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Electrostatic Forces: Coulomb's Law and Charged Particles, Exams of Physics

An excerpt from hrw 7e, chapter 21. It discusses the electrostatic forces between charged particles, including coulomb's law and the calculation of forces between charged spheres. The magnitudes and components of forces, as well as the sharing of charges when spheres come into contact.

Typology: Exams

Pre 2010

Uploaded on 08/19/2009

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HRW 7e Chapter 21 Page 1 of 5
Halliday/Resnick/Walker 7e
Chapter 21
1. (a) With a understood to mean the magnitude of acceleration, Newton’s second and third laws
lead to
ma ma m
22 11 2
7
7
63 10 70
90 49 10=⇒=
×
..
..
kg m s
ms kg.
2
2
chch
(b) The magnitude of the (only) force on particle 1 is
Fma k
qq
r
q
== = ×
11 12
2
9
2
2
899 10 00032
...
ch
Inserting the values for m1 and a1 (see part (a)) we obtain |q| = 7.1 × 10–11 C.
3. Eq. 21-1 gives Coulomb’s Law, Fk
qq
r
=12
2, which we solve for the distance:
()
(
)
(
)
922 6 6
12 8.99 10 N m C 26.0 10 C 47.0 10 C
|||| 1.39m.
5.70N
kq q
rF
−−
×⋅ × ×
== =
4. The fact that the spheres are identical allows us to conclude that when two spheres are in
contact, they share equal charge. Therefore, when a charged sphere (q) touches an uncharged one,
they will (fairly quickly) each attain half that charge (q/2). We start with spheres 1 and 2 each
having charge q and experiencing a mutual repulsive force . When the neutral sphere
3 touches sphere 1, sphere 1’s charge decreases to q/2. Then sphere 3 (now carrying charge q/2)
is brought into contact with sphere 2, a total amount of q/2 + q becomes shared equally between
them. Therefore, the charge of sphere 3 is 3q/4 in the final situation. The repulsive force between
spheres 1 and 2 is finally
2
/Fkqr=2
2
22
( / 2)(3 / 4) 3 3 ' 3
0.375.
88 8
qq q F
Fk k F
rr F
=====
7. The force experienced by q3 is
31 32 34
3313234 22
2
0
|||| |||| ||||
1ˆˆˆ
j(cos45isin45j)
4(2)
qq qq qq
FF F F aa
a
πε
⎛⎞
=++= + °+ °+
⎜⎟
⎝⎠
GG G G ˆ
i
(a) Therefore, the x-component of the resultant force on q3 is
pf3
pf4
pf5

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Halliday/Resnick/Walker 7e

Chapter 21

  1. (a) With a understood to mean the magnitude of acceleration, Newton’s second and third laws lead to

m a 2 (^) 2 m a 1 (^) 1 m 2

7 6 3 10 7 0 7 9 0

×

= ×

.. − .

kg m s m s

kg.

2 2

c hc h

(b) The magnitude of the (only) force on particle 1 is

F m a k

q q r

q = 1 1 = 1 22 = ×^9

2

c8 99.^10 h0 0032. 2.

Inserting the values for m 1 and a 1 (see part (a)) we obtain | q | = 7.1 × 10 –11^ C.

  1. Eq. 21-1 gives Coulomb’s Law, F = k q^^1 r^2 q 2 , which we solve for the distance:

| 1 || 2 | (^ 8.99^ 10 N m^9 2 C^2 )^ (^ 26.0^10 6 C^ )^ (^ 47.0^10 6 C) 1.39m.

5.70N

r k q^ q F

× ⋅ × −^ × −

  1. The fact that the spheres are identical allows us to conclude that when two spheres are in contact, they share equal charge. Therefore, when a charged sphere ( q ) touches an uncharged one, they will (fairly quickly) each attain half that charge ( q /2). We start with spheres 1 and 2 each having charge q and experiencing a mutual repulsive force. When the neutral sphere 3 touches sphere 1, sphere 1’s charge decreases to q /2. Then sphere 3 (now carrying charge q /2) is brought into contact with sphere 2, a total amount of q /2 + q becomes shared equally between them. Therefore, the charge of sphere 3 is 3 q /4 in the final situation. The repulsive force between spheres 1 and 2 is finally

F = kq^2 / r^2

2 2 2

F k q^ q^ k q^ F F r r F

  1. The force experienced by q 3 is

3 31 32 34 3 1 3 2 3 4 2 2 2 0

1 | || | (^) ˆj | || | (^) (cos45 iˆ (^) sin 45 j)ˆ | || | (^4) ( 2 )

F F F F q^ q^ q^ q^ q^ q

πε a a a

G G G G ˆ

i

(a) Therefore, the x -component of the resultant force on q 3 is

7 2 3 3 2 4 9 2 2 0

| | | | 2 1.0^101

| | 8.99 10 2 0.17N.

x 4 2 2 (0.050) 2 2 F q^ q q

πε a

⎛ ⎞ × − ⎛ ⎞

= ⎜ + ⎟ = × ⎜ + ⎟=

(b) Similarly, the y -component of the net force on q 3 is

7 2 3 2 9 (^3 2 ) 0

| | | | 2 1.0^101

| | 8.99 10 1 0.046N.

y 4 2 2 (0.050) 2 2 F q^ q q

πε a

× −

= ⎛^ − + ⎞^ = × ⎛^ − + ⎞= −

  1. (a) The individual force magnitudes (acting on Q ) are, by Eq. 21-1,

k

q Q a

k

q Q a (^) a a

1 2

2

2 2

b^ − −^ g =^ b − g^2

which leads to | q 1 | = 9.0 | q 2 |. Since Q is located between q 1 and q 2 , we conclude q 1 and q 2 are like-sign. Consequently, q 1 / q 2 = 9.0.

(b) Now we have

k

q Q a

k

q Q a (^) a a

1 32 2

2

b − − g =^ b −^32 g^2

which yields | q 1 | = 25 | q 2 |. Now, Q is not located between q 1 and q 2 , one of them must push and the other must pull. Thus, they are unlike-sign, so q 1 / q 2 = –25.

  1. With rightwards positive, the net force on q 3 is

3 13 23 1 3 2 22 3 12 23 23

F F F k q q^ k q q. L L L

We note that each term exhibits the proper sign (positive for rightward, negative for leftward) for all possible signs of the charges. For example, the first term (the force exerted on q 3 by q 1 ) is negative if they are unlike charges, indicating that q 3 is being pulled toward q 1 , and it is positive if they are like charges (so q 3 would be repelled from q 1 ). Setting the net force equal to zero L 23 = L 12 and canceling k , q 3 and L 12 leads to

1 2 1 2

q (^) q q q

  1. (a) The magnitude of the force between the (positive) ions is given by

F

q q r

k q r

= b gb g=

2

πε^2

We substitute q 2 = Qq 1 and solve for q 1 using the quadratic formula. The two roots obtained are the values of q 1 and q 2 , since it does not matter which is which. We get and 3.8 × 10

1.2 × 10 −^5 C

–5 (^) C. Thus, the charge on the sphere with the smaller charge is 1.2 × 10 − (^5) C.

  1. The unit Ampere is discussed in §21-4. Using i for current, the charge transferred is

q = it = ( 2.5 ×10 A 4 )( 20 × 10 −^6 s) =0.50 C.

  1. Keeping in mind that an Ampere is a Coulomb per second, and that a minute is 60 seconds, the charge (in absolute value) that passes through the chest is

| q | = ( 0.300 Coulombsecond ) ( 120 seconds ) = 36.0 Coulombs.

This charge consists of a number N of electrons (each of which has an absolute value of charge equal to e ). Thus,

N = |^ q |e = (^) 1.6036.0 C x 10 -19 (^) C = 2.25 × 1020.

  1. If the relative difference between the proton and electron charges (in absolute value) were

q q e

p −^ e = 0 0000010.

then the actual difference would be q (^) pqe = 16. × 10 − 25 C. Amplified by a factor of 29 × 3 × 1022 as indicated in the problem, this amounts to a deviation from perfect neutrality of

∆ q = c 29 × 3 × 10 22 hc1 6. × 10 − 25 Ch = 014. C

in a copper penny. Two such pennies, at r = 1.0 m, would therefore experience a very large force. Eq. 21-1 gives

F k q r

= b∆^ g = ×

2 2

17. 108 N.

  1. (a) A force diagram for one of the balls is shown below. The force of gravity mg^ G^ acts downward, the electrical force of the other ball acts to the left, and the tension in the thread

acts along the thread, at the angle θ to the vertical. The ball is in equilibrium, so its acceleration

is zero. The y component of Newton’s second law yields T cos θ – mg = 0 and the x component

yields T sin θ – F

G

Fe

e = 0. We solve the first equation for^ T^ and obtain^ T^ =^ mg /cos^ θ. We substitute

the result into the second to obtain mg tan θ – Fe = 0.

Examination of the geometry of Figure 21-43 leads to

tan θ =.

x L x

2 b 2 g^2

If L is much larger than x (which is the case if θ is very small), we may neglect x /2 in the

denominator and write tan θ ≈ x /2 L. This is equivalent to approximating tan θ by sin θ. The

magnitude of the electrical force of one ball on the other is

F q e (^) x

2

0

4 πε^2

by Eq. 21-4. When these two expressions are used in the equation mg tan θ = Fe , we obtain

mgx L

q x

x q L 2 mg

2 2

2 0

1 3 ≈ ⇒ ≈

F

HG^

I

πε πε KJ

/ .

(b) We solve x^3 = 2 kq^2 L / mg ) for the charge (using Eq. 21-5):

( )(^ )

3 2 3 8 9 2 2

0.010 kg 9.8 m s 0.050 m 2.4 10 C. (^2) 2 8.99 10 N m C 1.20 m

q mgx kL

= = = ± ×^ −

× ⋅

Thus, the magnitude is | q | = 2.4 × 10 −^8 C.