Power-Law Bounces in Gravity: Analysis of the Ekpyrosis and Accelerating Regimes
arXiv:2507.00242 · doi:10.1103/rrnm-z3qy
Abstract
We investigate the dynamics of the Friedmann-Lemaître-Robertson-Walker spacetime within the framework of gravity using a compact, model-independent dynamical systems approach. By assuming a power-law scale factor, we explore ekpyrotic and accelerating solutions to address the big bang singularity. Our analysis demonstrates that a cosmological bounce, characterized by a transition from contraction to expansion, possibly avoids the singularity without directly using the Raychaudhuri equation, unlike previous approaches using specific forms. We identify a key fixed point in the phase space corresponding to the bounce, supported by perturbation analysis and qualitative description of trajectories in the phase space. The results suggest that gravity provides a robust framework for non-singular cosmologies.
arXiv commentv3: Corrected minor typos and removed an unused table from the appendix
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