Scalar fields and their quasinormal modes on asymptotically locally flat rotating black holes in three dimensions

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...

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Bibliographic Details
Published in:The European Physical Journal C
Main Authors: Anabalon, A., Fierro, O., Figueroa, J., Oliva, J.
Format: Article in Journal/Newspaper
Language:unknown
Published: 2019
Subjects:
Online Access:http://hdl.handle.net/21.11116/0000-0002-DC90-3
http://hdl.handle.net/21.11116/0000-0002-DC92-1
http://hdl.handle.net/21.11116/0000-0003-5439-F