作者: TR Seshadri , Kandaswamy Subramanian , None
DOI: 10.1103/PHYSREVLETT.87.101301
关键词: Cosmic microwave background 、 Scattering 、 Redshift 、 Anisotropy 、 Background radiation 、 Polarization (waves) 、 Astrophysics 、 Magnetic field 、 Physics 、 Scalar (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