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Hawking Radiation of Scalar and Vector Particles from 5D Myers-Perry Black Holes

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Abstract

In the present paper we explore the Hawking radiation as a quantum tunneling effect from a rotating 5 dimensional Myers-Perry black hole (5D-MPBH) with two independent angular momentum components. First, we investigate the Hawking temperature by considering the tunneling of massive scalar particles and spin-1 vector particles from the 5D-MPBH in the Painlevé coordinates and then in the corotating frames. More specifically, we solve the Klein-Gordon and Proca equations by applying the WKB method and Hamilton-Jacobi equation in both cases. Finally, we recover the Hawking temperature and show that coordinates systems do not affect the Hawking temperature.

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Acknowledgments

We thank the anonymous referees and editor for their valuable and constructive suggestions.

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Authors and Affiliations

  1. Physics Department, State University of Tetovo, Ilinden Street nn, 1200, Tetovo, Macedonia

    Kimet Jusufi

  2. Physics Department, Eastern Mediterranean University, Famagusta, Northern Cyprus, Mersin 10, Turkey

    Ali Övgün

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  1. Kimet Jusufi
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  2. Ali Övgün
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Correspondence to Ali Övgün.

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Jusufi, K., Övgün, A. Hawking Radiation of Scalar and Vector Particles from 5D Myers-Perry Black Holes. Int J Theor Phys 56, 1725–1738 (2017). https://doi.org/10.1007/s10773-017-3317-7

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  • DOI: https://doi.org/10.1007/s10773-017-3317-7

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