On the Vacuum Structure of the $\mathcal{N}=4$ Conformal Supergravity

Abstract

We consider $\mathcal{N}=4$ conformal supergravity with an arbitrary holomorphic function of the complex scalar $S$ which parametrizes the $SU(1,1)/U(1)$ coset. Assuming non-vanishings vevs for $S$ and the scalars in a symmetric matrix $E_{ij}$ of the $\overline{10}$ of $SU(4)$ R-symmetry group, we determine the vacuum structure of the theory. We find that the possible vacua are classified by the number of zero eigenvalues of the scalar matrix and the spacetime is either Minkowski, de Sitter or anti-de Sitter. We determine the spectrum of the scalar fluctuations and we find that it contains tachyonic states which however can be removed by appropriate choice of the unspecified at the supergravity level holomorphic function. Finally, we also establish that $S$-supersymmetry is always broken whereas $Q$-supersymmetry exists only on flat Minkowski spacetime.

17 pages

References in corpus (6)

• Einstein Gravity from Conformal Gravity
• Higher-Derivative Chiral Superfield Actions Coupled to N=1 Supergravity
• Emerging Potentials in Higher-Derivative Gauged Chiral Models Coupled to N=1 Supergravity
• Maximally Supersymmetric AdS4 Vacua in N=4 Supergravity
• Cosmological properties of a generic (\cal R)^2-supergravity
• Aspects of Conformal Supergravity