ISSN 1063-7850, Technical Physics Letters, 2015, Vol. 41, No. 1, pp. 43–45. © Pleiades Publishing, Ltd., 2015.
Original Russian Text © K.D. Kapustin, M.B. Krasil’nikov, A.A. Kudryavtsev, 2015, published in Pis’ma v Zhurnal Tekhnicheskoi Fiziki, 2015, Vol. 41, No. 1, pp. 87–93.
43
The electron distribution function (EDF) in
plasma is usually determined with the use of the local
approximation when in solving the kinetic equation
the terms with spatial variables are excluded and the
EDF is factorized in the form of the product of the
electron density, which depend on spatial coordinates
and time, and the EDF itself, which depends on the
electron kinetic energy
(1)
In this approximation, the electron distribution by
kinetic energy w at space point r depends on local val-
ues of the reduced field E/p and other parameters (gas
temperature, concentration of excited particles, etc.).
The local distribution attracts researchers and is
widely used mainly due to the considerably simplified
computational procedure in solving the Boltzmann
kinetic equation, which depends, in this case, on only
one variable, kinetic energy w.
The local approximation applicability criteria are
obtained by a standard technique with regard to small-
ness of the terms with coordinate derivatives as com-
pared with the terms with energy derivatives in the
kinetic equation for electrons. This yields the estima-
tion in the form of the condition
(2)
i.e., characteristic diffusion length L of the plasma vol-
ume should exceed electron energy relaxation
length λ
ε
(see, e.g., [1, 2]). In expression (2), D
r
=
Vλ/3 is the diffusivity of free electrons and the corre-
sponding energy relaxation time
(3)
is determined by energy loss upon elastic and inelastic
collisions (corresponding frequencies ν and ν*).
Since at the elastic scattering the energy relaxation
occurs at many collisions (the corresponding energy
exchange factor is δ = < 10
–4
), in the elastic
energy range ε < ε
1
, where ε
1
is the first threshold of
inelastic processes, the length
(4)
is significant and exceeds the free electron path by
more than two orders of magnitude. For atomic gases,
conditions (2) and (4) require relatively large values of
the parameter pL > 5–10 cm Torr, where p is the gas
pressure.
It should be noted that when the local approxima-
tion is used, the condition L > λ
ε
is implicitly assumed
to be also the condition for negligibility of ambipolar
field E
amb
as compared with current field E
heat
that
heats electrons. Indeed, the simple estimations
(5)
show that the inequality L λ
ε
is followed by the con-
dition E
heat
E
amb
.
It can be seen from (5) that, in reality, the ambipo-
lar field is small at the central plasma parts, where the
plasma concentration is maximum, and grows toward
the periphery, where it exceeds the longitudinal (heat)
field. Since electrons react to the resulting electric
fwrt ,, ( ) n
e
rt , ( ) f
0
wE / p , ( ) . =
L λ
ε
2 D
r
τ
ε
, =
τ
ε
1 –
δν ν * + =
2 m/ M
λ
s
D
r
/ δλ ( ) λ / δ 100 λ > ≅ ≅
E
heat
T
e
/ λ
ε
, E
amb
≅ T
e
∇n
e
/ n
e
– T
e
/ L ≅ =
The Role of the Ambipolar Field
and the Local Approximation Inapplicability in Determination
of the Electron Distribution Function at High Pressures
K. D. Kapustin
b
, M. B. Krasil’nikov
a
, and A. A. Kudryavtsev
a
*
a
St. Petersburg State University, St. Petersburg, 199034 Russia
b
St. Petersburg State University of Information Technologies, Mechanics, and Optics,
St. Petersburg, 197101 Russia
*e-mail: akud@ak2138.spb.edu
Received September 12, 2014
Abstract—It is demonstrated that the condition for applicability of the local approximation in solving the
kinetic equation for electrons includes not only smallness of the electron kinetic relaxation length as com-
pared with the characteristic plasma volume, but also smallness of the ambipolar filed as compared with the
current (heating) field. Therefore, at the discharge periphery, where the ambipolar field exceeds the longitu-
dinal one, the local approximation cannot be used for calculating the electron distribution function even at
high gas pressures.
DOI: 10.1134/S1063785015010071