Magnetized CMB anisotropies
arXiv:astro-ph/0508544 · doi:10.1088/0264-9381/23/2/R01
Abstract
Possible effects of large-scale magnetic fields on the Cosmic Microwave Background (CMB) are reviewed. Depending on the specific branch of the spectrum of plasma excitations, magnetic fields are treated either within a two-fluid plasma description or within an effective (one-fluid) approach. The uniform field approximation is contrasted with the fully inhomogeneous field approximation. It is argued that the interplay between CMB physics and large-scale magnetic fields will represent a rather interesting cross-disciplinary arena along the next few years.
61 pages, 5 figures, references added, to appear as Topical Review in Classical and Quantum Gravity
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- The Impact of Stochastic Primordial Magnetic Fields on the Scalar Contribution to Cosmic Microwave Background Anisotropies
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- Entropy perturbations and large-scale magnetic fields
- Numerical simulations of the decay of primordial magnetic turbulence
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- Phase Transition Generated Cosmological Magnetic Field at Large Scales
- Cosmological magnetic fields from nonlinear effects
- Constraints on primordial magnetic fields from magnetically-induced perturbations: current status and future perspectives with LiteBIRD and future ground based experiments
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- Symmetry restoration at finite temperature with weak magnetic fields
- Constraining primordial magnetic fields with CMB polarization experiments
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- Statistical anisotropy from inflationary magnetogenesis
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- Primordial vorticity and gradient expansion
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- Seminal Electromagnetic fields from preinflation
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