Quasinormal modes of modified gravity (MOG) black holes
The Quasinormal modes (QNMs) for gravitational and electromagnetic perturbations are calculated in a Scalar–Tensor–Vector (Modified Gravity) spacetime, which was initially proposed to obtain correct dynamics of galaxies and galaxy clusters without the need for dark matter. It is found that for the i...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2018-04-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269317308985 |