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Stationary Lifshitz black holes of R^2-corrected gravity theory
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In this short note, I present a generalization of a set of static D-dimensional (D >= 3) Lifshitz black holes, which are solutions of the gravitational model obtained by amending the cosmological Einstein theory with the addition of only the curvature-scalar-squared term and that are described by two parameters, to a more general class of exact, analytic solutions that involves an additional parameter which now renders them stationary. In the special D=3 and the dynamical exponent z=1 case, the parameters can be adjusted so that the solution becomes identical to the celebrated BTZ black hole metric.
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Revisiting Lifshitz-type solutions in $R^2$-corrected gravity
Exact Lifshitz-type black holes and branes, including rotating and extremal cases, are constructed in R²-corrected gravity at the critical point in arbitrary dimensions.
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