Abstract:
We study the Hawking radiation of spin-1 particles (so-called vector particles) from a three-dimensional
rotating black hole with scalar hair using a Hamilton–Jacobi ansatz. Using the Proca equation in the
WKB approximation, we obtain the tunneling spectrum of vector particles. We recover the standard Hawking
temperature corresponding to the emission of these particles from a rotating black hole with scalar hair
Description:
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