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Stability of five-dimensional Myers-Perry black holes with equal angular momenta

Stability of five-dimensional Myers-Perry black holes with equal angular momenta. Kyoto University, Japan Keiju Murata & Jiro Soda. Introduction. In string theory. Our spacetime should be higher dimension. 4D spacetime + compactified space. It need not be planck scale.

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Stability of five-dimensional Myers-Perry black holes with equal angular momenta

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  1. Stability of five-dimensional Myers-Perry black holes with equal angular momenta Kyoto University, Japan Keiju Murata & Jiro Soda

  2. Introduction In string theory Our spacetime should be higher dimension. 4D spacetime + compactified space It need not be planck scale. large extra dimension scenario (ADD model, brane world, …) The compactified space can be mm scale. The fundamental Planck mass can be TeV scale. Mini black holes may be produced at LHC. evidence for higher dimensional spacetime It is important to study the higher dimensional black holes.

  3. variety of higher dimensional black holes (Emparan & Reall, 2006) They can have same masses and angular momenta. black ring Myers-Perry BH Ｍ, J Ｍ, J There is no uniqueness theorem in higher dimensional spacetime. What kind of black holes are formed in colliders? To answer this problem, we need the stability analysis of higher dimensional black holes. We focus on the stability analysis of Myers-Perry black holes.

  4. What is the stability analysis? We consider the perturbation of the background metric. substitute perturbation equation If the grows exponentially, the background spacetime is unstable. If the oscillates , the background spacetime is stable. In general, the perturbation equation is given by PDE. However, in some cases, the perturbtion equation can be separated and becomes ODE. ex) Schwarzschild BH

  5. stability analysis of rotating black holes Killing vectors of general D-dimensional Myers-Perry BH are (n+1) Killing vectors n+1 < D-1 (for D >= 4) In general, the symmetry is not enough to separate the perturbation equation. However, in some cases, the symmetry is enhanced and the perturbation equation of the Myers-Perry spacetime becomes separable.

  6. Myers-Perry black holes with equal angular momenta The spaceime symmetry is enhanced and we can separate the perturbation equations. We constructed the formalism for stability analysis of 5-dimensional Myers-Perry BH with equal angular momenta and We gave the strong evidence for stability of this BH. (KM & J.Soda, Prog.Theor.Phys.120:561-579,2008 [arXiv:0803.1371 ])

  7. 5D Myers-Perry BH with equal angular momenta stability analysis PDEs of The PDEs can be reduced to ODEs by the mode decomposition.

  8. Symmetry are invariant forms of SU(2). that is SU(2) symmetry SU(2)Killing part has a rotational symmetry. U(1) symmetry The symmetry of this spacetime is We decompose by using this symmetry and obtain ODEs.

  9. mode function , and are simultaneously diagonalizable. eigenfunction Wigner functions

  10. We can also construct vector and tensor eigen functions. vector Wigner function tensor Wigner function Making use of these mode functions, we can separate the tensor field as Substituting this into , we can get ODEs labeled by (J, K, M). In general, the resultant ODEs are coupled each other and cannot reduce to single ODE. However, special modes are decoupled and reduce to single ODE. We studied the stability of these mode.

  11. Master equations symmetric mode master equation for J=M=K=0 mode gauge conditions master variable tortoise coordianate We obtain Schrodinger type master equation.

  12. master equation V_0 The potential is positive definite. This mode is stable. r / r_h From bottom to top,a/a_max = 0.25, 0.5, 0.75, 0.99

  13. J=M=0, K=±1 ∀J, ∀M, K=±(J+2) (J=0, M=0, K=0,±1) and (J, M, K=±(J+2)) modes reduce to single ODE. These equations are not Schrodinger type equations. We solved the equations numerically and found that there is not mode with Im(ω)> 0. These mode are stable.

  14. Summary We have studied the stability of 5-dimensional Myers-Perry black holes with equal angular momenta. The perturbation equations can be separate and reduce to ODEs. Some modes are decoupled and reduce to single ODEs. We got the master equations for these modes and showed the stability. evidence for the stability of this BH.

  15. We found that these modes are stable. evidence for stability of this spacetime

  16. example 4-dimensional Schwarzschild BH Killing vectors of this spacetime are time translation symmetry spherical symmetry We define operators are simultaneously diagonalizable. Eingen functions are and We also find Modes with different do not couple each other in perturbation equation. separable

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