2020
DOI: 10.1007/jhep01(2020)029
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$$ \mathcal{N} $$ = 4 conformal supergravity: the complete actions

Abstract: The most general class of 4D N = 4 conformal supergravity actions depends on a holomorphic function of the scalar fields that parametrize an SU(1, 1)/U(1) coset space. The bosonic sector of these actions was presented in a letter [1]. Here we provide the complete actions to all orders in the fermion fields. They rely upon a new N = 4 density formula, which permits a direct but involved construction. This density formula also recovers the on-shell action for vector multiplets coupled to conformal supergravity. … Show more

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Cited by 18 publications
(37 citation statements)
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“…This action with (n, m) = (1, 0) describes a conformal Weyl spinor, while the n = m = 0 case corresponds to an auxiliary complex scalar that appears, at the component level, in the conformal Wess-Zumino model (7.25). 7 The action (7.5) with (n, m) = (2, 0) describes a self-dual two-form that emerges in extended conformal supergravity theories [30][31][32][33][34][35][36] (see [7] for a review). The field χ α(2) played an important role in the pseudo-graviton model constructed in section 3.…”
Section: Jhep08(2020)068mentioning
confidence: 99%
“…This action with (n, m) = (1, 0) describes a conformal Weyl spinor, while the n = m = 0 case corresponds to an auxiliary complex scalar that appears, at the component level, in the conformal Wess-Zumino model (7.25). 7 The action (7.5) with (n, m) = (2, 0) describes a self-dual two-form that emerges in extended conformal supergravity theories [30][31][32][33][34][35][36] (see [7] for a review). The field χ α(2) played an important role in the pseudo-graviton model constructed in section 3.…”
Section: Jhep08(2020)068mentioning
confidence: 99%
“…In this section we will revisit the arguments made in [26] to show that the constraints coming from the higher Bianchi will follow from the preliminary constraints (2.22, 2.29). The argument is based on taking a Bianchi identity of the Bianchi identity.…”
Section: Bianchi Identity Of the Bianchi Identity: Constraints Frommentioning
confidence: 99%
“…This is a standard method which is used to construct invariant actions in supergravity in various dimensions (See [20][21][22][23]). It was first introduced in superspace as the 'ectoplasm principle' [24,25] and has been recently applied in [26] to construct the most general actions for N = 4 conformal supergravity. Similar ideas have also been used in rheonomic approach to supergravity [27,28].…”
Section: Introductionmentioning
confidence: 99%
“…12 The standard conformal supergravity theories in d = 4 based on the conformal superalgebras SU(2, 2|N ) exist only for N ≤ 4. All N =4 conformal supergravities in d = 4 have recently been constructed in [51,52]. In addition to a massless graviton they contain a massive spin two ghost field and hence are not unitary.…”
Section: Jhep06(2021)081mentioning
confidence: 99%