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N=2 Supersymmetric Gauge Theories with Nonpolynomial Interactions

N=2 Supersymmetric Gauge Theories with Nonpolynomial Interactions

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2.2. Consistent Deformations 21<br />

implies<br />

D i αa = −ψ i α , (2.18)<br />

which suggests to combine a and L into a complex scalar field that is then chiral,<br />

φ ≡ 1<br />

2 (iL − a) ⇒ Di αφ = ψ i α , ¯ D ˙αiφ = 0 . (2.19)<br />

Using U ≈ 0, the Lagrangian (2.15) turns into<br />

Ldual = 2 ∂ µ φ¯ ∂µφ − 1<br />

4 V µν Vµν − iψ i ↔<br />

µ<br />

σ ∂µ ¯ ψi , (2.20)<br />

while the transformations of ψ i and ¯ ψi read<br />

D i αψ j i<br />

β ≈ 2εij Vµνσ µν αβ , D i α ¯ ψ j<br />

˙α ≈ iεij∂α ˙α ¯ φ . (2.21)<br />

Thus an on-shell equivalence has been established between the vector-tensor multiplet<br />

and an abelian vector multiplet.<br />

2.2 Consistent Deformations<br />

To couple the vector-tensor multiplet to an abelian vector multiplet such that the<br />

central charge transformations are realized locally, it will be necessary to modify the<br />

superfield constraints (2.3) which determine the multiplet. This is different from the<br />

hypermultiplet where the constraints could be retained when gauging the central charge.<br />

But also self-interactions and couplings to nonabelian vector multiplets are obtained<br />

from suitable deformations of the constraints. Instead of starting from a distinct Ansatz<br />

for each single case and then working out anew all the transformations and Bianchi<br />

identities, we treat all models simultaneously as far as possible by considering the<br />

most general deformation that does not alter the field content of the vector-tensor<br />

multiplet. The supersymmetry algebra imposes conditions on the constraints that<br />

restrict the possible deformations. These consistency conditions come in two kinds:<br />

First there are conditions that involve spacetime derivatives like the Bianchi identities<br />

(we shall call the differential constraints on W µ and Gµν so generically even if they<br />

cannot be solved, in which case the constraints are inconsistent), and second there are<br />

algebraic conditions <strong>with</strong>out derivatives. We shall use the latter to single out possible<br />

constraints before trying to solve the conditions of the first kind. In the course of this<br />

we will encounter constraints that pass all hurdles save said Bianchi identities, so the<br />

consistency conditions of the second kind are necessary but not sufficient. Furthermore,<br />

seemingly different superfield constraints may be connected by a field redefinition. We<br />

do not distinguish such constraints as they do not lead to different theories. This will<br />

be of great help, for it allows to simplify the calculations by choosing certain “gauges”.<br />

Let us consider the constraints<br />

D (i D j) L = M ij , D (i<br />

α ¯ D j) i L =<br />

˙α<br />

2<br />

ij<br />

Nα ˙α , (2.22)

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