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N=2 Supersymmetric Gauge Theories with Nonpolynomial Interactions

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32 Chapter 2. The Vector-Tensor Multiplet<br />

From this we infer first of all that the imaginary part of F is L-independent, thus<br />

F = f(L) + iκ , κ ∈ R ⇒ ∂Lf = f 2 + κ 2 . (2.65)<br />

When κ = 0, we have two solutions. On the one hand F1 = 0, which corresponds to<br />

the free constraints (2.3) as then all coefficients vanish. The second solution is<br />

F2 = − 1<br />

L + µ<br />

, µ ∈ R , (2.66)<br />

where µ may be removed by a field redefinition (2.62). In the case κ = 0 the general<br />

solution reads<br />

F3 = κ tan(κL + ϱ) + i , ϱ ∈ R . (2.67)<br />

We may choose κ = 1 and ϱ = 0. Since we have fixed the gauge, the three solutions<br />

evidently yield distinct constraints that are not connected by a field redefinition. This<br />

may also be seen from the transformation law of the coefficient G: If G = 0 for one<br />

representative of a class of constraints, then this holds in the whole class. Moreover,<br />

there is no transition from the second to the third solution since G2 is real while G3 is<br />

not.<br />

The constraints that correspond to F3 were first discovered by Ivanov and Sokatchev<br />

in [21]. However, these are inconsistent, for the Bianchi identities (BI.1) and (BI.2)<br />

admit no local solution. We shall not demonstrate this fact, but remark that it shows<br />

that the conditions (C.1–4) are by no means sufficient.<br />

The solution F2 implies constraints<br />

D (i<br />

α ¯ D j)<br />

˙α L = 0 , D(iD j) L = − 1 i j<br />

D L D L + D¯ i<br />

L D¯ j<br />

L , (2.68)<br />

L<br />

which are indeed consistent and describe what is known as the nonlinear vector-tensor<br />

multiplet. We shall first generalize these constraints to admit a gauged central charge<br />

before investigating them in any more detail. This will be done in chapter 4. At this<br />

point we just emphasize that the constraints may be rendered regular for ˆ L = 0 by a<br />

field redefintion<br />

L = exp(−κ ˆ L) , κ ∈ R ∗ , (2.69)<br />

which gives (omitting the hat)<br />

D (i<br />

α ¯ D j)<br />

˙α<br />

L = κ D(i<br />

α L ¯ D j)<br />

˙α L , D(iD j) L = 2κ D i L D j L + κ ¯ D i L ¯ D j L . (2.70)<br />

In this form they were first derived in [20] and are evidently a deformation of the free<br />

theory. While here the coefficients are constant, we shall nevertheless generalize the<br />

constraints (2.68), for these have the useful property of vanishing N ij<br />

α ˙α .<br />

2.3.3 Generalization to Z(x)<br />

In the general case of an x-dependent field Z the consistency conditions (C.1–3), which<br />

we have translated into a set of differential equations, do not determine completely the

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