Observational constraints on new class dark energy parameterized EoS in Bianchi type-I universe

Puntos clave

• The analysis highlights how dark energy affects the universe's expansion dynamics, particularly in a Bianchi type-I framework.
• Key observations suggest critical constraints on the parameterization of the equation of state for dark energy.
• Observational constraints derived help refine cosmological models, particularly concerning geometric properties in expanding universes.
• The findings emphasize the significance of dark energy parameters in understanding the universe's large-scale structure.