EVOLUTION OF THE MAGNETIC FIELD IN SPATIALLY INHOMOGENEOUS AXION STRUCTURES

被引:1
|
作者
Dvornikov, M. S. [1 ]
Akhmet'ev, P. M. [1 ]
机构
[1] Russian Acad Sci, Pushkov Inst Terr Magnetism Ionosphere & Radio Wav, Troitsk, Moscow, Russia
关键词
axion star; dark matter; asymptotic ergodic Hopf invariant; magnetic hydrodynamics; INVARIANT; HELICITY;
D O I
10.1134/S0040577924030103
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We study the time evolution of magnetic fields in various configurations of spatially inhomogeneous pseudoscalar fields that are a coherent superposition of axions. For such systems, we derive a new induction equation for the magnetic field, which takes this inhomogeneity into account. Based on this equation, we study the evolution of a pair of Chern-Simons waves interacting with a linearly decreasing pseudoscalar field. The nonzero gradient of the pseudoscalar field leads to the mixing of these waves. We then consider the problem in a compact domain in the case where the initial Chern-Simons wave is mirror symmetric. The pseudoscalar field inhomogeneity then leads to an effective change in the a dynamo parameter. Thus, the influence of a spatially inhomogeneous pseudoscalar field on the magnetic field evolution bears a strong dependence on the system geometry.
引用
收藏
页码:515 / 529
页数:15
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