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x
x 1
x 2
q < 0
xq
F1q F2q
Solution:
Part (a): Since Q 1 > 0 and q < 0, the force (F 1 q) between Q 1 > 0 and q < 0 points to the left (as shown in the figure above) due to the fact that these charges will attract each other. Since Q 2 > 0 and q < 0, the force (F 2 q) between Q 2 > 0 and q < 0 points to the right, once again due to the fact that these charges will attract each other. As stated in the problem, the sum of these two forces is +5. 56 × 10 −^4 N (Ftot). Using this fact in conjunction with Coulomb’s Law, we can do a little algebra to solve for q:
Ftot = F 2 q − F 1 q
= ke
|Q 2 | |q| r^22 q
− ke
|Q 1 | |q| r^21 q
= ke |q|
[ |Q 2 | r 22 q
r^21 q
] ,
|q| = Ftot ke
[ |Q 2 | r^22 q
r 12 q
]− 1 .
r 1 q = xq − x 1 = 2.89 m − (− 4 .56 m) = 7.45 m r 2 q = (x 2 − xq) = 8.05 m − 2 .89 m = 5.16 m |Q 1 | r^21 q
(7.45 m)^2
55 .5025 m^2
= 1. 24 × 10 −^6 C/m^2.
|Q 2 | r^22 q
(5.16 m)^2
26 .6256 m^2
= 8. 75 × 10 −^6 C/m^2.
|q| =
[
]− 1
Since q has to be negative as stated in the problem, q = − 8. 24 × 10 −^9 C.
Part (b): Here we just use Newton’s Second Law of Motion: F = m a, and solve for a the acceleration (remembering to change the mass from cgs units to SI units):
a =
Ftot m
= 0 .727 m/s^2.
x 0 x o xf
E = 6.68 x 10^6 N/C
q = +e mp v
Solution:
Part (a): The figure to the right diagrams the problem, where our particle (a proton), has mass mp = 1. 672 × 10 −^27 kg, charge q = +e = 1. 602 × 10 −^19 C, and travels along the x-axis from x◦ = -4.56 m (where it starts from rest) to xf = 7.58 m for a total distance of d = xf − x◦ = 7.58 m - (-4.56 m) = 12.14 m. This proton travels in an electric field E of strength 6. 68 × 106 N/C which runs parallel to the x axis. The change in potential energy can now be determined with:
∆PE = −q E d = −(1. 602 × 10 −^19 C) (6. 68 × 106 N/C) (12.14 m) = − 1. 30 × 10 −^11 J ,
where the negative sign results from the fact that q > 0 (i.e., a positive value).
Part (b): To determine the final velocity, the simplest way is to just use the conservation of energy. Here, we do not need to include the gravitational potential energy since the mass just moves in the horizontal direction, hence PEg i = PEg f. Since we are starting from rest, the initial kinetic energy is equal to 0.
KE (^) i + PE (^) i = KE (^) f + PE (^) f PE (^) i − PE (^) f = KE (^) f − KE (^) i −∆PE =
m vf^2 − 0
v^2 f =
mp
vf =
√ −2(− 1. 30 × 10 −^11 J)
vf = 1. 25 × 108 m/s.
Q 1 Q 2
Q 3
P
r 12
r 13 r 23
x
Solution: y
First we need to calculate the distances that point P is from each charge. We will define r 1 as the distance from Q 1 to P, r 2 as the distance from Q 2 to P, and r 3 as the distance from Q 3 to P — note that r 3 is perpendicular to r 12 :
r 1 = 12 r 12 = 12 (1.34 m) = 0.670 m r 2 = 12 r 12 = 12 (1.34 m) = 0.670 m
r 3 =
√ r^223 − r^22 = 1.16 m
Now we use the superposition principle (Eq. II-8) to calculate the total potential at point P:
V = ke
∑^3 i=
( (^) q i ri
)
= ke
( Q 1 r 1
r 2
r 3
)
(
0 .670 m
0 .670 m
1 .16 m
]
(
) [ − 6. 04 × 10 −^6 C/m
]
Solution:
Part (a): Since there are no other components in this circuit, the potential across the plates of the capacitor is the same as the potential delivered by the battery: ∆V = 1.50 V. We now need to convert the energy of this capacitor from eVs to SI units:
U = 6. 89 × 106 eV · 1. 602 × 10 −^19 J/eV = 1. 10 × 10 −^12 J.
To calculate the area, we first must convert the radius from cgs to SI units, r = 1.34 cm =
A = π r^2 = π (1. 34 × 10 −^2 m)^2 = 5. 64 × 10 −^4 m^2.
Part (b): We determine the capacitance using the capacitor energy equation (Eq. II-28):
U =
= 9. 81 × 10 −^13 F = 0.981 pF.
Part (c): For the separation use Eq. (II-14):
C = ◦
d
d = ◦
(
) (^5). 64 × 10 − (^4) m 2
Part (d): We can now use either Eq. (II-12) or Eq. (II-28) to calculate the full charge, here we will use Eq. (II-12) first, then Eq. (II-28):