In this work we will shown how can obtain some of Cosmic Microwave Background Radiation (CMBR) parameters if we adopt the models of entanglement with different Universe epochs as sources of a magnetic field (MF) from stress-energy Einstein tensor as been infused by flux lines (bit threads) of fluxoids type, that being born at by Electroweak symmetry breaking (EWPT), projected just to the CMBR horizon.

Also, it is demonstrated that the scaled MF at the CMBR time, keeps the B-curl pattern of the same values as obtained in BICEP2, therefore, these images are not wrong.

We argue that the most promising way to test the hypothesis of CMBR as a projected entanglement hologram is to look for possible imprints of magnetic fields on the temperature and polarization anisotropies of the cosmic microwave background radiation (CMBR).