Cosmic Microwave Background Anomalies Explained by the Modified Einstein Field Interaction (MEFI) Theory

This paper explores how the Modified Einstein Field Interaction (MEFI) theory provides insights into anomalies observed in the Cosmic Microwave Background (CMB). By introducing the concept of the dark field, we simulate its effects on CMB anisotropies and investigate how spacetime compression influences temperature fluctuations and polarization patterns. A series of simulations are presented to demonstrate how the MEFI theory may offer new explanations for the observed large-scale anomalies in the CMB. Python code for each simulation is provided alongside results that showcase the impact of the dark field on early-universe phenomena.<br><br>