Hawking radiation and Quasinormal modes

2005/10/03 by SangChul Yoon, Yoon, SangChul · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Noncommutative and Quantum Gravity Theories #Quantum Electrodynamics and Casimir Effect #gr-qc

paper · pdf · doi:10.48550/arxiv.gr-qc/0510009

6 pages, references added

openalex publication_date 2005/10/03 · arxiv created 2005/10/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The spectrum of Hawking radiation by quantum fields in the curved spacetime is continuous, so the explanation of Hawking radiation using quasinormal modes can be suspected to be impossible. We find that quasinormal modes do not explain the relation between the state observed in a region far away from a black hole and the short distance behavior of the state on the horizon.

Citations

• Quasinormal modes: the characteristic `sound' of black holes and neutron stars
• Particle creation by black holes
• Stability of a Schwarzschild Singularity

Cited by

• The Geometry of Black Hole Singularities

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