Electrical conductivity of plasmas of DB white dwarf atmospheres

被引:6
|
作者
Sreckovic, V. A. [1 ]
Ignjatovic, Lj. M. [1 ,2 ]
Mihajlov, A. A. [1 ,2 ]
Dimitrijevic, M. S. [2 ,3 ,4 ]
机构
[1] Inst Phys, Belgrade 11001, Serbia
[2] Isaac Newton Inst Chile, Yugoslavia Branch, Santiago, Chile
[3] Astron Observ, Belgrade 11160 74, Serbia
[4] Observ Paris, F-92195 Meudon, France
关键词
stars: atmospheres; stars: kinematics and dynamics; white dwarfs; CROSS-SECTIONS; HELIUM; HE; SCATTERING; ELECTRONS; COLLISIONS; STARS;
D O I
10.1111/j.1365-2966.2010.16702.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The static electrical conductivity of non-ideal, dense, partially ionized helium plasma was calculated over a wide range of plasma parameters: temperatures 1 x 104 less than or similar to T less than or similar to 1 x 105 K and mass density 1 x 10-6 g cm-3 less than or similar to less than or similar to 2 g cm-3. Calculations of electrical conductivity of plasma for the considered range of plasma parameters are of interest for DB white dwarf atmospheres with effective temperatures 1 x 104 K less than or similar to T-eff less than or similar to 3 x 104 K. Electrical conductivity of plasma was calculated by using the modified random phase approximation and semiclassical method, adapted for the case of dense, partially ionized plasma. The results were compared with the unique existing experimental data, including the results related to the region of dense plasmas. In spite of low accuracy of the experimental data, the existing agreement with them indicates that results obtained in this paper are correct.
引用
收藏
页码:590 / 596
页数:7
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