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- W2207257083 abstract "In 1974, the British physicist Stephen Hawking discovered that black holes have a characteristic temperature and are therefore capable of emitting radiation. Given the scientific importance of this discovery, there is a profuse literature on the subject. Nevertheless, the available literature ends up being either too simple, which does not convey the true physical significance of the issue, or too technical, which excludes an ample segment of the audience interested in science, such as physics teachers and their students. The present article seeks to remedy this shortcoming. It develops a simple and plausible argument that provides insight into the fundamental aspects of Hawking's discovery, which leads to an approximate equation for the so-called Hawking temperature. The exposition is mainly intended for physics teachers and their students, and it only requires elementary algebra, as well as basic notions of Newtonian mechanics and quantum theory." @default.
- W2207257083 created "2016-06-24" @default.
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- W2207257083 date "2015-12-16" @default.
- W2207257083 modified "2023-09-25" @default.
- W2207257083 title "Hawking temperature: an elementary approach based on Newtonian mechanics and quantum theory" @default.
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- W2207257083 doi "https://doi.org/10.1088/0031-9120/51/1/015010" @default.
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