2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/109949Recent work that treats the Hawking radiation as a semi-classical tunnelling process from the four-dimensional Schwarzschild and Reissner-Nordstrom black holes is extended to the case of higher dimensional Reissner-Nordstrom-de Sitter black holes. The result shows that the tunnelling rate is related to the change of Bekenstein-Hawking entropy and the exact radiant spectrum is no longer precisely thermal after considering the black hole background as dynamical and incorporating the self-gravitation effect of the emitted particles when the energy conservation and electric charge conservation are taken into account.13 pages, no figure, enlarged versionHigh Energy Physics - TheoryGeneral Relativity and Quantum Cosmologytext