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Probing Helical Primordial Magnetic Fields via Chiral Gravitational Waves in the LISA-TAIJI Network
Primordial magnetic fields (PMFs) are anticipated to be a cosmological candidate for generating a stochastic gravitational wave background (SGWB) through their anisotropic stress. In particular, if parity violation is present in the production of PMFs, it can induce a helical component in the PMFs,
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