Magnetic Knots as The origin of Spikes in the Gravitational Waves Backgrounds
Massimo Giovannini (University of Cambridge, DAMTP)

TL;DR
This paper explores how magnetic knot configurations in the early universe's plasma can generate distinctive spikes in the gravitational wave spectrum, potentially detectable within specific frequency ranges.
Contribution
It introduces explicit magnetic knot configurations and calculates their impact on gravitational wave spectra, revealing a novel source of gravitational wave spikes from primordial magnetic structures.
Findings
Magnetic knots can produce spikes in the gravitational wave spectrum.
The spectrum shows power suppression at low frequencies and exponential suppression at high frequencies.
The amplitude of these spikes can exceed standard inflationary gravitational wave backgrounds.
Abstract
The dynamical symmetries of hot and electrically neutral plasmas in a highly conducting medium suggest that, after the epoch of the electron-positron annihilation, magnetohydrodynamical configurations carrying a net magnetic helicity can be present. The simultaneous conservation of the magnetic flux and helicity implies that the (divergence free) field lines will possess inhomogeneous knot structures acting as source seeds in the evolution equations of the scalar, vector and tensor fluctuations of the background geometry. We give explicit examples of magnetic knot configurations with finite energy and we compute the induced metric fluctuations. Since magnetic knots are (conformally) coupled to gravity via the vertex dictated by the equivalence principle, they can imprint spikes in the gravitational wave spectrum for frequencies compatible with the typical scale of the knot…
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