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Thermal radiation of scalar particles and Dirac fermions from squashedcharged rotating five-dimensional black holes is considered. To obtaintemperature of the black holes we use the tunnelling method. In case of scalarparticles we make use of the Hamilton-Jacobi equation. To consider tunnellingof fermions the Dirac equation was investigated. The examination shows thatradial parts of the action for scalar particles and fermions in quasi-classicallimit in the vicinity of horizon are almost the same and as a consequence itgives rise to the identical expressions for the temperature in both cases.

Tunnelling of scalar and Dirac particles from squashed charged rotating Kaluza-Klein black holes