Observational Constraints and Future of the Universe with Dynamic Dark Energy

Florian Neukart

doi:10.20944/preprints202401.0137.v1

Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Version 1 : Received: 1 January 2024 / Approved: 3 January 2024 / Online: 3 January 2024 (04:20:40 CET)

This paper is dedicated to examining dynamic dark energy models in the context of observational constraints and their implications for the universe's future. By integrating theoretical models with various observational data, we aim to provide a comprehensive view of how dynamic dark energy influences cosmic evolution and the universe's fate. This study tests these models against the latest observational evidence, including the Cosmic Microwave Background, supernovae, and large-scale structure surveys, to refine our understanding of the universe's accelerating expansion and the mysterious nature of dark energy.

Hubble tension; Cosmic Microwave Background; Large-scale structures; Dark energy constraints; Future cosmological observations

Physical Sciences, Astronomy and Astrophysics

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Observational Constraints and Future of the Universe with Dynamic Dark Energy

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