That breakthrough led us to new ways of understanding not only black holes but the ways that universe grows and changes over time. And much of it can be expressed in just a few letters:
The S that the equation serves to calculate is entropy: a complicated but significant part of black holes, that can be understood as a measure of how much disorder is present in the system. Sometimes the letter is written with a little “BH” next to it, standing for Professor Hawking and Jacob Bekenstein, the other scientist who did so much to help understand black holes.
The rest gives the important numbers required to calculate that entropy. The h is the Planck constant, so important in quantum mechanics; the G is Newton’s constant, used to understand gravity; the A refers to the area of the event horizon; the c is the speed of light, made so famous by Einstein’s great formula; and the k is Boltzmann’s constant, which is a way of understanding how energy relates to temperature.
All of which may appear to be a little complicated. But, as ever, Professor Hawking gave an incredibly simple explanation of how he arrived at the itself deceptively simple formula.
“In particular, I wondered, can one have atoms in which the nucleus is a tiny primordial black hole, formed in the early universe?” he wrote in 2002, during the celebrations of his 60th birthday. “To answer this, I studied how quantum fields would scatter off a black hole. I was expecting that part of an incident wave would be absorbed, and the remainder scattered.
Stephen Hawking: a life in pictures
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“But to my great surprise, I found there seemed to be emission from the black hole. At first, I thought this must be a mistake in my calculation. But what persuaded me that it was real, was that the emission was exactly what was required to identify the area of the horizon with the entropy of a black hole.
“I would like this simple formula to be on my tombstone.”
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