100% satisfaction guarantee Immediately available after payment Both online and in PDF No strings attached 4,6 TrustPilot
logo-home
Exam (elaborations)

SOLUTIONS MANUAL for Plasma Physics An Introduction 2nd Edition by Fitzpatrick Richard.

Rating
-
Sold
-
Pages
101
Grade
A+
Uploaded on
08-01-2024
Written in
2024/2025

SOLUTIONS MANUAL for Plasma Physics An Introduction 2nd Edition by Fitzpatrick Richard.

Institution
Plasma Physics An Introduction
Course
Plasma Physics An Introduction











Whoops! We can’t load your doc right now. Try again or contact support.

Written for

Institution
Plasma Physics An Introduction
Course
Plasma Physics An Introduction

Document information

Uploaded on
January 8, 2024
Number of pages
101
Written in
2024/2025
Type
Exam (elaborations)
Contains
Questions & answers

Subjects

Content preview

, CHAPTER 1

Chapter 1



1.1 (a) Consider a one-dimensional slab of plasma whose whose bounding surfaces are nor-
mal to the x-axis. Suppose that the electrons (whose mass, charge, and number density
are me, −e, and ne, respectively) displace a distance δxe parallel to the x-axis, whereas
the ions (whose mass, charge, and number density are mi, +Z e, and ni = ne/Z, re-
spectively) displace a distance δxi. The resulting charge density that develops on the
leading edge of the slab is
σ = −e ne δxe + Z e ni δxi = e ne (δxi − δxe). (1)

An equal and opposite charge density develops on the opposite face of the slab. The
x-directed electric field generated inside the slab is
σ e ne
E =− =− (δx − δx ). (2)
x i e
ǫ0 ǫ0
The equation of motion of an individual electron inside the slab is thus

.. e2 ne
me δ xe = −e Ex = (δxi − δxe). (3)
ǫ0
Likewise, the equation of motion of an individual ion is

.. Z 2 e2 n i
mi δ xi = Z e Ex = − (δxi − δxe). (4)
ǫ0
Let us search for simultaneous solutions of Equations (3) and (4) of the form

δxe(t) = δxˆe cos(ω t), (5)
δxi(t) = δxˆi cos(ω t). (6)

It follows that

(ω2 − Π e2) δxˆe + ω p2 e δxˆi = 0, (7)
Πi2 δxˆe + (ω2 − ω p2 i) δxˆi = 0, (8)
where Πe = (e2 ne/ǫ0 me)1/2 and Πi = (Z 2 e2 ni/ǫ0 mi)1/2. The solutions are ω = 0
with δxˆe = δxˆi, and ω2 = Π 2 + Π 2 with Π 2 δxˆe + Π 2 δxˆi = 0. The former mode
e i i e
corresponds to a uniform translation of the slab. The latter mode is a plasma oscillation
whose frequency, Π, satisfies
1/2
Π = Πe2 + Πi2 , (9)

1

,2 □ Plasma Physics: An Introduction (Second Edition): Solutions to Exercises

and whose characteristic ratio of ion to electron displacement amplitudes is
δxˆi Π i2 me
δxˆ = − = −Z i . (10)
e Π e2 m
(b) Suppose that the electrons, whose temperature is Te, are distributed according to the
Maxwell-Boltzmann law,

ne + δne = ne exp(+e δΦ/Te), (11)

where ne is the equilibrium number density, and δne is the number density perturbation
due to the perturbing potential δΦ. Likewise, the ions, whose temperature is Ti, are
distributed according to

ni + δni = ni exp(−Z e δΦ/Ti). (12)

Thus, in the limit that δΦ is small, we obtain
e ne
δne = δΦ, (13)
Te
Z e ni
δni = − δΦ. (14)
Ti
If δΦ is a consequence of a small perturbing charge density, δρext, then the total charge
density is
2 2
!
e2 ne Z e ni
δρ = δρext + Z e δni − e δne = δρext − + . (15)
Te Ti
Thus, Poisson’s equation,
2 δρ
∇ δΦ = − , (16)
ǫ0
yields 2
2 δρext
∇ – δΦ = − , (17)
λ 2D ǫ 0

where !2 !2 !2
1 1 1 1
= + , (18)
λD 2 λD e λD i
with λD e = (ǫ0 Te/ne e2)1/2 and λD i = (ǫ0 Ti/ni Z 2 e2)1/2. Comparison of Equation (17)
with Eq. (1.14) in the book reveals that λD is the effective Debye length.
1.2 It is reasonable to assume, by symmetry, that the perturbed potential is a function only of the
radial spherical coordinate r. In other words, δΦ = δΦ(r). Thus, the governing differential
equation becomes !
1 d 2 dδΦ 2
2 r – 2 δΦ = 0 (19)
r dr dr λD
for r ≠ 0. However, in the limit r → 0 we expect the perturbed potential to approach the
Coulomb potential: i.e.,
q
δΦ → (20)
4π ǫ0 r

, Chapter 1 □ 3

as r → 0. We also expect the potential to be well behaved in the limit r → ∞ . Let δΦ =
V(r)/r. Equation (19) transforms to give
d2V 2
− V = 0. (21)
dr2 λD2
The solution that is consistent with the boundary conditions at r = 0 and r = ∞ is
√2 r
V(r) = q . (22)
4π ǫ0 exp − λD
Thus, √
δΦ(r) = q 2r . (23)
4π ǫ0 r exp − λD

According to Poisson’s equation, the charge density of the shielding cloud is

δρ(r) = −ǫ0 ∇2δΦ. (24)

However, according to the governing differential equation,
2 2
∇ δΦ = δΦ (25)
λD2
for r ≠ 0. Hence, √
2q 2r
δρ(r) = − exp − . (26)
4π r λD2 λD
The net shielding charge contained within a sphere of radius r, centered on the origin, is
∫ r ∫ √ ′
′ ′2 ′ 2q r ′ 2r ′
Q(r) = 4π δρ(r ) r dr = − r exp − dr . (27)
0 λD 0 λD
2

Thus, √ √
∫ √

x.λD r/ 2
λD r/ 2 λD r/ 2
Q(r) = −q x e−x dx = −q −x e− 0 + e− dx , (28)
0 0 x
.
which reduces to √2 r √ 2r
Q(r) = −q 1 − 1 + exp − . (29)
λD λD
1.3 Consider a one-dimensional slab of plasma whose bounding surfaces are normal to the x-
axis. Suppose that the electrons (whose mass, charge, and number density are me, −e, and
ne, respectively) displace a distance δxe parallel to the x-axis, whereas the ions remain sta-
tionary. The resulting charge density that develops on the leading edge of the slab is

σ = −e ne δxe. (30)

An equal and opposite charge density develops on the opposite face of the slab. The x-
directed electric field generated inside the slab is
σ e ne
E =− = δx . (31)
x e
ǫ0 ǫ0

Get to know the seller

Seller avatar
Reputation scores are based on the amount of documents a seller has sold for a fee and the reviews they have received for those documents. There are three levels: Bronze, Silver and Gold. The better the reputation, the more your can rely on the quality of the sellers work.
Succeed Havard University
View profile
Follow You need to be logged in order to follow users or courses
Sold
1796
Member since
5 year
Number of followers
1499
Documents
5757
Last sold
6 hours ago

3.9

286 reviews

5
162
4
34
3
34
2
9
1
47

Recently viewed by you

Why students choose Stuvia

Created by fellow students, verified by reviews

Quality you can trust: written by students who passed their exams and reviewed by others who've used these notes.

Didn't get what you expected? Choose another document

No worries! You can immediately select a different document that better matches what you need.

Pay how you prefer, start learning right away

No subscription, no commitments. Pay the way you're used to via credit card or EFT and download your PDF document instantly.

Student with book image

“Bought, downloaded, and aced it. It really can be that simple.”

Alisha Student

Frequently asked questions