliary fields gives the corresponding scalar potential, which is a D-term:

V (φ) =

1

Tr

[φ, φ]

2

.

(8.71)

2g2

 

The ground state is obtained for φ and φcommuting. Since φ ≡ φaσa/2, this means that one can put it, through a gauge transformation, under the form

φ = a

σ3

(8.72)

2 .

It is straightforward to compute the spectrum of the theory in such a vacuum. The

fields Aa , λa, φa, ψa with a = 1, 2 all have mass a

 

whereas the corresponding a = 3

2

µ

 

 

A3 is the U (1) gauge potential

component has vanishing mass: in other words Aµ

µ

a

= F

a

= 0), it

and, since supersymmetry is not broken by the vacuum (8.72) (D

 

 

appears in a full N = 2 massless multiplet, of vanishing U (1) electric charge.

 

Let us check these results explicitly on the bosonic fields. As usual (see Appendix Appendix A), the gauge field mass terms arise from the scalar kinetic terms

N = 2 supersymmetry and the Seiberg–Witten model 217

once the gauge symmetry is spontaneously broken. Defining A(µ±) ≡ A1µ iA2µ /2, the mass term simply reads

 

 

 

 

 

 

a2

Aµ(+)A(),

 

 

 

 

 

 

 

 

 

 

 

 

 

g2

µ

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

whereas the kinetic terms fix the normalization

 

 

 

 

 

 

 

1

F (+)F ()µν +

1

m2Aµ(+)A().

 

 

 

 

 

 

 

8g2

µν

2g2

 

 

 

µ

 

 

 

 

Hence m = a

 

 

 

 

 

 

 

 

 

 

 

 

 

 

2.

 

 

 

 

 

 

 

 

 

2 /

 

 

The scalar fields also form two combinations φ(

)

φ1

 

 

of common

 

2

 

 

 

 

 

 

 

 

 

 

±

 

 

 

 

 

mass m = a2 and respective electric charge Qe =

 

 

 

±1.

 

 

We conclude that the massive states can be organized in two multiplets of re-

spective charge ±1 but same mass a 2. Each multiplet has eight degrees of freedom. But since supersymmetry is not broken in the vacuum (8.72), these multiplets must be N = 2 supermultiplets. This seems in contradiction with what we have seen in Section 4.3.2 of Chapter 4: massive representations of N supersymmetry theories have a multiplicity of 22N (2j + 1), which gives for N = 2 a minimum of 16 (for j = 0), unless there are central charges.

This necessarily means that the theory has a central charge and that the supermultiplets that we consider are the short supermultiplets discussed in Section 4.3.3 of Chapter 4. The mass of these supermultiplets is directly related to the central charge of the theory: m = z/2. Let us recall that the central charge is an operator which commutes with all the generators of the supersymmetry algebra. We deduce an expression

for this central charge:

 

 

z = 2 2 |aQe| .

(8.73)

Let us note that this expression might be incomplete since it has been obtained in the ultraviolet regime of the theory where the degrees of freedom have only electric charge. As expected from the considerations of Chapter 4, and as seen below, we expect that, in other regimes of the theory, appear solitons which carry magnetic charge.

We now try to identify the e ective low energy action. In the regime where we have easily access to it, it corresponds to a N = 2 supersymmetric U (1) theory, which we may describe in terms of a N = 1 abelian gauge supermultiplet Wα and a N = 1

chiral supermultiplet Φ of vanishing electric charge. The action reads:

 

S =

1

 

d4xd2θ F (Φ)W αWα +

d4x

d4θ ΦF (Φ) ,

(8.74)

16π Im

where the holomorphic function F (Φ) is a N = 2 prepotential which generalizes the discussion of Section 4.4.1 of Chapter 4: it determines simultaneously the holomorphic gauge kinetic function f (Φ) iF (Φ) and the K¨ahler potential K, Φ) = ImF (Φ) which fixes the normalization of the scalar kinetic term.

We have already noted that the zeroes of the K¨ahler potential represent singular points in the scalar field parameter space where the parametrization is inadequate,

218 Dynamical breaking. Duality

usually because the light degrees of freedom have not been identified properly. Indeed, because F (Φ) is holomorphic, K, Φ) = ImF (Φ) is harmonic and has thus no minimum in the complex plane. If it is not constant, it should reach zero at some point.

We will see however that the e ective action (8.74) has alternate descriptions which may thus describe other regimes of the theory. We start by performing what is known as a duality transformation.

We define

 

 

 

ΦD = F (Φ)

 

 

 

(8.75)

 

 

 

FDD) = F (Φ) ΦΦD,

(8.76)

which allows us to make a Legendre transformation since

 

We thus have

 

 

Φ = −FDD).

 

 

(8.77)

 

d4x

 

 

 

 

 

 

Im

d4θ ΦF (Φ) = Im

d4x

d4θ [FDD)]ΦD

 

 

 

 

= Im

d4x

d4θ ΦDFDD).

(8.78)

Hence the second term of (8.74) allows us to identify FD as the prepotential in the dual formulation. Before checking this with the first term, let us note that

 

 

dΦ

1

 

 

FD

D) =

 

=

 

.

(8.79)

dΦD

F (Φ)

Hence the duality transformation yields an alternative description where the parameter τ introduced in (8.66) transforms as

τD(aD) =

1

 

(8.80)

τ (a)

 

in moduli space where

 

 

 

φD = aDσ3/2

(8.81)

as in (8.72). Moreover (8.67) tells us that this is a duality relation of the weak coupling/strong coupling type, i.e. g2 1/g2, that we have encountered when discussing electric–magnetic duality.

Before dwelling more on this, let us show that the gauge part of the action (8.74) is invariant under the duality transformation. For this we recall that the gauge superfield Wα can be defined as a generic chiral superfield which satisfies the constraint (C.68) of

Appendix C: D

α

 

 

 

¯

¯

α˙

which we may write Im D

α

Wα = 0. Thus, performing

 

Wα = Dα˙

W

 

 

a functional integration in superspace, we may write

 

 

 

 

 

 

DV exp

i

Im

d4xd2θF (Φ)W αWα

 

 

 

 

 

 

 

 

 

 

 

16π

 

 

 

d4xd4θVDDαWα

,

=

DW DVD exp

 

16π Im

d4xd2θF (Φ)W αWα + 2

 

 

 

 

 

 

 

i