Inhomogeneous Cosmology, Inflation and Late-Time Accelerating Universe

Abstract

An exact inhomogeneous solution of Einstein's field equations is shown to be able to inflate in a non-uniform way in the early universe and explain anomalies in the WMAP power spectrum data. It is also possible for the model to explain the accelerated expansion of the universe by late-time inhomogeneous structure.

10 pages, Latex file, no figures. Major revision of paper

References in corpus (2)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis

Cited by in corpus (1)

• Redshift Drift in LTB Void Universes