<P> Hawking radiation, also known as Hawking--Zel'dovich radiation,, or Hawking--Bekenstein radiation, is blackbody radiation that is predicted to be released by black holes, due to quantum effects near the event horizon . It is named after the physicist Stephen Hawking, who provided a theoretical argument for its existence in 1974, and Jacob Bekenstein, who predicted that black holes should have a finite entropy . </P> <P> Hawking's work followed his visit to Moscow in 1973 where the Soviet scientists Yakov Zel'dovich and Alexei Starobinsky showed him that, according to the quantum mechanical uncertainty principle, rotating black holes should create and emit particles . Hawking radiation reduces the mass and energy of black holes and is therefore also known as black hole evaporation . Because of this, black holes that do not gain mass through other means are expected to shrink and ultimately vanish . Micro black holes are predicted to be larger emitters of radiation than larger black holes and should shrink and dissipate faster . </P>

Who predicted that black holes emit radiation and what it is called
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