Kavli Affiliate: Stephan Meyer | Summary:Anisotropy of space-time is measured on the scale of the cosmic horizon, using the angular correlation function $C(Θ)$ of cosmic microwave background (CMB) temperature at large angular separation $Θ$. Even-parity correlation $C_rm even(Θ)$ is introduced to obtain a direct, precise measure of horizon-scale curvature anisotropy independent of the unknown dipole, […]
Continue.. Dipole-independent measurements of nearly-zero CMB correlation: a possible symmetry of primordial causal quantum coherence