Shadows of Einstein–dilaton–Gauss–Bonnet black holes
We study the shadows of the fully non-linear, asymptotically flat Einstein–dilaton–Gauss–Bonnet (EdGB) black holes (BHs), for both static and rotating solutions. We find that, in all cases, these shadows are smaller than for comparable Kerr BHs, i.e. with the same total mass and angular momentum und...
Main Authors: | , , , , |
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Format: | Article |
Language: | English |
Published: |
Elsevier
2017-05-01
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Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269317302071 |