Superradiance of Gravitational Waves and Relic Photons from Binary Black Holes and Neutron Stars

Abstract

Type Ia supernova explosions and the merging of binary black holes and neutron stars are considered separate sources of pulsing in the Universe. Their transient signals and characteristic parameters are described using the Dicke superradiance model and quantum statistical theory. Estimates are given for the parameters of gravitational waves, the intensity of relic photons, the boson and Higgs fields, and binary black holes and neutron stars before and after merging.