Preventing Curvature Singularities in Dark Energy Models
arXiv:2508.20430 · doi:10.1142/S0217751X25501544
Abstract
The curvature singularity problem in dark energy models poses a significant challenge to their viability as alternatives to the CDM paradigm. In this work, we investigate the possibility of resolving this issue by incorporating higher-order corrections that are compatible with the inflationary phase. We analyze the effects of adding , and -attractor representation in gravity terms to types of dark energy models, focusing on their ability to prevent singularities in high-density environments. Our results demonstrate that these corrections can effectively stabilize the models, ensuring their consistency across both inflationary and late-time cosmological scales.
arXiv comment25 pages, 8 figures
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