Testing the cosmological evolution of magnetic fields in galaxies with the SKA

Авторы: Arshakian T.G., Beck R., Krause M., Sokoloff D.
Сборник: IAU Symposium
Серия: IAU Symposium
Том: 259
Год издания: 2009
Место издания: Springer
Первая страница: 667
Последняя страница: 668
DOI: 10.1017/S1743921309031512
Аннотация: We investigate the cosmological evolution of large- and small-scale magnetic fields in galaxies at high redshifts. Results from simulations of hierarchical structure formation cosmology provide a tool to develop an evolutionary model of regular magnetic fields coupled to galaxy formation and evolution. Turbulence in protogalactic halos generated by thermal virialization can drive an efficient turbulent dynamo. The mean-field dynamo theory is used to derive the timescales of amplification and ordering of regular magnetic fields in disk and dwarf galaxies. For future observations with the SKA, we predict an anticorrelation at fixed redshift between galaxy size and the ratio between ordering scale and galaxy size. Undisturbed dwarf galaxies should host fully coherent fields at z < 1, spiral galaxies at z < 0.5.
Добавил в систему: Соколов Дмитрий Дмитриевич

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