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Book Boris V. Vasiliev Astrophysics

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Astrophysics

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where ˜ λ C =<br />

<br />

m ec<br />

is the Compton radius.<br />

At introducing of the new variable<br />

we can transform the Laplacian:<br />

ϕ(r) = χ(r)<br />

r , (10.15)<br />

∆ϕ(r) = 1 r<br />

d 2 χ(r)<br />

dr 2 . (10.16)<br />

As (Eq.(10.12))<br />

χ(r) = 3 m ec 2<br />

Yβr , (10.17)<br />

8 e<br />

the differential equation can be rewritten:<br />

where<br />

L =<br />

d 2 χ(r)<br />

dr 2<br />

= χ(r)<br />

L 2 , (10.18)<br />

( ) 1/2 9π Yβ<br />

˜ λ<br />

32 αξ 3 C , (10.19)<br />

α = 1 is the fine structure constant.<br />

137<br />

With taking in to account the boundary condition, this differential equation has<br />

the solution:<br />

χ(r) = C · exp<br />

(<br />

− r L<br />

)<br />

. (10.20)<br />

Thus, the equation of equilibrium of the electron gas inside a cell (Eq.(10.10)) obtains<br />

the form:<br />

Ze<br />

r · e−r/L = 3 8 mec2 βY . (10.21)<br />

10.2 The Thomas-Fermi screening<br />

Let us consider the case when an ion is placed at the center of a cell, the external shells<br />

don’t permit the plasma electron to approach to the nucleus on the distances much<br />

smaller than the Bohr radius. The electron moving is non-relativistic in this case. At<br />

that ξ → 0, the kinetic energy of the electron<br />

E kin = 3 8 mec2 ξY → 3 EF , (10.22)<br />

5<br />

and the screening length<br />

√<br />

EF<br />

L → . (10.23)<br />

6πe 2 n e<br />

Thus, we get the Thomas-Fermi screening in the case of the non-relativistic motion of<br />

an electron.<br />

78

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