Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes

Abstract

In this article we present results for tensor graviton modes (in seven dimensions and greater, $n\ge 3$) for greybody factors of Kerr-dS black holes and for Hawking radiation from simply rotating (n+4)-dimensional Kerr black holes. Although there is some subtlety with defining the Hawking temperature of a Kerr-dS black hole, we present some preliminary results for emissions assuming the standard Hawking normalization and a Bousso-Hawking-like normalization.

12 pages, 18 figures

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Cited by in corpus (17)

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• Hawking emission from quantum gravity black holes
• Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
• Phenomenology of Production and Decay of Spinning Extra-Dimensional Black Holes at Hadron Colliders
• Greybody factors for rotating black holes in higher dimensions
• Effective Temperatures and Radiation Spectra for a Higher-Dimensional Schwarzschild-de-Sitter Black-Hole
• Graviton Emission in the Bulk by a Simply Rotating Black Hole
• Asymptotic iteration method for spheroidal harmonics of higher-dimensional Kerr-(A)dS black holes
• Hawking Radiation from Higher-Dimensional Black Holes
• Emission of Massive Scalar Fields by a Higher-Dimensional Rotating Black-Hole
• Absorption Cross-section and Decay Rate of Rotating Linear Dilaton Black Holes
• Quasi-normal modes for doubly rotating black holes
• Spin-3/2 fields in $D$-dimensional Schwarzschild black hole space-times
• Angular profile of emission of non-zero spin fields from a higher-dimensional black hole
• Gravitational parameter estimation in a waveguide
• Angular Eigenvalues of Higher-Dimensional Kerr-(A)dS Black Holes with Two Rotations
• Superradiant instability of the Kerr brane