We show that the semiclassical entropy of $D$-dimensional rotating(an)isotropic black holes with planar horizon can be successfully computedaccording to a Cardy-like formula. This formula does not refer to any centralcharges but instead involves the vacuum energy which is identified with agravitational bulk soliton. The soliton is obtained from the non-rotating blackhole solution by means of a double analytic continuation. The robustness of theCardy-like formula is tested with numerous and varied examples, including AdS,Lifshitz and hyperscaling violation planar black holes.
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机译：我们表明，可以根据Cardy式公式成功地计算出具有平面水平线的$ D $维旋转（各向同性）黑洞的半经典熵。该公式不涉及任何中心电荷，而是涉及由重力本体孤子确定的真空能。通过双重分析连续性从非旋转黑洞溶液中获得孤子。类卡迪公式的鲁棒性已通过众多示例进行了测试，包括AdS，Lifshitz和超标违规平面黑洞。
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