Hawking Radiation of Spin-1 Particles From Three Dimensional Rotating Hairy Black Hole

Abstract

In the present article, we study the Hawking radiation (HR) of spin-1 particles -- so-called vector particles -- from a three dimensional (3D) rotating black hole with scalar hair (RBHWSH) using Hamilton-Jacobi (HJ) ansatz. Putting the Proca equation amalgamated with the WKB approximation in process, the tunneling spectrum of vector particles is obtained. We recover the standard Hawking temperature corresponding to the emission of these particles from RBHWSH.

minor corrections, corrected typos

References in corpus (8)

• Subtleties in the quasi-classical calculation of Hawking radiation
• Black hole radiation of spin-1 particles in (1+2) dimensions
• Black hole emission of vector particles in (1+1) dimensions
• Hawking radiation from the quantum Lemaitre-Tolman-Bondi model
• Gravitational Lensing Effect on the Hawking Radiation of Dyonic Black Holes
• Thermodynamics of rotating black holes with scalar hair in three dimensions
• Vector particles tunneling from BTZ black holes
• Backreaction due to quantum tunneling and modification to the black hole evaporation process

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