Cosmology;
Magnetic fields;
Early Universe;
Cosmic microwave background;
Gamma rays;
EXTRAGALACTIC BACKGROUND LIGHT;
ENERGY COSMIC-RAYS;
ELECTROWEAK PHASE-TRANSITION;
LARGE-SCALE STRUCTURE;
FARADAY-ROTATION SEARCH;
ACTIVE GALACTIC NUCLEI;
TEV GAMMA-RAYS;
INTERGALACTIC MEDIUM;
AREA TELESCOPE;
FILLING FACTOR;
D O I:
10.1007/s00159-013-0062-7
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We review the possible mechanisms for the generation of cosmological magnetic fields, discuss their evolution in an expanding Universe filled with the cosmic plasma and provide a critical review of the literature on the subject. We put special emphasis on the prospects for observational tests of the proposed cosmological magnetogenesis scenarios using radio and gamma-ray astronomy and ultra-high-energy cosmic rays. We argue that primordial magnetic fields are observationally testable. They lead to magnetic fields in the intergalactic medium with magnetic field strength and correlation length in a well defined range. We also state the unsolved questions in this fascinating open problem of cosmology and propose future observations to address them.