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Three Roads To Quantum Gravity

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AREA AND INFORMATION<br />

105<br />

physics are expressed as limitations on what we can know.<br />

Einstein's principle of relativity (which was an extension of a<br />

principle of Galileo's) says that we cannot do any experiment<br />

that would distinguish being at rest from moving at a constant<br />

velocity. Heisenberg's uncertainty principle tells us that we<br />

cannot know both the position and momentum of a particle to<br />

arbitrary accuracy. This new limitation tells us there is an<br />

absolute bound to the information available to us about what<br />

is contained on the other side of a horizon. It is known as<br />

Bekenstein's bound, as it was discussed in papers Jacob<br />

Bekenstein wrote in the 1970s shortly after he discovered the<br />

entropy of black holes.<br />

It is curious that, despite everyone who has worked on<br />

quantum gravity having been aware of this result, few seem to<br />

have taken it seriously for the twenty years following the<br />

publication of Bekenstein's papers. Although the arguments<br />

he used were simple, Jacob Bekenstein was far ahead of his<br />

time. The idea that there is an absolute limit to information<br />

which requires each region of space to contain at most a<br />

certain ®nite amount of information was just too shocking for<br />

us to assimilate at the time. There is no way to reconcile this<br />

with the view that space is continuous, for that implies that<br />

each ®nite volume can contain an in®nite amount of information.<br />

Before Bekenstein's bound could be taken seriously,<br />

people had to discover other, independent reasons why space<br />

should have a discrete, atomic structure. <strong>To</strong> do this we had to<br />

learn to do physics at the scale of the smallest possible things.

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