The accelerating universe as a research area investigates the observed late-time acceleration of cosmic expansion and its implications for fundamental physics and cosmology. It encompasses precise measurements of distance–redshift relations using Type Ia supernovae, baryon acoustic oscillations, and weak gravitational lensing, as well as constraints from cosmic microwave background anisotropies and large-scale structure growth. The field focuses on characterizing dark energy (e.g., cosmological constant, dynamical scalar fields, or modified gravity), determining its equation-of-state parameter and possible evolution, testing general relativity on cosmological scales, and developing theoretical frameworks and numerical simulations to reconcile observational data with models of cosmic expansion history.
Science never stops. Get notified about trending stories.
