Probing Helical Primordial Magnetic Fields via Chiral Gravitational Waves in the LISA-TAIJI Network
astro-ph.CO, gr-qc
Submitted: 2026-09-30
Updated: 2026-09-30
Terminology
Sources
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Cosmological Backgrounds of Gravitational Waves
- Cosmological Magnetic Fields: Their Generation, Evolution and Observation
- The origin, evolution and signatures of primordial magnetic fields
- The intergalactic magnetic field constrained by Fermi/LAT observations of the TeV blazar 1ES 0229+200
- Evidence for strong extragalactic magnetic fields from Fermi observations of TeV blazars
- Limits on primordial magnetic fields from direct detection experiments of gravitational wave background
- Adding helicity to inflationary magnetogenesis
- Scale-invariant Helical Magnetic Fields from Inflation
- The generation of helical magnetic field in a viable scenario of Inflationary Magnetogenesis
- Search for CP Violating Signature of Intergalactic Magnetic Helicity in the Gamma Ray Sky
- Chiral Gravitational Waves Produced in a Helical Magnetogenesis Model
- Gravitational wave generation in a viable scenario of inflationary magnetogenesis
- Simulations of helical inflationary magnetogenesis and gravitational waves
- The LISA-Taiji network
- Alternative LISA-TAIJI networks
- Circularly Polarized Gravitational Wave Background Search with a Network of Space-borne Triangular Detectors
- Alternative LISA-TAIJI networks: Detectability of the Parity Violation in Stochastic Gravitational Wave Background
- Massive Neutrinos and Magnetic Fields in the Early Universe
- Planck 2015 results. XIX. Constraints on primordial magnetic fields
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