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| | 4.2 String theory |
 | | Unlike supergravity, string theory appears to be a consistent and well-defined theory of quantum gravity, and therefore calculating the value of the cosmological constant should, at least in principle, be possible. |
 | | More generally, it is now understood that (at least in some circumstances) string theory obeys the ``holographic principle'', the idea that a theory with gravity in D dimensions is equivalent to a theory without gravity in D -1 dimensions [235, 234]. |
 | | Kachru, Kumar and Silverstein [139] have constructed such a string theory, and argue that the perturbative contributions to the cosmological constant should vanish (although the actual calculations are somewhat delicate, and not everyone agrees [136]). |
| relativity.livingreviews.org /Articles/lrr-2001-1/node18.html (902 words) |
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