Abstract
The stability properties of the Einstein Static solution of General Relativity is altered when corrective terms arising from modifications of the underlying gravitational theory appear in the cosmological equations. Employing dynamical system techniques and numerical integrations, we discuss the stability of static cosmological solutions in the framework of two recently proposed quantum gravity models, namely Loop Quantum Cosmology and Horava-Lifshitz gravity.
Information
Published: 1 January 2011
First available in Project Euclid: 13 July 2015
zbMATH: 1382.83033
MathSciNet: MR2850376
Digital Object Identifier: 10.7546/giq-12-2011-290-304
Rights: Copyright © 2011 Institute of Biophysics and Biomedical Engineering, Bulgarian Academy of Sciences
