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12 - M/string theory and anthropic reasoning

Published online by Cambridge University Press:  05 July 2014

By
Renata Kallosh
Edited by
Bernard Carr
Renata Kallosh
Affiliation:
Stanford University
Bernard Carr
Affiliation:
Queen Mary University of London
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Summary

Introduction

After the development of inflationary cosmology, anthropic reasoning (AR) became one of the most important methods in theoretical cosmology. However, until recently it was not in the toolbox of many high-energy physicists studying 11- or 10-dimensional M/string theory and supergravity. The attitude of high-energy physicists changed dramatically in 1998, when the physics community was shocked by the new cosmological observations suggesting that we may live in a world with a tiny cosmological constant, Λ ~ 10–120M4P, with a weird combination of matter and dark energy.

The recent WMAP observations seem to confirm the earlier data and also support the existence of an inflationary stage in the very early Universe. In view of the accumulating observational evidence, the level of tolerance towards AR is currently increasing. More people are starting to take it into consideration when thinking about cosmology from the perspective of M/string theory and particle physics. I belong to this group, and I recently had two rather impressive encounters with AR that I would like to discuss in this chapter.

In the first encounter, Andrei Linde and I considered a model of maximal supergravity related to the 11-dimensional M-theory, which has a 4-dimensional de Sitter (dS) solution with spontaneously broken super-symmetry [1]. We found that this model offers an interesting playground for the successful application of AR.

Type
Chapter
Information
Universe or Multiverse? , pp. 191 - 210
Publisher: Cambridge University Press
Print publication year: 2007

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References

[1] R., Kallosh and A., Linde. M-theory, cosmological constant and anthropic principle. Phys. Rev. D 67 (2003), 023510.Google Scholar
[2] S., Kachru, R., Kallosh, A., Linde and S. R., Trivedi. de Sitter vacua in string theory. Phys. Rev. D 68 (2003), 046005 [hep-th/0301240].Google Scholar
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[9] S., Weinberg. Anthropic bound on the cosmological constant. Phys. Rev. Lett. 59 (1987), 2607.Google Scholar
[10] G., Efstathiou. An anthropic argument for a cosmological constant. Mon. Not. Roy. Astron. Soc. 274 (1995), L73.Google Scholar
[11] A., Vilenkin. Predictions from quantum cosmology. Phys. Rev. Lett. 74 (1995), 846 [gr-qc/9406010].Google Scholar
[12] H., Martel, P. R., Shapiro and S., Weinberg. Likely values of the cosmological constant. Astrophys. J. 492 (1998), 29 [astro-ph/9701099].Google Scholar
[13] J., Garriga and A., Vilenkin. On likely values of the cosmological constant. Phys. Rev. D 61 (2000), 083502 [astro-ph/9908115].Google Scholar

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