http://arxiv.org/abs/1806.01903
A regular rotating MOG compact object is derived that reduces to the Kerr black hole when the parameter $\alpha=0$. Physical consequences of the dark compact object, which is regular everywhere in spacetime for $\alpha > \alpha_{\rm crit}=0.674$ and is a rotating Kerr-MOG black hole for $\alpha < \alpha_{\rm crit}$ are investigated.
J. Moffat
Thu, 7 Jun 18
7/51
Comments: 7 pages, 2 figures
You must be logged in to post a comment.