Abstract
We explore static spherically symmetric black hole solutions allowing a bulk U(1) vector field in the khronometric formulation of Hǒrava gravity by way of Einsteinther. We examine analytic solutions and study numerical results in the limit that the khronon does not backreact on the metric. © The Authors.
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APA
Janiszewski, S., Karch, A., Robinson, B., & Sommer, D. (2014). Charged black holes in Hǒrava gravity. Journal of High Energy Physics, 2014(4). https://doi.org/10.1007/JHEP04(2014)163
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