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{{ | {{SeeWikipedia|Hawking radiation}} | ||
In physics, '''Hawking radiation''' (also known as '''Bekenstein-Hawking radiation''') is a thermal radiation with a black body spectrum emitted by black holes due to quantum effects. It is named after the physicist [[Wikipedia:Stephen Hawking|Stephen Hawking]] who provided the theoretical argument for its existence in 1974, and sometimes also after the physicist Jacob Bekenstein who predicted that black holes should have a finite, non-zero temperature and entropy.<ref>[[Wikipedia:Hawking radiation|'''Wikipedia''': ''Hawking radiation'']]</ref><ref>[[Wikipedia:Stephen Hawking|'''Wikipedia''': ''Stephen Hawking'']]</ref> Hawking's analysis became the first convincing insight into a possible theory of [[Wikipedia:Quantum gravity|quantum gravity]]. | In physics, '''Hawking radiation''' (also known as '''Bekenstein-Hawking radiation''') is a thermal radiation with a black body spectrum emitted by black holes due to quantum effects. It is named after the physicist [[Wikipedia:Stephen Hawking|Stephen Hawking]] who provided the theoretical argument for its existence in 1974, and sometimes also after the physicist Jacob Bekenstein who predicted that black holes should have a finite, non-zero temperature and entropy.<ref>[[Wikipedia:Hawking radiation|'''Wikipedia''': ''Hawking radiation'']]</ref><ref>[[Wikipedia:Stephen Hawking|'''Wikipedia''': ''Stephen Hawking'']]</ref> Hawking's analysis became the first convincing insight into a possible theory of [[Wikipedia:Quantum gravity|quantum gravity]]. | ||
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==Sources== | ==Sources== | ||
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[[Category:Physics]] | [[Category:Physics]] |