Low Mach and Peclet number limit for a model of stellar tachocline and upper radiative zones

Low Mach and Peclet number limit for a model of stellar tachocline and upper radiative zones

We study a hydrodynamical model describing the motion of internal stellar layers based on compressible Navier-Stokes-Fourier-Poisson system. We suppose that the medium is electrically charged, we include energy exchanges through radiative transfer and we assume that the system is rotating. We an...

Full description

Bibliographic Details
Main Authors: Donatella Donatelli, Bernard Ducomet, Marek Kobera, Sarka Necasova
Format: Article
Language:English
Published: Texas State University 2016-09-01
Series:Electronic Journal of Differential Equations
Subjects:
Navier-Stokes-Fourier-Poisson system
radiation transfer
compressible magnetohydrodynamics
rotation
stellar radiative zone
weak solution
elliptic-parabolic initial boundary value problem
vanishing Peclet number
vanishing Mach number
vanishing Alfven number
classical physics
plasma
Online Access:http://ejde.math.txstate.edu/Volumes/2016/245/abstr.html

Internet

http://ejde.math.txstate.edu/Volumes/2016/245/abstr.html

Similar Items