Near-zone symmetries of Kerr black holes

被引:0
作者
Lam Hui
Austin Joyce
Riccardo Penco
Luca Santoni
Adam R. Solomon
机构
[1] Columbia University,Center for Theoretical Physics, Department of Physics
[2] University of Chicago,Kavli Institute for Cosmological Physics, Department of Astronomy and Astrophysics
[3] Carnegie Mellon University,McWilliams Center for Cosmology, Department of Physics
[4] ICTP,Department of Physics and Astronomy
[5] International Centre for Theoretical Physics,undefined
[6] McMaster University,undefined
[7] Perimeter Institute for Theoretical Physics,undefined
来源
Journal of High Energy Physics | / 2022卷
关键词
Black Holes; Classical Theories of Gravity;
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摘要
We study the near-zone symmetries of a massless scalar field on four-dimensional black hole backgrounds. We provide a geometric understanding that unifies various recently discovered symmetries as part of an SO(4, 2) group. Of these, a subset are exact symmetries of the static sector and give rise to the ladder symmetries responsible for the vanishing of Love numbers. In the Kerr case, we compare different near-zone approximations in the literature, and focus on the implementation that retains the symmetries of the static limit. We also describe the relation to spin-1 and 2 perturbations.
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