Abstract
Using Proca equation and WKB approximation, we investigate Hawking radiation of vector particles via tunneling from 4-dimensional Kerr-de Sitter black hole and 5-dimensional Schwarzschild-Tangherlini black hole. The results show that the tunneling rates and Hawking temperatures are dependent on the properties of spacetime (event horizon, mass and angular momentum). Besides, our results are the same as scalars and fermions tunneling from 4-dimensional Kerr-de Sitter black hole and 5-dimensional Schwarzschild-Tangherlini black hole.
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Acknowledgements
This work is supported by the Natural Science Foundation of China (Grants No. 11573022 and No. 11205125), the Sichuan Province Science Foundation for Youths (Grant No. 2014JQ0040), and the Innovative Research Team in China West Normal University (Grant No. 438061).
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Feng, Z., Chen, Y. & Zu, X. Hawking radiation of vector particles via tunneling from 4-dimensional and 5-dimensional black holes. Astrophys Space Sci 359, 48 (2015). https://doi.org/10.1007/s10509-015-2498-x
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DOI: https://doi.org/10.1007/s10509-015-2498-x