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Cosmological dynamics and observational constraints: Conclusions
This paper is available on arxiv under CC 4.0 license.
Authors:
(1) A. Oliveros, Programa de F´ısica, Universidad del Atl´antico;
(2) Mario A. Acero, Programa de F´ısica, Universidad del Atl´antico.
Table of Links
- Abstract and Intro
- The f(Q) gravity: a brief review
- Cosmological dynamics in late-time
- Parameter constraints
- Conclusions
- Acknowledgments and References
5. Conclusions
Until now, a definitive and satisfactory resolution to the enigma of DE remains elusive within the cosmological community. Consequently, cosmologists continue to propose new and often exotic theories in their pursuit of someday attaining a comprehensive explanation for this perplexing problem. Among these proposals, the f(Q) non-metric gravity has recently gained prominence as an alternative framework for elucidating phenomena in both early and late-time cosmology. Remarkably, this theory achieves this without necessitating the inclusion of dark energy, the inflaton field, or dark matter. This innovative approach represents a significant step forward in our quest to understand the fundamental nature of the universe.
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