Abstract
The paper considers the issue of the anomalously low temperature dispersion of the cosmic microwave background (CMB) of the Universe, which was discovered by researchers R. Penrose and V. Gurzadyan according to the data of the WMAP and Planck missions. A new explanation of this phenomenon is given as evidence of residual traces in the CMB after the occurrence of multiple instabilities in the vacuum phase of matter in the first moments of the development of our Universe. It is these instabilities that have become the centers of the emergence of the fundamental mass of matter – massive photon pairs (ultralight scalar bosons). Theoretical and experimental evidence of the connection of CMB with massive photon pairs is presented using data from the Interball-Tail Probe, RHESSI and XMM-Newton missions.
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