This chapter is devoted to the most important property of black holes when quantum effects are included, Hawking radiation. Black holes emit quantum radiation with an almost perfect black body spectrum, and therefore ultimately evaporate. We outline the computation and properties of Hawking radiation from both four-dimensional and higher-dimensional black holes.
CITATION STYLE
Calmet, X., Carr, B., & Winstanley, E. (2014). Hawking Radiation and Black Hole Evaporation. In SpringerBriefs in Physics (Vol. Part F878, pp. 27–50). Springer VS. https://doi.org/10.1007/978-3-642-38939-9_3
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