Energy Loss of a Heavy Particle near 3D Charged Rotating Hairy Black Hole

Abstract

In this paper we consider charged rotating black hole in 3 dimensions with an scalar charge and discuss about energy loss of heavy particle moving near the black hole horizon. We also study quasi-normal modes and find dispersion relations. We find that the effect of scalar charge and electric charge is increasing energy loss.

Accepted for publication in EPJC. arXiv admin note: text overlap with arXiv:1205.4254 by other authors

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Cited by in corpus (4)

• Thermodynamics of Higher Order Entropy Corrected Schwarzschild-Beltrami-de Sitter Black Hole
• Einstein-Born-Infeld black holes with a scalar hair in three-dimensions
• Gravity coupled to a scalar field from a Chern-Simons action: describing rotating hairy black holes and solitons with gauge fields
• The Hawking temperature in the context of dark energy for four-dimensional asymptotically AdS black holes with scalar hair