TY - JOUR
T1 - 11D supergravity as a gauge theory for the M-algebra
AU - Hassaïne, Mokhtar
AU - Troncoso, Ricardo
AU - Zanelli, Jorge
N1 - Funding Information:
C. In the presence of negative cosmological constant, eleven-dimensional AdS supergravity [12] can be written as a Chern-Simons theory for osp(32|1), which is the supersymmetric extension of AdS11. It is natural to ask whether there is a link between that theory in the vanishing cosmological constant limit, and the one discussed here. Since the M-algebra has 55 bosonic generators more than osp(32|1), these theories cannot be related through a Inönü-Wigner contraction for a generic value of α. However, it has been recently pointed out in [23], generalizing the procedure of [24], that it is possible to obtain the M-algebra from an expansion of osp(32|1). In this light, applying this procedure to the eleven-dimensional AdS supergravity theory, it should be expected that the action presented here will be recovered up to some additional terms decoupled from the vielbein, that are supersymmetric by themselves. ————————– Acknowledgments.- We thank J. Edelstein, G. Kofinas, C. Martínez, C. Núñez, R. Portugués and C. Teitelboim for many enlightening discussions and useful comments. This work is partially supported by grants 3020032, 1010450, 1010446, 1010449, 1020629 and 1040921 from FONDE-CYT. We thank the organizers of Fourth International Winter Conference on Mathematical Methods in Physics for the lively and stimulating conference in Rio. Institutional support to the Centro de Estudios Científicos (CECS) from Empresas CMPC is gratefully acknowledged. CECS is a Millennium Science Institute and is funded in part by grants from Fundación Andes and the Tinker Foundation.
Publisher Copyright:
© 2004 Sissa Medialab Srl. All Rights Reserved.
PY - 2004
Y1 - 2004
N2 - The eleven-dimensional gravitational action invariant under local Poincaré transformations is given by the dimensional continuation of the Euler class of ten dimensions. Here we show that the supersymmetric extension of this action leads, through the Noether procedure, to a theory with the local symmetry group given by the M-algebra. The fields of the theory are the vielbein eaµ, the Lorentz (spin) connection ωabµ , one gravitino (ψµ), and two 1-forms, babµ and babcdeµ , which transform as antisymmetric Lorentz tensors. These fields are components of a single connection for the M-algebra and the supersymmetric Lagrangian can be seen to be a Chern-Simons form. The dynamics has a multiplicity of degenerate vacua without propagating degrees of freedom. The theory is shown to admit solutions of the form S10−d × Xd+1, where Xd+1 is a warped product of R with a d-dimensional spacetime. Among this class, the gravitational effective action describes a propagating graviton only if d = 4 and the spacetime has positive cosmological constant. The perturbations around this solution reproduce linearized General Relativity around four-dimensional de Sitter spacetime.
AB - The eleven-dimensional gravitational action invariant under local Poincaré transformations is given by the dimensional continuation of the Euler class of ten dimensions. Here we show that the supersymmetric extension of this action leads, through the Noether procedure, to a theory with the local symmetry group given by the M-algebra. The fields of the theory are the vielbein eaµ, the Lorentz (spin) connection ωabµ , one gravitino (ψµ), and two 1-forms, babµ and babcdeµ , which transform as antisymmetric Lorentz tensors. These fields are components of a single connection for the M-algebra and the supersymmetric Lagrangian can be seen to be a Chern-Simons form. The dynamics has a multiplicity of degenerate vacua without propagating degrees of freedom. The theory is shown to admit solutions of the form S10−d × Xd+1, where Xd+1 is a warped product of R with a d-dimensional spacetime. Among this class, the gravitational effective action describes a propagating graviton only if d = 4 and the spacetime has positive cosmological constant. The perturbations around this solution reproduce linearized General Relativity around four-dimensional de Sitter spacetime.
UR - http://www.scopus.com/inward/record.url?scp=85057623997&partnerID=8YFLogxK
U2 - 10.22323/1.013.0006
DO - 10.22323/1.013.0006
M3 - Conference article
AN - SCOPUS:85057623997
SN - 1824-8039
VL - 13
JO - Proceedings of Science
JF - Proceedings of Science
T2 - 4th International Winter Conference on Mathematical Methods in Physics, WC 2004
Y2 - 9 August 2004 through 13 August 2004
ER -