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- W2314745947 abstract "Since Parikh and Wilczek adopted a semi-classical tunnelling picture to investigate Hawking radiation of static and spheri-cally symmetric black holes in the year of 2000, their work had been paid much attention to and extended to various other cases. However, in almost all of the subsequent papers, there exist two important shortcomings: (1) different from the massless case, one has to use a different and very lame approach to derive the geodesic equation obeyed by the massive particles; (2) to deal with the tunnelling radiation of a rotating black hole, one is limited to use the dragging coordinates to do the job. In this paper, we shall adopt a new idea to re-investigate the tunnelling radiation of the Kerr black holes, that is, by applying the method of Lagrangian analysis in Classical Mechanics, we will make a new, consistent and unified treatment on the geodesics of massive and massless particles from Kerr black holes. Moreover, we can simultaneously overcome the two main defects mentioned above, thus making Parikh-Wilczeks semi-classical approach more perfect and consistent" @default.
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- W2314745947 date "2013-02-01" @default.
- W2314745947 modified "2023-09-23" @default.
- W2314745947 title "New treatment on tunneling radiation from Kerr black holes" @default.
- W2314745947 doi "https://doi.org/10.1360/132012-382" @default.
- W2314745947 hasPublicationYear "2013" @default.
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