Time delay in the ultrahigh-energy signal from Cygnus X-3
Arbuzov B. A. , Razuvaev E. A.
The time delay in the signal from the source Cygnus X-3, detected from extensive air showers with £>3 X 10'4 eV and reckoned from the maximum of the radio burst from this source in October 1985, can be explained by an interpretation offered previously for the emission at ultrahigh energies from this source, as consisting of free gluons. This interpretation is shown to be consistent with the set of experimental data. The interaction energy of background-radiation gluons may be an important component of the density of the hidden mass in the universe.