Gravitomagnetic relativistic effects on turbulence
arXiv:2005.10871 · doi:10.1142/S0129183121501291
Abstract
The dynamics of fluid-matter under the influence of gravitomagnetic fields are formulated and solved for the case of fully developed turbulence. Gravitomagnetic effects reduce the vortical complexity and nonlinearity of turbulence, even leading to its extinction within large volumes, and generate departures from Kolmogorov turbulence scalings, that are explained via a combination of dimensional and exact analysis arguments.
17 pages, 5 figures
References in corpus (5)
- Planck evidence for a closed Universe and a possible crisis for cosmology
- Turbulence and Magnetic Fields in the Large Scale Structure of the Universe
- General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers
- General relativistic viscous hydrodynamics of differentially rotating neutron stars
- Magnetic structures produced by the small-scale dynamo