Physical properties of compact star-like systems harboring traversable wormholes: Effects of chaotic magnetic fields and anisotropic matter
This research investigates neutron-star–wormhole systems using two scalar fields to see how chaotic magnetic fields and matter anisotropy affect their properties. The study finds that these complex factors can create extremely massive configurations exceeding 8 solar masses and surface redshifts above 1.5, showing a dependence of the gravitational-wave echo time on the magnetic field strength.