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Charged Particles’ Tunneling from Hot-NUT-Kerr-Newman-Kasuya Spacetime

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Abstract

We study the Hawking radiation as charged particles’ tunneling across the horizons of the Hot-NUT-Kerr-Newman-Kasuya spacetime by considering the spacetime background as dynamical and incorporating the self-gravitation effect of the emitted particles when the energy conservation, the angular momentum conservation, and the electric charge conservation are taken into account. Our result shows that the tunneling rate is related to the change of Bekenstein-Hawking entropy and the radiant spectrum is not pure thermal, but is consistent with an underlying unitary theory. The emission process is a reversible one, and the information is preserved as a natural result of the first law of black hole thermodynamics.

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Authors and Affiliations

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

    M. Hossain Ali

  2. The Abdus Salam International Centre for Theoretical Physics, Strada Costiera 11, 34014, Trieste, Italy

    M. Hossain Ali

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  1. M. Hossain Ali
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Correspondence to M. Hossain Ali.

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To my teacher late Prof. Mainuddin Ahmed.

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Ali, M.H. Charged Particles’ Tunneling from Hot-NUT-Kerr-Newman-Kasuya Spacetime. Int J Theor Phys 47, 2203–2217 (2008). https://doi.org/10.1007/s10773-008-9652-y

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