Chiral Gravitational Waves Produced in a Helical Magnetogenesis Model

Abstract

We investigate the gravitational wave production induced by the primordial magnetic fields in a parity-violating magnetogenesis model. It is shown that the gravitational waves detectable by LISA, DECIGO or BBO and the magnetic fields strong enough to explain the blazar observation can be simultaneously produced. The magnetic fields and the gravitational waves have the same chirality and their amplitudes are related, which may also be tested by future observations.

21 pages, 7 figures

References in corpus (20)

• The Chiral Magnetic Effect
• Strong magnetic fields in normal galaxies at high redshifts
• Lower limit on the strength and filling factor of extragalactic magnetic fields
• Magnetic fields from inflation?
• N-flationary magnetic fields
• Probing reheating temperature of the universe with gravitational wave background
• Evolution of Primordial Magnetic Fields from Phase Transitions
• Adding helicity to inflationary magnetogenesis
• Schwinger Effect in 4D de Sitter Space and Constraints on Magnetogenesis in the Early Universe
• Consistent generation of magnetic fields in axion inflation models
• Baryogenesis from Decaying Magnetic Helicity
• Evolution of the Baryon Asymmetry through the Electroweak Crossover in the Presence of a Helical Magnetic Field
• Baryon Asymmetry and Gravitational Waves from Pseudoscalar Inflation
• Universal upper limit on inflation energy scale from cosmic magnetic field
• Chiral Anomaly, Schwinger Effect, Euler-Heisenberg Lagrangian, and application to axion inflation
• Magnetic field spectrum at cosmological recombination revisited
• Primordial magnetic helicity evolution with a homogeneous magnetic field from inflation
• Stealth magnetic field in de Sitter spacetime
• Model-independent constraints in inflationary magnetogenesis
• Synthetic Gravitational Waves from a Rolling Axion Monodromy

Cited by in corpus (21)

• Relic gravitational waves from the chiral magnetic effect
• Analytic study of dark photon and gravitational wave production from axion
• Simulating relic gravitational waves from inflationary magnetogenesis
• Universality of linear perturbations in SU($N$)-natural inflation
• Non-thermally trapped inflation by tachyonic dark photon production
• Circumventing the challenges in the choice of the non-conformal coupling function in inflationary magnetogenesis
• Constraining models of Inflationary Magnetogenesis with NANOGrav
• Measuring the maximally allowed polarization states of the isotropic stochastic gravitational wave background with the ground-based detectors
• Probing Reheating Phase via Non-Helical Magnetogenesis and Secondary Gravitational Waves
• Gauge Field Production and Schwinger Reheating in Runaway Axion Inflation
• Inflation with two-form field: the production of primordial black holes and gravitational waves
• Fate of the first-order chiral phase transition in QCD: Implications for dark QCD studied via a Nambu-Jona-Lasinio model
• First astrometric constraints on parity-violation in the gravitational wave background
• Minimal Magnetogenesis: The Role of Inflationary Perturbations and ALPs, and Its Gravitational Wave Signatures
• Chiral gravitational waves from thermalized neutrinos in the early Universe
• Magnetogenesis from Sawtooth Coupling: Gravitational Wave Probe of Reheating
• Simulations of helical inflationary magnetogenesis and gravitational waves
• Chiral gravitational waves from multi-phase magnetogenesis
• First-order CP phase transition in two-flavor QCD at $\theta =\pi$ under electromagnetic scale anomaly via a Nambu-Jona-Lasinio description
• Twisting inflation to sub-Planckian axion decay constants
• When does the Schwinger Preheating Occur?