Scalar field quasinormal modes on asymptotically locally flat rotating black holes in three dimensions

• Main Authors: Anabalon, Andres, Fierro, Octavio, Figueroa, Jose, Oliva, Julio
• Format: Text
• Language: unknown
• Published: arXiv 2019
• Subjects: High Energy Physics - Theory hep-th; General Relativity and Quantum Cosmology gr-qc; FOS Physical sciences; North Pole; Myers
• Online Access: https://dx.doi.org/10.48550/arxiv.1901.00448; https://arxiv.org/abs/1901.00448

The pure quadratic term of New Massive Gravity in three dimensions admits asymptotically locally flat, rotating black holes. These black holes are characterized by their mass and angular momentum, as well as by a hair of gravitational origin. As in the Myers-Perry solution in dimensions greater than...