Consistency between black hole and mimetic gravity -- Case of $(2+1)$-dimensional gravity

Abstract

We show that the mimetic theory with the constraint $g^{\rho \sigma }{\partial }_{\rho }\varphi {\partial }_{\sigma }\varphi =1$ cannot realize the black hole geometry with the horizon(s). To overcome such issue, we may change the mimetic constraint a little bit by $\omega (\varphi )g^{\rho \sigma }{\partial }_{\rho }\varphi {\partial }_{\sigma }\varphi =-1,$ where $\omega (\varphi )$ is a function of the scalar field $\varphi$. As an example, we consider $(2+1)$-dimensional mimetic gravity with the mimetic potential and construct black hole (BH) solutions by using this modified constraint. We study three different classes: In the first class, we assume the Lagrange multiplier and mimetic potential are vanishing and obtain a BH solution that fully matches the BH of GR despite the non-triviality of the mimetic field which ensures the study presented in {\it JCAP 01 (2019) 058}. In the second class, we obtain a BH having constant mimetic potential and a non-trivial form of the Lagrange multiplier. In the third class, we obtain a new BH solution with non-vanishing values of the mimetic field, the Lagrange multiplier, and the mimetic potential. In any case, the solutions correspond to the space-time with only one horizon but we show that the formalism for the constraint works.

10 pages Accepted in PLB

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• Multi-horizons black hole solutions, photon sphere and perihelion shift in weak ghost-free Gauss-Bonnet theory of gravity
• Isotropic stellar model in mimetic theory
• Mimetic Weyl geometric gravity