Black holes in Einstein-aether theory: Quasinormal modes and time-domain evolution
arXiv:2002.03450 · doi:10.1103/PhysRevD.102.024076
Abstract
We propose accurate calculations of quasinormal modes of black holes in the Einstein-aether theory, which were previously considered in the literature, partially, with insufficient accuracy. We also show that the arbitrarily long-lived modes, quasiresonances, are allowed in the Einstein-aether theory as well and demonstrate that the asymptotic tails, unlike quasinormal frequencies, are indistinguishable from those in the Einstein theory.
arXiv comment9 pages, 7 figures, revtex, the version accepted for publication in Physical Review D
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