刊物主题:Physics Mathematical and Computational Physics Relativity and Cosmology Differential Geometry Quantum Physics Astronomy, Astrophysics and Cosmology
出版者:Springer Netherlands
ISSN:1572-9532
文摘
We examine the effect on cosmological evolution of adding a Gauss–Bonnet term to the standard Einstein–Hilbert action for a (1 + 3) + d dimensional Friedman–Robertson–Walker (FRW) metric. By assuming that the additional dimensions compactify as a power law as the usual 3 spatial dimensions expand, we solve the resulting dynamical equations and find that the solution may be of either de Sitter or Kasner form depending upon whether the Gauss–Bonnet term or the Einstein term dominates.