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Three Roads To Quantum Gravity

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HOW TO WEAVE A STRING<br />

185<br />

What is remarkable ± indeed, what is almost a miracle ± is<br />

that the hardest problem faced by each group was precisely<br />

the key problem that the other had solved. Loop quantum<br />

gravity tells us how to make a background independent<br />

quantum theory of space and time. It offers a lot of scope to<br />

the M theorist looking for a way to make string theory<br />

background independent. On the other hand, if we believe<br />

that strings must emerge from the description of space and<br />

time provided by loop quantum gravity, we then have a lot of<br />

information about how to formulate the theory so that it does<br />

describe classical spacetime. The theory must be formulated<br />

in such a way that the gravitons appear not on their own, but<br />

as modes of excitations of extended objects that behave as<br />

strings.<br />

It is then possible to entertain the following hypothesis:<br />

string theory and loop quantum gravity are each part of a<br />

single theory. This new theory will have the same relationship<br />

to the existing ones as Newtonian mechanics has to<br />

Galileo's theory of falling bodies and Kepler's theory of<br />

planetary orbits. Each is correct, in the sense that it describes<br />

to a good approximation what is happening in a certain<br />

limited domain. Each solves part of the problem. But each<br />

also has limits which prevent it from forming the basis for a<br />

complete theory of nature. I believe that this the most likely<br />

way in which the theory of quantum gravity will be completed,<br />

given the present evidence. In this penultimate<br />

chapter I shall describe some of this evidence, and the<br />

progress that has recently been made towards inventing a<br />

theory that uni®es string theory and loop quantum gravity.<br />

As a ®rst step we can ask for a rough picture of how the two<br />

theories might ®t together. As it happens, there is a very<br />

natural way in which strings and loops can emerge from the<br />

same theory. The key to this is a subtlety that I have so far only<br />

hinted at. Both loop quantum gravity and string theory<br />

describe physics on very small scales, roughly the Planck<br />

length. But the scale that sets the size of strings is not exactly<br />

equal to the Planck length. That scale is called the string<br />

length. The ratio of the Planck length to the string length is a<br />

number of great signi®cance in string theory. It is a kind of

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