We extend Parikh's recent work to the arbitrarily dimensional Schwarzschild black holes whose Arnowitt–Deser–Misner (ADM) mass is identical to its mass parameter. We view Hawking radiation as a tunnelling process across the event horizon. From the tunnelling probability we also find a leading correction to the semiclassical emission rate. The result consists with an underlying unitary theory.
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Jun Ren (2005) studied this question.
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