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Three Roads To Quantum Gravity

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KNOTS, LINKS AND KINKS<br />

127<br />

What we had done was to apply the usual methods for<br />

constructing a quantum theory to the simple form of the<br />

equations for general relativity that Sen and Ashtekar had<br />

discovered. These led to the equations for the quantum theory<br />

of gravity. These equations had ®rst been written down in the<br />

1960s, by Bryce DeWitt and John Wheeler, but we found new<br />

forms for them which were dramatically simpler. We had to<br />

plug into these equations formulas that described possible<br />

quantum states of the geometry of space and time. On an<br />

impulse I tried something that Louis Crane and I had played<br />

with, which was to build these states directly from the<br />

expressions Polyakov used to describe the quantized loops<br />

of electric ®elds. What we found was that, as long as the loops<br />

did not intersect, they satis®ed the equations. They looked<br />

like the loops in Figure 23.<br />

FIGURE 23<br />

<strong>Quantum</strong> states of the geometry of space are expressed in loop quantum<br />

gravity in terms of loops. These states are exact solutions to the equations of<br />

quantum gravity, as long as there are no intersections or kinks in the loops.<br />

It took us a few days of hard work to ®nd still more<br />

solutions. We found that even if the loops intersected, we<br />

could still combine them to make solutions provided certain<br />

simple rules were obeyed. In fact, we could write down an<br />

in®nite number of these states ± all we had to do was draw<br />

loops and apply some simple rules whenever they intersected.

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