New appearance of cosmic coincidence problem
Abstract
The integrals of the Friedmann cosmology equations are identified as constant physical characteristics for both vacuum and non-vacuum cosmic energies. The integrals are found to be numerically coincident. A model shows that the coincidence can naturally originate in the electroweak scale physics at TeV temperatures. The coincidence seems to reflect a new type of symmetry that relates vacuum and non-vacuum energies.
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