Angular Correlation of the CMB in the R_h=ct Universe

@inproceedings{Melia2012AngularCO,
  title={Angular Correlation of the CMB in the R\_h=ct Universe},
  author={Fulvio Melia},
  year={2012}
}
Context. The emergence of several unexpected large-scale features i n the cosmic microwave background (CMB) has pointed to possible new physics driving the origin of density fluctuati ons in the early Universe and their evolution into the largescale structure we see today. Aims. In this paper, we focus our attention on the possible absence of angular correlation in the CMB anisotropies at angles lar ger than∼ 60◦, and consider whether this feature may be the signature of flu ctuations expected… Expand

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