Gravitational stability of simply rotating Myers-Perry black holes: Tensorial perturbations

Journal Article · Mon Feb 15 00:00:00 EST 2010 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.81.044007· OSTI ID:21409295

Kodama, Hideo; Konoplya, R A; Zhidenko, Alexander ^[1]

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1. Cosmophysics Group, IPNS, KEK, and the Graduate University of Advanced Studies, 1-1 Oho, Tsukuba 305-0801 (Japan)

We study the stability of D{>=}7 asymptotically flat black holes rotating in a single two-plane against tensor-type gravitational perturbations. The extensive search of quasinormal modes for these black holes did not indicate any presence of growing modes, implying the stability of simply rotating Myers-Perry black holes against tensor-type perturbations.

• OSTI ID: 21409295
• Journal Information: Physical Review. D, Particles Fields, Vol. 81, Issue 4; Other Information: DOI: 10.1103/PhysRevD.81.044007; (c) 2010 The American Physical Society; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BLACK HOLES
DISTURBANCES
GRAVITATION
PERTURBATION THEORY
SIMULATION
STABILITY