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

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    0462799 - MÚ 2017 RIV US eng J - Journal Article
    Donatelli, D. - Ducomet, B. - Kobera, M. - Nečasová, Šárka
    Low Mach and Peclet number limit for a model of stellar tachocline and upper radiative zones.
    Electronic Journal of Differential Equations. Roč. 2016, Č. 245 (2016), s. 1-31. ISSN 1072-6691
    R&D Projects: GA ČR GA16-03230S
    Institutional support: RVO:67985840
    Keywords : Navier-Stokes-Fourier-Poisson system * radiation transfer * compressible magnetohydrodynamics
    Subject RIV: BA - General Mathematics
    Impact factor: 0.954, year: 2016
    Result website:
    http://ejde.math.txstate.edu/Volumes/2016/245/abstr.html

    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 analyze the singular limit of this system when the Mach number, the Alfven number, the Peclet number and the Froude number approache zero in a certain way and prove convergence to a 3D incompressible MHD system with a stationary linear transport equation for transport of radiation intensity. Finally, we show that the energy equation reduces to a steady equation for the temperature corrector.

    Permanent Link: http://hdl.handle.net/11104/0262186

     
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