On the relationship between quantum cosmology and the dimensions of the superstring

Physics – Nuclear Physics

Scientific paper

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Scientific paper

We examine the possibility of constraining the dimensions M + 1 and N of the physical space-time and the internal space, respectively, of the D(= M + N + 1)-dimensional theory L=√-ĝ(1/2K-2R + 1/2ΦAΦBĝAB), which is the field-theory limit of both the bosonic string and the superstring when higher-order terms K2φ-4/(D-2)R2 and K2φ-8/(D-2)ĤABC 2 can be ignored, where φ --- exp(1/2√(D-2)KΦ) is the dilation. The Wheeler-De Witt equation for the wave function of the Universe ψ is derived for the topology R × SM × RN, where the space RN is to approximate a (Ricci-flat) Kähler space. By requiring that ψ remain finite at the origin (zero (D - 1)-volume) and assuming that the eigenvalue of the dilaton energy-momentum tensor vanishes, we show that the metric initially possesses the ``no-scale'' form ds2 = -n2 dt2 + a2(t)dx2 + a-2(t)dy2, provided that (M - N)2 = M + N. This condition includes not only the cases D = 26 (M = 10, N = 15) and D = 10 (M = 3, N = 6), for which the dilaton beta function βφ vanishes (to lowest order in α') in the bosonic string and the superstring, respectively, but also the case D = 5 (M = 3, N = 1) corresponding to the original Kaluza-Klein theory. Since M = 3 for the physical space, then the superstring is allowed, while the bosonic string appears to be ruled out.
The analysis was motivated by a preprint of Enqvist, Mohanty and Nanopoulos.

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