Gravitational Waves from Primordial Magnetic Fields via Photon-Graviton Conversion
arXiv:2002.07548 · doi:10.1103/PhysRevD.102.103501
Abstract
We explore a novel process in the early Universe in which thermalized photons are converted into gravitons in the presence of strong primordial magnetic fields. It is found that the frequency of generated gravitational waves (GWs) is typically of order of GHz and their amplitude can be up to . If detected with future developments of the technology to explore this frequency region, the produced stochastic GW background enables us to know when and how strong the primordial magnetic fields are generated. From the peak frequency of the GWs, we can also probe the number of relativistic degrees of freedom at that time.
9 pages, 1 figure, updated to match the published version
References in corpus (13)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Science with the space-based interferometer LISA. IV: Probing inflation with gravitational waves
- Lower limit on the strength and filling factor of extragalactic magnetic fields
- N-flationary magnetic fields
- Consistent generation of magnetic fields in axion inflation models
- Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton-photon mixing
- Baryogenesis from Decaying Magnetic Helicity
- Search for a stochastic background of 100-MHz gravitational waves with laser interferometers
- Evolution of the Baryon Asymmetry through the Electroweak Crossover in the Presence of a Helical Magnetic Field
- The turbulent chiral-magnetic cascade in the early universe
- Conversion of relic gravitational waves into photons in cosmological magnetic fields
- Updated constraint on a primordial magnetic field during big bang nucleosynthesis and a formulation of field effects
- Baryon asymmetry from hypermagnetic helicity in dilaton hypercharge electromagnetism
Cited by in corpus (21)
- A novel search for high-frequency gravitational waves with low-mass axion haloscopes
- Potential of radio telescopes as high-frequency gravitational wave detectors
- Rare Events Detected with a Bulk Acoustic Wave High Frequency Gravitational Wave Antenna
- Graviton detection and the quantization of gravity
- Gravitational wave search through electromagnetic telescopes
- Discovery prospects with the Dark-photons & Axion-Like particles Interferometer
- Strongly Magnetized Hot QCD Matter and Stochastic Gravitational Wave Background
- Gravitational waves in neutrino plasma and NANOGrav signal
- Universal Hz stochastic gravitational waves from photon spheres of black holes
- Gravitational wave modes in matter
- Conversion of electromagnetic and gravitational waves by a charged black hole
- Scattering and conversion of electromagnetic and gravitational waves by Reissner-Nordström black holes: The Regge pole description
- Dark Energy with a Triplet of Classical U(1) Fields
- Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
- Graviton-photon conversion in stochastic magnetic fields
- An Upper Limit on the Initial Temperature of the Radiation-Dominated Universe
- Gravitational waves in minimal Maxwell gravity
- Self-consistent interaction of linear gravitational and electromagnetic waves in non-magnetized plasma
- Photons generated by gravitional waves in the near-zone of a neutron star
- An array of bulk-acoustic-wave sensors as a high-frequency antenna for gravitational waves
- Probing leptogenesis and the minimal neutrino seesaw mechanism through gravitational waves