Hydrodynamic time correlation functions in the presence of a gravitational field
Astrophysics
2009-11-07 v2 Statistical Mechanics
Abstract
This paper shows that the ordinary Brillouin spectrum peaks associated to scattered radiation off acoustic modes in a fluid suffer a shift in their values due to gravitational effects. The approach is based in the ordinary linearized Navier-Stokes equations for a fluid coupled to a Newtonian gravitational potential. The formalism leads to a dispersion relation that contains both gravitational and dissipative effects. It is also shown that the Brillouin peaks tend to condense into a single peak when the fluid modes approach the critical Jeans wave number.
Keywords
Cite
@article{arxiv.astro-ph/0301501,
title = {Hydrodynamic time correlation functions in the presence of a gravitational field},
author = {A. Sandoval-Villalbazo and L. S. Garcia-Colin},
journal= {arXiv preprint arXiv:astro-ph/0301501},
year = {2009}
}
Comments
6 pages, no figures. To appear in Physica A