Chemical In Homogeneities, Electric Currents, and Diffusion Waves in Stars

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SFRMXU8T

Chemical In Homogeneities, Electric Currents, and Diffusion Waves in Stars

Vadim Urpin
Vadim Urpin A.F.Ioffe Institute of Physics and Technology,
DOI

Abstract

The stars of the middle main sequence often have spot-like chemical structures at their surfaces. We consider diffusion caused by electric currents and argue that such current-driven diffusion can form chemical in homogeneities in plasma. Diffusion was considered using partial momentum equations derived by the Chapman-Enskog method. We argue that diffusion caused by electric currents can substantially change the surface chemistry of stars and form spotted chemical structures even in a relatively weak magnetic field. The considered mechanism can be responsible for a formation of element spots in Hg-Mn and Ap-stars. Diffusion in the presence of electric currents can be accompanied by propagation of a particular type of magneto hydrodynamic modes in which only the impurity number density oscillate. Such modes exist if the magnetic pressure is much greater than the gas pressure and can be the reason of variations of the abundance peculiarities in stars.

Chemical In Homogeneities, Electric Currents, and Diffusion Waves in Stars

The stars of the middle main sequence often have spot-like chemical structures at their surfaces. We consider diffusion caused by electric currents and argue that such current-driven diffusion can form chemical in homogeneities in plasma. Diffusion was considered using partial momentum equations derived by the Chapman-Enskog method. We argue that diffusion caused by electric currents can substantially change the surface chemistry of stars and form spotted chemical structures even in a relatively weak magnetic field. The considered mechanism can be responsible for a formation of element spots in Hg-Mn and Ap-stars. Diffusion in the presence of electric currents can be accompanied by propagation of a particular type of magneto hydrodynamic modes in which only the impurity number density oscillate. Such modes exist if the magnetic pressure is much greater than the gas pressure and can be the reason of variations of the abundance peculiarities in stars.

Vadim Urpin
Vadim Urpin A.F.Ioffe Institute of Physics and Technology,

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Vadim Urpin. 2018. “. Global Journal of Science Frontier Research – A: Physics & Space Science GJSFR-A Volume 18 (GJSFR Volume 18 Issue A1): .

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Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

Issue Cover
GJSFR Volume 18 Issue A1
Pg. 47- 53
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GJSFR-A Classification: FOR Code: 020105
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Chemical In Homogeneities, Electric Currents, and Diffusion Waves in Stars

Vadim Urpin
Vadim Urpin A.F.Ioffe Institute of Physics and Technology,

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