{ "id": "0704.2002", "version": "v1", "published": "2007-04-16T12:37:39.000Z", "updated": "2007-04-16T12:37:39.000Z", "title": "Fluctuation dynamo and turbulent induction at low magnetic Prandtl numbers", "authors": [ "A. A. Schekochihin", "A. B. Iskakov", "S. C. Cowley", "J. C. McWilliams", "M. R. E. Proctor", "T. A. Yousef" ], "comment": "IoP latex, 27 pages, 25 figures, 3 tables. Accepted by New J. Physics", "journal": "New J. Phys. 9, 300 (2007)", "doi": "10.1088/1367-2630/9/8/300", "categories": [ "physics.flu-dyn", "astro-ph", "nlin.CD", "physics.plasm-ph" ], "abstract": "This paper is a detailed report on a programme of simulations used to settle a long-standing issue in the dynamo theory and demonstrate that the fluctuation dynamo exists in the limit of large magnetic Reynolds number Rm>>1 and small magnetic Prandtl number Pm<<1. The dependence of the critical Rm_c vs. the hydrodynamic Reynolds number Re is obtained for 11. The stability curve Rm_c(Re) (and, it is argued, the nature of the dynamo) is substantially different from the case of the simulations and liquid-metal experiments with a mean flow. It is not as yet possible to determine numerically whether the growth rate is ~Rm^{1/2} in the limit Re>>Rm>>1, as should be the case if the dynamo is driven by the inertial-range motions. The magnetic-energy spectrum in the low-Pm regime is qualitatively different from the Pm>1 case and appears to develop a negative spectral slope, although current resolutions are insufficient to determine its asymptotic form. At 1