Dynamical Resolution of the Hubble Tension via Generalized Chaplygin Gas Phase Transitions and Elastomeric Brane Topologies

Key Points

• This research aims to address the Hubble Tension by proposing a dynamic model that replaces the cosmological constant with a unified dark fluid.
• Developed a self-consistent framework integrating phase transitions with elastomeric brane topology.
• Examined the implications of dynamic dark fluid on cosmological models and Hubble measurements.
• Demonstrated a potential resolution of the Hubble Tension by achieving an intermediate value between early and late universe measurements.
• Indicated that the dynamic model provides a more coherent understanding of cosmic expansion dynamics.