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Hawking Radiation from the Cylindrical Symmetric Black Hole via Covariant Anomaly

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Abstract

Hawking radiation from the cylindrical symmetric black hole, which is asymptotically anti-de Sitter not only in the transverse direction but also in the string or membrane direction, is discussed from the anomaly point of view. We implement the covariant anomaly cancellation method, the more refined formalism that was proposed by Banerjee and Kulkarni recently than the initial work of Robinson et al., to discuss the near-horizon gauge and gravitational anomalies. Our result shows that Hawking radiation from the cylindrical configurations with horizons also can be reproduced by the anomaly cancellation method.

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Correspondence to Xiao-Xiong Zeng.

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Zeng, XX., Yang, SZ. Hawking Radiation from the Cylindrical Symmetric Black Hole via Covariant Anomaly. Int J Theor Phys 47, 3180–3185 (2008). https://doi.org/10.1007/s10773-008-9753-7

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  • DOI: https://doi.org/10.1007/s10773-008-9753-7

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