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Three Roads To Quantum Gravity

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EPILOGUE:<br />

209<br />

And quantum gravity is nothing if not high risk. The<br />

unfortunate lack of experimental tests means that relatively<br />

large groups of people may work for decades only to ®nd that<br />

they have completely wasted their time, or at least done little<br />

but eliminate what at ®rst seemed to be attractive possibilities<br />

for the theory. Measured sociologically, string theory seems<br />

very healthy at the moment, with perhaps a thousand<br />

practitioners; loop quantum gravity is robust but much less<br />

populous, with about a hundred investigators; other directions,<br />

such as Penrose's twistor theory, are still pursued by<br />

only a handful. But thirty years from now all that will matter<br />

is which parts of which theory were right. And a good idea<br />

from one person is still worth hundreds of people working<br />

incrementally to advance a theory without solving its fundamental<br />

problems. So we cannot allow the politics of the<br />

academy too much in¯uence here, or we shall all end up<br />

doing one thing. If that happens, then a century from now<br />

people may still be writing books about how quantum gravity<br />

is almost solved. If this is to be avoided, all the good ideas<br />

must be kept alive. Even more important is to maintain a<br />

climate in which young people feel there is a place for their<br />

ideas, no matter how initially unlikely or how far from the<br />

mainstream they may seem. As long as there is still room for<br />

the young scientist with the uncomfortable question and the<br />

bright idea, I see nothing to prevent the present rapid rate of<br />

progress from continuing until we have a complete theory of<br />

quantum gravity.<br />

I should like to close this book by sticking out any part of<br />

my neck which is not yet exposed, and making a few<br />

predictions about how the problem of quantum gravity will<br />

in the end be solved. I believe that the huge progress we have<br />

made in the last twenty years is best illustrated by the fact that<br />

it is now possible to make an educated guess about how the<br />

last stages of the search for quantum gravity will go. Until<br />

recently we could have done no more than point to a few good<br />

ideas that were not obviously wrong. Now we have several<br />

proposals on the table that seem right enough and robust<br />

enough, and it is hard to imagine that they are completely<br />

wrong. The picture I have presented in this book was

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