M-theory moduli space and cosmology

R. Brustein, S. P. de Alwis, and E. G. Novak
Phys. Rev. D 68, 043507 – Published 12 August 2003
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Abstract

We conduct a systematic search for a viable string or M-theory cosmology, focusing on cosmologies that include an era of slow-roll inflation, after which the moduli are stabilized and the Universe is in a state with an acceptably small cosmological constant. We observe that the duality relations between different cosmological backgrounds of string or M-theory moduli space are greatly simplified, and that this simplification leads to a truncated moduli space within which possible cosmological solutions lie. We review some known challenges to four dimensional models in the “outer,” perturbative, region of moduli space, and use duality relations to extend them to models of all of the (compactified) perturbative string theories and 11D supergravity, including brane world models. We conclude that cosmologies restricted to the outer region are not viable, and that the most likely region of moduli space in which to find realistic cosmology is the “central,” nonperturbative region, with coupling and compact volume both of order unity, in string units.

  • Received 31 December 2002

DOI:https://doi.org/10.1103/PhysRevD.68.043507

©2003 American Physical Society

Authors & Affiliations

R. Brustein*

  • Department of Physics, Ben-Gurion University, Beer-Sheva 84105, Israel

S. P. de Alwis

  • Department of Physics, Box 390, University of Colorado, Boulder, Colorado 80309, USA

E. G. Novak

  • Department of Physics, Ben-Gurion University, Beer-Sheva 84105, Israel

  • *Email address: ramyb@bgumail.bgu.ac.il
  • Email address: dealwis@pizero.colorado.edu
  • Email address: enovak@bgumail.bgu.ac.il

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Issue

Vol. 68, Iss. 4 — 15 August 2003

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