Relic gravitational waves from the chiral magnetic effect
Axel Brandenburg, Yutong He, Tina Kahniashvili, Matthias Rheinhardt,, Jennifer Schober

TL;DR
This paper investigates how relic gravitational waves are generated by primordial magnetic fields via the chiral magnetic effect, analyzing how different generation speeds influence GW amplitudes and spectra in early universe conditions.
Contribution
It introduces a generic model for magnetic field generation through the CME and explores its impact on GW production, revealing two distinct regimes with different spectral behaviors.
Findings
GW energy scales with the third power of magnetic energy in regime I
GW energy increases without magnetic energy growth in regime II
GW spectrum exhibits opposite slopes in the two regimes
Abstract
Relic gravitational waves (GWs) can be produced by primordial magnetic fields. However, not much is known about the resulting GW amplitudes and their dependence on the details of the generation mechanism. Here we treat magnetic field generation through the chiral magnetic effect (CME) as a generic mechanism and explore its dependence on the speed of generation (the product of magnetic diffusivity and characteristic wavenumber) and the speed characterizing the maximum magnetic field strength expected from the CME. When the latter exceeds the former (regime I), the regime applicable to the early universe, we obtain an inverse cascade with moderate GW energy that scales with the third power of the magnetic energy. When the generation speed exceeds the CME limit (regime II), the GW energy continues to increase without a corresponding increase of magnetic energy. In the early kinematic…
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