Diamagnetic field states in cosmological plasmas
Asenjo
F
A
author
Mahajan
S
M
author
2019
English
Using a generally covariant electrovortic (magnetofluid) formalism for relativistic plasmas, the dynamical evolution of a generalized vorticity (a combination of the magnetic and kinematic parts) is studied in a cosmological context. We derive macroscopic vorticity and magnetic field structures that can emerge in spatial equilibrium configurations of the relativistic plasma. These fields, however, evolve in time. These magnetic and velocity fields, self-consistently sustained in a plasma with arbitrary thermodynamics, constitute a diamagnetic state in the expanding universe. In particular, we explore a special class of magnetic and velocity field structures supported by a plasma in which the generalized vorticity vanishes. We derive a highly interesting characteristic of such "superconductor-like" fields in a cosmological plasmas in the radiation era in the early universe. In that case, the fields grow proportional to the scale factor, establishing a deep connection between the expanding universe and the primordial magnetic fields.
WOS:000467737500016
exported from refbase (http://ficpubs.uai.cl/show.php?record=999), last updated on Mon, 03 Jun 2019 19:44:39 +0000
text
10.1103/PhysRevE.99.053204
Asenjo+Mahajan2019
Physical Review E
Phys. Rev. E
2019
Amer Physical Soc
continuing
periodical
academic journal
99
5
7 pp
2470-0045