  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.
