Editing Dark Energy (section)

=== Overview ===
In modern cosmology, the '''Cosmological Principle''' is a fundamental assumption stating that the universe is homogeneous (uniform in composition) and isotropic (appearing the same in all directions) on large scales. These assumptions simplify the mathematical models used to describe the universe, such as the Friedmann equations and the Lambda-CDM model, which incorporates Dark Energy and Dark Matter. However, what if these assumptions are incorrect? This page explores the potential implications for our understanding of the universe, Dark Energy, and the nature of cosmic structures.