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Tunneling and Temperature of Demiański-Newman Black Holes

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Abstract

We investigate Hawking radiation of charged and magnetized (scalar /fermion) particles from Demiański-Newman (DN) black holes using Hamilton-Jacobi (HJ) ansatz. Taking into account conservation of energy and the backreaction of particles to the spacetime, we calculate the emission rate and find it proportional to the change of Bekenstein-Hawking entropy. The radiation spectrum deviates from the precisely thermal one and is accordant with that obtained by the null geodesic method, but its physical picture is more clear. The investigation specifies a quantum-corrected radiation temperature dependent on the black hole background and the radiation particle’s energy, angular momentum, and charges.

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Authors and Affiliations

  1. Department of Applied Mathematics, University of Rajshahi, Rajshahi, 6205, Bangladesh

    Md. Hossain Ali

  2. Department of Mathematics, Shahjalal University of Science & Technology, Sylhet, 3100, Bangladesh

    Kausari Sultana

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  1. Md. Hossain Ali
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  2. Kausari Sultana
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Correspondence to Md. Hossain Ali.

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Ali, M.H., Sultana, K. Tunneling and Temperature of Demiański-Newman Black Holes. Int J Theor Phys 53, 4035–4048 (2014). https://doi.org/10.1007/s10773-014-2154-1

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  • DOI: https://doi.org/10.1007/s10773-014-2154-1

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