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Three Roads To Quantum Gravity

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202 THREE ROADS TO QUANTUM GRAVITY<br />

values of the masses of the elementary particles and the<br />

strengths of the fundamental forces. One can estimate the<br />

probability that the constants in our standard theories of the<br />

elementary particles and cosmology would, were they chosen<br />

randomly, lead to a world with carbon chemistry. That<br />

probability is less than one part in 10 220 . But without carbon<br />

chemistry the universe would be much less likely to form<br />

large numbers of stars massive enough to become black holes,<br />

and life would be very unlikely to exist. This is evidence for<br />

some mechanism of self-organization, because what we mean<br />

by self-organization is a system that evolves from a more<br />

probable to a less probable con®guration. So the best argument<br />

we can give that such a mechanism has operated in the<br />

past must have two parts: ®rst, that the system be structured<br />

in some way that is enormously improbable; and second, that<br />

nothing acting from the outside could have imposed that<br />

organization on the system. In the case of our universe we are<br />

taking this second part as a principle. We then satisfy both<br />

parts of the argument, and are justi®ed in seeking mechanisms<br />

of self-organization to explain why the constants in the<br />

laws of nature have been chosen so improbably.<br />

But there is an even better piece of evidence for the same<br />

conclusion. It is right in front of us, and so familiar that it is<br />

dif®cult at ®rst to understand that it also is a structure of<br />

enormous improbability. This is space itself. The simple fact<br />

that the world consists of a three-dimensional space, which is<br />

almost Euclidean in its geometry, and which extends for huge<br />

distances on all sides, is itself an extraordinarily improbable<br />

circumstance. This may seem absurd, but this is only because<br />

we have become so mentally dependent on the Newtonian<br />

view of the world. For how probable the arrangement of the<br />

universe is cannot be answered a priori. Rather, it depends on<br />

the theory we have about what space is. In Newton's theory<br />

we posit that the world lives in an in®nite three-dimensional<br />

space. On this assumption, the probability of us perceiving a<br />

three-dimensional space around us, stretching in®nitely in all<br />

directions, is 1. But of course we know that space is not<br />

exactly Euclidean, only approximately so. On large scales<br />

space is curved because gravity bends light rays. Since this

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