Revisiting the dynamics of interacting vector-like dark energy
Carlos Rodriguez-Benites, Manuel Gonzalez-Espinoza, Giovanni Otalora, and Manuel Alva-Morales

TL;DR
This paper revisits the dynamics of interacting vector-like dark energy, analyzing how its interaction with dark matter affects cosmic expansion, equation of state, and energy density, with implications for cosmological models and observations.
Contribution
It introduces a revised analysis of vector-like dark energy interactions, emphasizing their impact on universe evolution and observational signatures.
Findings
Interaction significantly alters dark energy evolution
Distinct features in equation of state due to interaction
Comparison with observational data supports interaction effects
Abstract
We revise the dynamics of interacting vector-like dark energy, a theoretical framework proposed to explain the accelerated expansion of the universe. By investigating the interaction between vector-like dark energy and dark matter, we analyze its effects on the cosmic expansion history and the thermodynamics of the accelerating universe. Our results demonstrate that the presence of interaction significantly influences the evolution of vector-like dark energy, leading to distinct features in its equation of state and energy density. We compare our findings with observational data and highlight the importance of considering interactions in future cosmological studies.
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Dark Matter and Cosmic Phenomena
