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Quantum radiation of Kerr black hole in de Sitter background

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Abstract

In this paper, we investigate the tunneling of vector boson particles across the event horizon of Kerr–de Sitter black hole by using Hamilton–Jacobi ansatz to Proca equation and WKB approximation . The surface gravity of KdS black hole has been recovered by using direct calculation and Proca equation. These two different methods give the same Hawking temperature at the event horizon.

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Acknowledgements

Y. Kenedy Meitei acknowledges the CSIR for providing the financial support.

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Authors and Affiliations

  1. Mathematics Department, Manipur University, Canchipur, Manipur, 795003, India

    T. Ibungochouba Singh & Y. Kenedy Meitei

  2. Physics Department, Modern College, Imphal, Manipur, India

    I. Ablu Meitei

  3. Physics Department, Manipur University, Canchipur, Manipur, 795003, India

    K. Yugindro Singh

Authors
  1. T. Ibungochouba Singh
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  2. Y. Kenedy Meitei
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  3. I. Ablu Meitei
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  4. K. Yugindro Singh
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Correspondence to T. Ibungochouba Singh.

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Ibungochouba Singh, T., Kenedy Meitei, Y., Ablu Meitei, I. et al. Quantum radiation of Kerr black hole in de Sitter background. Indian J Phys 94, 2061–2064 (2020). https://doi.org/10.1007/s12648-019-01640-2

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  • DOI: https://doi.org/10.1007/s12648-019-01640-2

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