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Three Roads To Quantum Gravity

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WHAT CHOOSES THE LAWS OF NATURE?<br />

203<br />

directly contradicts a prediction of Newton's theory, we can<br />

deduce that, with probability 1, Newton's theory is false.<br />

It is a little harder to pose the question in Einstein's theory<br />

of spacetime, as that theory has an in®nite number of<br />

solutions. In many of them space is approximately ¯at, but<br />

in many of them it is not. Given that there are an in®nite<br />

number of examples of each, it is not straightforward to ask<br />

how probable it would be, were the solution chosen at<br />

random, that the resulting universe would look almost like<br />

three-dimensional Euclidean space.<br />

It is easier to ask the question in a quantum theory of<br />

gravity. <strong>To</strong> ask it we need a form of the theory that does not<br />

assume the existence of any classical background geometry<br />

for space. Loop quantum gravity is an example of such a<br />

theory. As I explained in Chapters 9 and 10, it tells us that<br />

there is an atomic structure to space, described in terms of the<br />

spin networks invented by Roger Penrose. As we saw there,<br />

each possible quantum state for the geometry of space can be<br />

described as a graph such as that shown in Figures 24 to 27.<br />

We can then pose the question this way: how probable is it<br />

that such a graph represents a geometry for space that would<br />

be perceived by observers like us, living on a scale hugely<br />

bigger than the Planck scale, to be an almost Euclidean threedimensional<br />

space? Well, each node of a spin network graph<br />

corresponds to a volume of roughly the Planck length on each<br />

side. There are then 10 99 nodes inside every cubic centimetre.<br />

The universe is at least 10 27 centimetres in size, so it contains<br />

at least 10 180 nodes. The question of how probable it is that<br />

space looks like an almost ¯at Euclidean three-dimensional<br />

space all the way up to cosmological scales can then be posed<br />

as follows: how probable is it that a spin network with 10 180<br />

nodes would represent such a ¯at Euclidean geometry?<br />

The answer is, exceedingly improbable! <strong>To</strong> see why, an<br />

analogy will help. <strong>To</strong> represent an apparently smooth, featureless<br />

three-dimensional space, the spin network has to have<br />

some kind of regular arrangement, something like a crystal.<br />

There is nothing special about any position in Euclidean space<br />

that distinguishes it from any other position. The same must<br />

be true, at least to a good approximation, of the quantum

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