We develop a superspace formulation for N = 3 conformal supergravity in four spacetime dimensions as a gauge theory of the superconformal group SU(2, 2|3). Upon imposing certain covariant constraints, the algebra of conformally covariant derivatives del(A)=(del(a),del(alpha)(i),del((sic))(i)) is shown to be determined in terms of a single primary chiral spinor superfield, the super-Weyl spinor W-alpha of dimension +1/2 and its conjugate. Associated with W-alpha is its primary descendant B-j(i) of dimension +2, the super-Bach tensor, which determines the equation of motion for conformal supergravity. As an application of this construction, we present two different but equivalent action principles for N = 3 conformal supergravity. We describe the model for linearised N = 3 conformal supergravity in an arbitrary conformally flat background and demonstrate that it possesses U(1) duality invariance. Additionally, upon degauging certain local symmetries, our superspace geometry is shown to reduce to the U(3) superspace constructed by Howe more than four decades ago. Further degauging proves to lead to a new superspace formalism, called SU(3) superspace, which can also be used to describe N = 3 conformal supergravity. Our conformal superspace setting opens up the possibility to formulate the dynamics of the off-shell N = 3 super Yang-Mills theory coupled to conformal supergravity.
机构:
Queen Mary Univ London, CRST, London E1 4NS, England
Queen Mary Univ London, Sch Phys & Astron, London E1 4NS, England
Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
Univ Chicago, Dept Phys, Chicago, IL 60637 USAQueen Mary Univ London, CRST, London E1 4NS, England
Buican, Matthew
Nishinaka, Takahiro
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机构:
Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, JapanQueen Mary Univ London, CRST, London E1 4NS, England