Bremsstrahlung of Light through Spontaneous Emission of Gravitational Waves

TL;DR

This paper proposes a theoretical effect where photons bending around massive objects emit gravitational waves, potentially detectable by future space-based observatories like LISA, linking quantum vacuum fluctuations to observable astrophysical phenomena.

Contribution

It introduces a novel theoretical effect of photon-induced gravitational wave emission during gravitational bending, connecting quantum vacuum fluctuations with classical and quantum gravity phenomena.

Findings

Gravitational bending of light can be accompanied by gravitational wave emission.

The effect may cause a redshift in light similar to bremsstrahlung.

Potential observability with the LISA gravitational wave detector.

Abstract

Zero-point fluctuations are a universal consequence of quantum theory. Vacuum fluctuations of electromagnetic field have provided crucial evidence and guidance for QED as a successful quantum field theory with a defining gauge symmetry through the Lamb shift, Casimir effect, and spontaneous emission. In an accelerated frame, the thermalisation of the zero-point electromagnetic field gives rise to the Unruh effect linked to the Hawking effect of a black hole via the equivalence principle. This principle is the basis of general covariance, the symmetry of general relativity as the classical theory of gravity. If quantum gravity exists, the quantum vacuum fluctuations of the gravitational field should also lead to the quantum decoherence and dissertation of general forms of energy and matter. Here we present a novel theoretical effect involving the spontaneous emission of soft gravitons by photons as they bend around a heavy mass and discuss its observational prospects. Our analytic and numerical investigations suggest that the gravitational bending of starlight predicted by classical general relativity should also be accompanied by the emission of gravitational waves. This in turn redshifts the light causing a loss of its energy somewhat analogous to the bremsstrahlung of electrons by a heavier charged particle. It is suggested that this new effect may be important for a combined astronomical source of intense gravity and high-frequency radiation such as X-ray binaries and that the proposed LISA mission may be potentially sensitive to the resulting sub-Hz stochastic gravitational waves.