Binary_Bark
Forging
In the early 1970s, people studying general relativity, our modern theory of gravity, noticed rough similarities between the properties of black holes and the laws of thermodynamics. Stephen Hawking proved that the area of a black hole’s event horizon — the surface that marks its boundary — cannot decrease. That sounded suspiciously like the second law of thermodynamics, which says entropy — a measure of disorder — cannot decrease.
Yet at the time, Hawking and others emphasized that the laws of black holes only looked like thermodynamics on paper; they did not actually relate to thermodynamic concepts like temperature or entropy.
Then in quick succession, a pair of brilliant results — one by Hawking himself — suggested that the equations governing black holes were, in fact, actual expressions of the thermodynamic laws applied to black holes. In 1972, Jacob Bekenstein argued that a black hole’s surface area was proportional to its entropy, and thus the second law similarity was a true identity. And in 1974, Hawking found that black holes appear to emit radiation — what we now call Hawking radiation — and this radiation would have exactly the same “temperature” in the thermodynamic analogy.
More At: https://www.quantamagazine.org/craig-callender-are-we-all-wrong-about-black-holes-20190905/