Cosmic Microwave Background Polarization Signals from Tangled Magnetic Fields

作者: TR Seshadri , Kandaswamy Subramanian , None

DOI: 10.1103/PHYSREVLETT.87.101301

关键词: Cosmic microwave backgroundScatteringRedshiftAnisotropyBackground radiationPolarization (waves)AstrophysicsMagnetic fieldPhysicsScalar (mathematics)

摘要: Tangled, primordial cosmic magnetic fields create small rotational velocity perturbations on the last scattering surface of microwave background radiation. For which redshift to a present value B{sub 0}=3 x 10{sup -9} G , these vector modes are shown generate polarization anisotropies order 0.1--4 {mu}K angular scales (500

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