Chiral gravitational waves from multi-phase magnetogenesis
H. V. Ragavendra, Gianmassimo Tasinato, and L. Sriramkumar

TL;DR
This paper proposes a novel inflationary mechanism with parity-violating interactions that amplifies primordial magnetic fields and produces chiral gravitational waves, offering potential observational signatures for future gravitational-wave detectors.
Contribution
It introduces a non-slow-roll inflationary framework with parity violation that enhances magnetic fields and predicts detectable chiral gravitational-wave signals.
Findings
Chiral magnetic fields can be significantly amplified during brief non-slow-roll phases.
Distinct polarization-dependent spectral features are imprinted in the magnetic fields.
Chiral gravitational-wave backgrounds with characteristic frequency profiles are predicted.
Abstract
Cosmological vector fields are central to many early-Universe phenomena, including inflationary dynamics, primordial magnetogenesis, and dark-matter scenarios. However, constructing models able to generate cosmological magnetic fields while avoiding strong coupling, backreaction, and cosmic microwave background constraints remains challenging. We study a novel mechanism in which brief non--slow-roll phases during inflation amplify primordial magnetic fields at small scales, while maintaining theoretical consistency and observational viability. We incorporate parity-violating interactions in the vector sector and demonstrate, for the first time in a non--slow-roll framework, that chirality can significantly boost magnetic-field amplitudes and imprint distinctive polarization-dependent spectral features. We complement detailed numerical computations with an analytical treatment yielding…
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