Inhomogeneous M-Theory Cosmologies

Abstract

We study a class of inhomogeneous and anisotropic $G_2$ string cosmological models. In the case of separable $G_2$ models we show that the governing equations reduce to a system of ordinary differential equations. We focus on a class of separable $G_2$ M-theory cosmological models, and study their qualitative behaviour (a class of models with time-reversed dynamics is also possible). We find that generically these inhomogeneous M-theory cosmologies evolve from a spatially inhomogeneous and negatively curved model with a non-trivial form field towards spatially flat and spatially homogeneous dilaton-moduli-vacuum solutions with trivial form--fields. The late time behaviour is the same as that of spatially homogeneous models previously studied. However, the inhomogeneities are not dynamically insignificant at early times in these models.

18 pages, 0 figures, REVTEX, AMSfonts; To appear in Jour. Math. Phys

References in corpus (4)

• Dynamics of M-Theory Cosmology
• Qualitative Analysis of String Cosmologies
• Qualitative Analysis of Early Universe Cosmologies
• Qualitative Analysis of Isotropic Curvature String Cosmologies

Cited by in corpus (1)

• Phase Space Analysis of Quintessence Cosmologies with a Double Exponential Potential