Rotating black holes at future colliders II: Anisotropic scalar field emission
Daisuke Ida (Gakushuin U.), Kin-ya Oda (Bonn U.), Seong Chan Park, (Cornell U., LEPP)
TL;DR
This paper investigates the emission of scalar fields from higher-dimensional rotating black holes at future colliders, extending previous work to general frequencies without low-frequency approximations.
Contribution
It provides a comprehensive analysis of scalar field emission from rotating black holes in arbitrary dimensions beyond the low-frequency limit.
Findings
Scalar emission spectra computed for various dimensions
No reliance on low-frequency approximation in analysis
Enhanced understanding of black hole evaporation processes
Abstract
This is the sequel to the first paper of the series, where we have discussed the Hawking radiation from five-dimensional rotating black holes for spin 0, 1/2 and 1 brane fields in the low frequency regime. We consider the emission of a brane localized scalar field from rotating black holes in general space-time dimensions without relying on the low frequency expansions.
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