Effective state, Hawking radiation and quasi-normal modes for Kerr black holes

Abstract

The non-strictly continuous character of the Hawking radiation spectrum generates a natural correspondence between Hawking radiation and black hole (BH) quasi-normal modes (QNM). In this work, we generalize recent results on this important issue to the framework of Kerr BHs (KBH). We show that also for the KBH, QNMs can be naturally interpreted in terms of quantum levels. Thus, the emission or absorption of a particle is in turn interpreted in terms of a transition between two different levels. At the end of the paper, we also generalize some concepts concerning the "effective state" of a KBH.

10 pages, to appear in Journal of High Energy Physics

References in corpus (5)

• The physical interpretation of the spectrum of black hole quasinormal modes
• Area spectrum of rotating black holes via the new interpretation of quasinormal modes
• On the Kerr Quantum Area Spectrum
• Effective temperature, Hawking radiation and quasinormal modes
• Effective temperature for black holes

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