Primordial Magnetic Field Effects on the CMB and Large Scale Structure
Dai G. Yamazaki, Kiyotomo Ichiki, Toshitaka Kajino, Grant J. Mathew

TL;DR
This paper reviews the theoretical modeling and numerical analysis of primordial magnetic fields and their impact on the cosmic microwave background and large-scale structure, providing updated constraints based on observational data.
Contribution
It introduces a high-precision theoretical framework and an improved numerical program for calculating the effects of primordial magnetic fields on cosmological perturbations.
Findings
PMF significantly influences small-scale cosmological structures
Current CMB data constrains PMF amplitude and spectral index
The developed computational framework improves accuracy over previous models
Abstract
Magnetic fields are everywhere in nature and they play an important role in every astronomical environment which involves the formation of plasma and currents. It is natural therefore to suppose that magnetic fields could be present in the turbulent high temperature environment of the big bang. Such a primordial magnetic field (PMF) would be expected to manifest itself in the cosmic microwave background (CMB) temperature and polarization anisotropies, and also in the formation of large- scale structure. In this review we summarize the theoretical framework which we have developed to calculate the PMF power spectrum to high precision. Using this formulation, we summarize calculations of the effects of a PMF which take accurate quantitative account of the time evolution of the cut off scale. We review the constructed numerical program, which is without approximation, and an improvement…
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