
TL;DR
This paper develops a perturbative formalism to analyze graviton-photon mixing in cosmic magnetic fields, accounting for dispersive effects, and estimates the electromagnetic radiation power generated by such mixing from astrophysical sources.
Contribution
It provides the first perturbative solutions for graviton-photon mixing in an expanding universe, including all known dispersive and coherence-breaking effects.
Findings
Electromagnetic radiation power from GRAPH mixing can reach 10^6 to 10^15 erg/s.
The effect guarantees simultaneous arrival of GWs and EM signals from sources.
The formalism applies to both uniform and non-homogeneous cosmic magnetic fields.
Abstract
In the era of gravitational wave (GW) detection from astrophysical sources by LIGO/VIRGO, it is of great importance to take the quantum gravity effect of graviton-photon (GRAPH) mixing in the cosmic magnetic field to the next level. In this work, we study such an effect and derive for the first time perturbative solutions of the linearized equations of motions of the GRAPH mixing in an expanding universe. In our formalism we take into account all known standard dispersive and coherence breaking effects of photons such as the Faraday effect, the Cotton-Mouton (CM) effect, and the plasma effects in the cosmic magnetic field. Our formalism, applies to a cosmic magnetic field either a uniform or a slowly varying non-homogeneous field of spacetime coordinates with an arbitrary field direction. For binary systems of astrophysical sources of GWs at extragalactic distances with chirp masses…
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