Rendition of the side view of a black hole, predicted to exist in 1915 by American mathematical physicist William Sidis, showing Hawking radiation shooting out the sides, as was predicted to exist in 1974 by British astrophysicist Stephen Hawking, following earlier circa 1970 discussion between American theoretical physicist John Wheeler, coiner of the term “black hole” (1967), and his graduate student Mexican-born Jewish physicist Jacob Bekenstein as whether or not black holes flout the second law of thermodynamics. [8] |
See main: Black hole thermodynamicsThe first ideas as to what happens to the lost information or energy-matter falling into a black hole, in the context of entropy increase, traces to early 1970s discussions between Wheeler and his graduate student Mexican-born Jewish physicist Jacob Bekenstein. In 1971, Wheeler pointed out to Bekenstein that black holes seem to flout the second law of thermodynamics. [5] In 1972, to remedy this issue, Bekenstein suggested that black holes should have a well-defined entropy and went on to formulate a generalized second law of black hole thermodynamics which states that “the sum of black hole entropy and ordinary entropy outside a black hole never decreases.” To find and measure this “black hole entropy”, Bekenstein reasoned that, because of the effect that the massive gravity of black holes pulls light, energy, and matter into its body, according to German-born American Albert Einstein’s mass-energy relation E=mc², a black hole's entropy increase must be proportional or related to its surface area.