应用Parkh-Wilczek等人的半经典量子遂穿模型,研究了任意维拓扑Reissner-Nordstrom-de Sitter 黑洞的Hawking辐射,得出的遂穿辐射谱不再是纯热谱.最后,通过作图对真实谱和纯热谱的差异直观的表示出来.%Applying Parikh-Wilczek's semi-classical quantum tunneling framework, we have investigatel the tunneling characteristic of charged particles via the arbitrarily dimensional topological Reissner-Nordstrom de Sitter black hole, and obtained the actual radiation spectrum that isn't pure thermal. The discrepancies of the actual radiation spectrum and pure thermal one are expressed in figures.
展开▼