Do all D-dimensional Schwarzschild black holes behave as one-dimensional entropy emitters?
Perfect black-body emitters in a flat three-dimensional space are characterized by the well-known relation S˙flat3D=(32π2AP3/1215ħ3)1/4, where S˙flat3D and P are respectively the entropy and energy emission rates out of the 3-D hot body, and A is the 2-D surface area of the emitting body. However, B...
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| Format: | Article |
| Language: | English |
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Elsevier
2015-06-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269315003056 |