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Three Roads To Quantum Gravity

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HOW TO WEAVE A STRING<br />

193<br />

may be the birth of a new universe inside the horizon. This<br />

idea has been studied using approximation techniques in<br />

which the matter forming the black hole is treated quantum<br />

theoretically, but the geometry of spacetime is treated as in<br />

the classical theory. The results do suggest that the singularities<br />

are eliminated, and one may hope that this will be<br />

con®rmed by an exact treatment. But, at least so far, neither<br />

string theory nor loop quantum gravity, nor any other<br />

approach, has been strong enough to study this problem.<br />

Until 1995 no approach to quantum gravity could describe<br />

black holes in any detail. None could explain the meaning of<br />

the entropy of a black hole or tell us anything about what<br />

black holes look like when probed on the Planck scale. Now<br />

we have two approaches that are able to do all these things, at<br />

least in some cases. Every time we are able to calculate<br />

something about a black hole, in either theory, it comes out<br />

right. There are many questions we still cannot answer, but it<br />

is dif®cult to avoid the impression that we are ®nally understanding<br />

something real about the nature of space and time.<br />

Furthermore, the fact that both string theory and loop<br />

quantum gravity both succeed in giving the right answers<br />

about quantum black holes is strong evidence that the two<br />

approaches may be revealing different sides of a single theory.<br />

Like Galileo's projectiles and Kepler's planets, there is more<br />

and more evidence that we are glimpsing the same world<br />

through different windows. <strong>To</strong> ®nd the relation of his work to<br />

Kepler's, Galileo would only have had to imagine throwing a<br />

ball far enough and fast enough that it became a moon. Kepler,<br />

from his point of view, could have imagined what a planet<br />

orbiting very close to the Sun might have looked like to<br />

people living on the Sun. In the present case, we only have to<br />

ask whether a string can be woven from a network of loops, or<br />

whether, if we look closely enough at a string, we can see the<br />

discrete structures of the loops. I personally have little doubt<br />

that in the end loop quantum gravity and string theory will be<br />

seen as two parts of a single theory. Whether it will take a<br />

Newton to ®nd that theory, or whether it is something we<br />

mortals can do, is something that only time will tell.

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