Higher-spin gauge interactions for massive matter fields in 3D AdS space-time
Autor: | Mikhail A. Vasiliev, Sergey Prokushkin |
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Rok vydání: | 1999 |
Předmět: | |
Zdroj: | Nuclear Physics B. 545:385-433 |
ISSN: | 0550-3213 |
DOI: | 10.1016/s0550-3213(98)00839-6 |
Popis: | A remarkable feature of the models with interactions exhibiting higher-spin (HS) gauge symmetries in $d>2$ is that their most symmetric vacua require (anti)-de Sitter (AdS) geometry rather than the flat one. In striking parallelism to what might be expected of M theory HS gauge theories describe infinite towers of fields of all spins and possess naturally space-time SUSY and Chan-Paton type inner symmetries. In this paper, we analyze at the level of the equations of motion the simplest non-trivial HS model which describes HS gauge interactions (on the top of the usual supergravitational and (Chern-Simons) Yang-Mills interactions) of massive spin-0 and spin-1/2 matter fields in d=2+1 AdS space-time. The parameter of mass of the matter fields is identified with the vev of a certain auxiliary field in the model. The matter fields are shown to be arranged into d3 N=2 massive hypermultiplets in certain representations of $U(n)\times U(m)$ Yang-Mills gauge groups. Discrete symmetries of the full system are studied, and the related N=1 supersymmetric truncations with O(n) and Sp(n) Yang-Mills symmetries are constructed. The simplicity of the model allows us to elucidate some general properties of the HS models. In particular, a new result, which can have interesting implications to the higher-dimensional models, is that our model is shown to admit an "integrating" flow that proves existence of a non-local B��cklund-Nicolai-type mapping to the free system. LaTeX, 46 pages, no figures; minor corrections, typos |
Databáze: | OpenAIRE |
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