Higher spin de Sitter quasinormal modes
arXiv:2010.09684 · doi:10.1007/JHEP11(2021)025
Abstract
We construct higher spin quasinormal modes algebraically in -dimensional de Sitter spacetime using the ambient space formalism. The quasinormal modes fall into two nonunitary lowest-weight representations of . From a local QFT point of view, the lowest-weight quasinormal modes of massless higher spin fields are produced by gauge-invariant boundary conserved currents and boundary higher-spin Weyl tensors inserted at the southern pole of the past boundary. We also show that the quasinormal spectrum of a massless/massive spin- field is precisely encoded in the Harish-Chandra character corresponding to the unitary massless/massive spin- representation.
38 pages, 1 figure
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