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Note on constants of motion in conformal mechanics associated with near horizon extremal Myers-Perry black holes

机译:关于与近地平线迈尔斯 - 佩里黑洞相关的保形力学常数的注意事项

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摘要

We investigate dynamics of probe particles moving in the near-horizon limit of (2N + 1)-dimensional extremal Myers Perry black hole (in the cases of N = 3, 4, 5) with arbitrary rotation parameters. Very recently it has been shown in [T. Hakobyan, A. Nersessian and M. M. Sheikh-Jabbari, Phys. Lett. B 772, 586 (2017)] that in the most general cases with non-equal nonvanishing rotational parameters the system admits separation of variables in N-dimensional ellipsoidal coordinates. We wrote down the explicit expressions of Liouville integrals of motion, given in the above-mentioned reference in ellipsoidal coordinates, in initial "Cartesian" coordinates in seven, nine and eleven dimensions, and found that these expressions hold in any dimension. Then, taking the limit where all of the rotational parameters are equal, we reveal that each of these N - 1 integrals of motion results in the Hamiltonian of the spherical mechanics of a (2N + 1)-dimensional MP black hole with equal nonvanishing rotational parameters.
机译:我们调查探头颗粒的动态,在近地平线上移动(2n + 1) - 二维极值麦克雷黑洞(在n = 3,4,5)中,具有任意旋转参数。最近,它已经显示在[T. Hakobyan,A. Nersessian和M. M. Sheikh-Jabbari,Phy。吧。 B 772,586(2017)]在最常规的非等于非衰弱旋转参数的情况下,系统承认在N维椭圆坐标中的变量分离。我们介绍了Liouville Motion的明确表达,在椭圆形坐标上的上述参考中,在初始的“笛卡尔”坐标中,在七个,九个和十一尺寸中,发现这些表达式在任何维度中保持。然后,采取所有旋转参数等于的极限,我们揭示了这些N - 1的每个N - 1的整体中的每一个在具有相等的非丹麦旋转的(2N + 1) - 二维MP黑洞的球形机械的Hamiltonian中产生的运动结果参数。

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