Revisiting the dynamics of interacting vector-like dark energy

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.

15 pages, 19 figures. Updated to match the published version in EPJC

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Cited by in corpus (8)

• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Cosmological Dynamics in Interacting Scalar-Torsion f(T,$\varphi$) Gravity: Investigating Energy and Momentum Couplings
• Teleparallel Gravity and Quintessence: The Role of Nonminimal Boundary Couplings
• Screening fifth forces in scalar-vector-tensor theories
• Some Classes of Interacting Two-Fluid Model of the Expanding Universe
• Power-law Bianchi type I inflation with multiple vector fields