Decay of Dirac massive hair in the background of a spherical black hole

2008/05/06 by R. Moderski, Rafał Moderski, Marek Rogatko · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.77.124007

published as Phys.Rev.D77:124007,2008 · 8 pages, 5 figures, RevTex, to be published in Phys.Rev.D15

arxiv created 2008/05/06 · openalex publication_date 2008/06/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The intermediate and late-time behavior of massive Dirac hair in the static spherically general black hole spacetime is studied. It is revealed that the intermediate asymptotic pattern of decay of massive Dirac spinor hair is dependent on the mass of the field under consideration as well as the multiple number of the wave mode. The long-lived oscillatory tail observed at timelike infinity in the considered background decays slowly as t^\ensuremath-5/6.

Citations

• Abelian Higgs hair for rotating and charged black holes
• Decay of massive scalar hair in the background of a dilaton gravity black hole
• Influence of Lorentz violation on Dirac quasinormal modes in the Schwarzschild black hole spacetime
• Late-time behavior of massive Dirac fields in a Schwarzschild background
• Late-time behavior of stellar collapse and explosions. I. Linearized perturbations
• Vortices and extreme black holes: The question of flux expulsion

Cited by

• Collapse of charged scalar field in dilaton gravity

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