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VbvAstE-001

Book Boris V. Vasiliev Astrophysics

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Astrophysics

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infinity. 1 With this in mind, we can write the energy balance equation of electron<br />

E kin = eϕ(r). (10.5)<br />

The potential energy of an electron at its moving in an electric field of the nucleus<br />

can be evaluated on the basis of the Lorentz transformation [14]§24. If in the laboratory<br />

frame of reference, where an electric charge placed, it creates an electric potential ϕ 0,<br />

the potential in the frame of reference moving with velocity v is<br />

ϕ =<br />

ϕ 0<br />

√<br />

1 − v2<br />

c 2 . (10.6)<br />

Therefore, the potential energy of the electron in the field of the nucleus can be written<br />

as:<br />

E pot = − Ze2 ξ<br />

r β . (10.7)<br />

Where<br />

β = v c . (10.8)<br />

and<br />

ξ ≡<br />

p<br />

m , ec (10.9)<br />

m e is the mass of electron in the rest.<br />

And one can rewrite the energy balance Eq.(10.5) as follows:<br />

where<br />

Y =<br />

3<br />

8 mec2 ξY = eϕ(r) ξ β . (10.10)<br />

[<br />

ξ(2ξ 2 + 1) √ ]<br />

ξ 2 + 1 − Arcsinh(ξ) − 8 3 ξ3<br />

. (10.11)<br />

ξ 4<br />

Hence<br />

ϕ(r) = 3 m ec 2<br />

βY. (10.12)<br />

8 e<br />

In according with Poisson’s electrostatic equation<br />

∆ϕ(r) = 4πen e (10.13)<br />

or at taking into account that the electron density is depending on momentum<br />

(Eq.(10.2)), we obtain<br />

∆ϕ(r) = 4e ( ) 3 ξ<br />

, (10.14)<br />

3π ˜λ C<br />

1 In general, if there is an uncompensated electric charge inside the cell, then we would<br />

have to include it to the potential ϕ(r). However, we can do not it, because will consider only<br />

electro-neutral cell, in which the charge of the nucleus exactly offset by the electronic charge,<br />

so the electric field on the cell border is equal to zero.<br />

77

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