Applying the semi-classical quantum tunneling model, we have studied the Hawking radiation via tunneling from a cylindrically symmetric black hole. The derived results show that the tunneling rate of at the event horizon of the black hole is related to Bekenstein–Hawking entropy and the factual radiation spectrum is not strictly pure thermal, but is consistent with the underlying unitary theory.
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PACS numbers: 04.20.-s, 97.60.Lf.
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Jiang, QQ., Ren, W., Tang, J. et al. Characteristics of Quantum Radiation as Tunneling from a Cylindrically Symmetric Black Hole. Int J Theor Phys 46, 1449–1454 (2007). https://doi.org/10.1007/s10773-006-9284-z
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DOI: https://doi.org/10.1007/s10773-006-9284-z