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Quasinormal modes of a scalar perturbation coupling with Einstein’s tensor in the warped<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>AdS</mml:mi><mml:mn>3</mml:mn></mml:msub></mml:math>black hole spacetime

Quasinormal modes of a scalar perturbation coupling with Einstein’s tensor in the warped<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>AdS</mml:mi><mml:mn>3</mml:mn></mml:msub></mml:math>black hole spacetime

We have studied the quasinormal modes of a massive scalar field coupling to Einstein's tensor in the spacelike stretched ${\mathrm{AdS}}_{3}$ black hole spacetime. We find that both the right-moving and left-moving quasinormal frequencies depend not only on the warped parameter $v$ of the black hole, but also on the coupling …