Spontaneous creation of circularly polarized photons in chiral astrophysical systems
arXiv:2002.01593 · doi:10.1103/PhysRevLett.124.211301
Abstract
This work establishes a relation between chiral anomalies in curved spacetimes and the radiative content of the gravitational field. In particular, we show that a flux of circularly polarized gravitational waves triggers the spontaneous creation of photons with net circular polarization from the quantum vacuum. Using waveform catalogues we identify precessing binary black holes as astrophysical configurations that emit such gravitational radiation, and then solve the fully non-linear Einstein's equations with numerical relativity to evaluate the net effect. The quantum amplitude for a merger is comparable to the Hawking emission rate of the final black hole, and small to be directly observed. However, the implications for the inspiral of binary neutron stars could be more prominent, as argued on symmetry grounds.
7 pages, 3 figures
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- Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
- Gravitational leptogenesis from metric perturbations
- Curvature and dynamical spacetimes: can we peer into the quantum regime?
- Chiral anomalies induced by gravitational waves
- Cosmological mirror symmetry and gravitational-wave helicity