Influence of the turbulent motion on the chiral magnetic effect in the early universe
We study the magnetohydrodynamics of relativistic plasmas accounting for the chiral magnetic effect (CME). To take into account the evolution of the plasma velocity, obeying the Navier-Stokes equation, we approximate it by the Lorentz force accompanied by the phenomenological drag time parameter. On...
Published in: | Physical Review D Vol. 95, № 4. P. 043538-1-043538-10 |
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Format: | Article |
Language: | English |
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Online Access: | http://vital.lib.tsu.ru/vital/access/manager/Repository/vtls:000615948 Перейти в каталог НБ ТГУ |