Resumen
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.
Idioma original | Inglés |
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Páginas (desde-hasta) | 404-407 |
Número de páginas | 4 |
Publicación | Journal of Experimental and Theoretical Physics |
Volumen | 121 |
N.º | 3 |
DOI | |
Estado | Publicada - 1 sep. 2015 |
Publicado de forma externa | Sí |