The origin of the magnetic fields of the universe: The plasma astrophysics of the free energy of the universe

被引:52
作者
Colgate, SA
Li, H
Pariev, V
机构
[1] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[2] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[3] PN Lebedev Phys Inst, Moscow 11792, Russia
关键词
D O I
10.1063/1.1351827
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The interpretation of Faraday rotation measure maps of active galactic nuclei (AGNs) within galaxy clusters has revealed ordered or coherent regions, L(mag)similar to 50-100 kpc (similar to 3x10(23) cm), that are populated with large, similar to 30 muG magnetic fields. The magnetic energy of these coherent regions is L-mag(3)(B-2/8 pi)similar to 10(59-60) ergs, and the total magnetic energy over the whole cluster (similar to1 Mpc across) is expected to be even larger. Understanding the origin and role of these magnetic fields is a major challenge to plasma astrophysics. A sequence of physical processes that are responsible for the production, redistribution, and dissipation of these magnetic fields is proposed. These fields are associated with single AGNs within the cluster and therefore with all galaxies during their AGN (active galactic nucleus or quasar) phase, simply because only the central supermassive black holes (similar to 10(8)M) formed during the AGN phase have an accessible energy of formation, similar to 10(61) ergs, that can account for the magnetic field energy budget. An alpha-Omega dynamo process has been proposed that operates in an accretion disk around a black hole. The disk rotation naturally provides a large winding number, similar to 10(11) turns, sufficient to make both large gain and large flux. The helicity of the dynamo can be generated by the differential plume rotation derived from star-disk collisions. This helicity generation process has been demonstrated in the laboratory and the dynamo gain was simulated numerically. A liquid sodium analog of the dynamo is being built. Speculations are that the back reaction of the saturated dynamo will lead to the formation of a force-free magnetic helix, which will carry the energy and flux of the dynamo away from the accretion disk and redistribute the field within the clusters and galaxy walls. The magnetic reconnection of a small fraction of this energy logically is the source of the AGN (active galactic nucleus or quasar) luminosity, and the remainder of the field energy should then dominate the free energy of the present-day universe. The reconnection of this intergalactic field during a Hubble time is the only sufficient source of energy necessary to produce an extragalactic cosmic ray energy spectrum as observed in this galaxy, and at the same time allow this spectrum to escape to the galaxy voids faster than the GZK (blackbody radiation) loss. (C) 2001 American Institute of Physics.
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页码:2425 / 2431
页数:7
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