The derivation of Hawking temperature stems from the principles of quantum mechanics applied to black holes. Stephen Hawking proposed that particle-antiparticle pairs are constantly being created in the vacuum of space. Near the event horizon of a black hole, one of these particles can fall into the black hole while the other escapes, leading to the phenomenon of Hawking radiation. This escaping particle appears as radiation emitted from the black hole, and its energy corresponds to a temperature, known as the Hawking temperature.
The temperature can be derived using the formula:
where:
This equation shows that the temperature of a black hole is inversely proportional to its mass, implying that smaller black holes emit more radiation and thus have a higher temperature than larger ones.
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