Cosmological Magnetic Fields vs. CMB
arXiv:astro-ph/0405184 · doi:10.1016/j.newar.2005.01.006
Abstract
I present a short review of the effects of a cosmological magnetic field on the CMB temperature and polarization anisotropies. Various possibilities for constraining the magnetic field amplitude are discussed.
6 pages, to appear in proc. of Dark Matter 2004
References in corpus (4)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Origin of Galactic and Extragalactic Magnetic Fields
- The Cosmic Microwave Background and Helical Magnetic Fields: the tensor mode
- Small-scale CMB polarization anisotropies due to tangled primordial magnetic fields
Cited by in corpus (5)
- POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields
- Semi-analytical approach to magnetized temperature autocorrelations
- Statistical Properties of Scale-Invariant Helical Magnetic Fields and Applications to Cosmology
- Evolution of the cosmic matter density field with a primordial magnetic field
- Contrasting formulations of cosmological perturbations in a magnetic FLRW cosmology