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Testing Ho\v{r}ava-Lifshitz gravity using thin accretion disk properties · Around

2009

Testing Ho\v{r}ava-Lifshitz gravity using thin accretion disk properties

Harko, Tiberiu, Kovács, Zoltán, Lobo, Francisco S. N.

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Recently, a renormalizable gravity theory with higher spatial derivatives in four dimensions was proposed by Horava.

The theory reduces to Einstein gravity with a non-vanishing cosmological constant in IR, but it has improved UV behaviors.
The spherically symmetric black hole solutions for an arbitrary cosmological constant, which represent the generalization of the standard Schwarzschild-(A)dS solution, has also been obtained for the Horava-Lifshitz theory.
The exact asymptotically flat Schwarzschild type solution of the gravitational field equations in Horava gravity contains a quadratic increasing term, as well as the square root of a fourth order polynomial in the radial coordinate, and it depends on one arbitrary integration constant.

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T. P. Sotiriou, M. Visser and S. Weinfurtner, arXiv:0904.4464 [hep-th]; M. Visser, arXiv:0902.0590 [hep-th]; P. Horava, Phys. Rev. Lett. 102
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