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Eruptive Massive Vector Particles of 5-Dimensional Kerr-Gödel Spacetime

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Abstract

In this paper, we investigate Hawking radiation of massive spin-1 particles from 5-dimensional Kerr-Gödel spacetime. By applying the WKB approximation and the Hamilton-Jacobi ansatz to the relativistic Proca equation, we obtain the quantum tunneling rate of the massive vector particles. Using the obtained tunneling rate, we show how one impeccably computes the Hawking temperature of the 5-dimensional Kerr-Gödel spacetime.

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Acknowledgments

The authors are grateful to the Editor and anonymous Referees for their valuable comments and suggestions to improve the paper. This work was supported by the Chilean FONDECYT Grant No. 3170035 (AÖ).

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Authors and Affiliations

  1. Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4950, Valparaíso, Chile

    A. Övgün

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

    A. Övgün & I. Sakalli

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  1. A. Övgün
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  2. I. Sakalli
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Correspondence to A. Övgün.

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Övgün, A., Sakalli, I. Eruptive Massive Vector Particles of 5-Dimensional Kerr-Gödel Spacetime. Int J Theor Phys 57, 322–328 (2018). https://doi.org/10.1007/s10773-017-3564-7

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  • DOI: https://doi.org/10.1007/s10773-017-3564-7

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