





Study with the several resources on Docsity
Earn points by helping other students or get them with a premium plan
Prepare for your exams
Study with the several resources on Docsity
Earn points to download
Earn points by helping other students or get them with a premium plan
Community
Ask the community for help and clear up your study doubts
Discover the best universities in your country according to Docsity users
Free resources
Download our free guides on studying techniques, anxiety management strategies, and thesis advice from Docsity tutors
Material Type: Exam; Professor: Kiley; Class: Introductory Physics II; Subject: Physics; University: University of California-Merced;
Typology: Exams
1 / 9
This page cannot be seen from the preview
Don't miss anything!
Final Solutions
For the midterm, you may use one sheet of notes with whatever you want to put on it, front and back. Please sit every other seat, and please don’t cheat! If something isn’t clear, please ask. You may use calculators. All problems are weighted equally. PLEASE BOX YOUR FINAL ANSWERS! You have the full length of the class. If you attach any additional scratch work, then make sure that your name is on every sheet of your work. Good luck!
(a) What is the index of refraction of the transparent substance? Hint: Note that sin (90◦^ − θ) = cos θ. (b) What is the critical angle for the total internal reflection in this substance?
————————————————————————————————————
Solution
(a) Recall Snell’s law, taking nair = 1, and the index of refraction in the substance n,
sin θ 1 = n sin θ 2.
We’re told that the reflected and refracted rays are mutually perpendicular, such that θ 1 +θ 2 = 90◦. So, solving for θ 2 = 90◦^ −θ 1 , such that sin θ 2 = sin (90◦^ − θ 1 ) = cos θ 1 , then we have
n =
sin θ 1 cos θ 1
= tan θ 1 = tan (58◦) = 1. 6.
(b) The condition for total internal reflection is, again taking nair = 1,
n 2 sin θc = sin (90◦) = 1 ⇒ θc = sin−^1
n 2
In part (a) we found n 2 = 1.6, and so
θc = sin−^1
(a) What is the depth of the submarine? (b) Based on the frequency shift, is the submarine ascending or descending? (c) If the speed of sound in seawater is 1.54 km/s, then what is the vertical speed of the submarine (remember that, since the pulse is reflected, it’s going to be Doppler shifted twice!).
————————————————————————————————————
Solution
(a) The sound pulse takes 80 ms to travel down to the submarine and back up to the destroyer. If the sound travels at speed v, then 2D = v∆t, so
v∆t =
(1540) (0.080) = 62 m.
(b) The reflected frequency is smaller than the original frequency which tells us that the submarine is moving away from the destroyer, and so it is descending. (c) The destroyer sends out the f 0 = 40 MHz pulse, which is Doppler shifted once as it is traveling towards the submarine. If the sound travels at speed v, then the submarine receives the pulse with a frequency
fSub =
v − vsub v
f 0.
Now, the submarine reflects this same frequency back to the destroyer, but it is Doppler shifted again, since the submarine is still descending. So, the frequency received by the destroyer is
fdestroyer =
v v + vsub
fsub =
v − vsub v + vsub
f 0.
So we just have to now solve for vsub. Doing so gives
vsub =
f 0 − fdestroyer f 0 + fdestroyer
v =
× 1540 = 0.81 m/s.
Solution
From Gauss’s law, the electric field from a line charge is E = (^2) π^10 λr. The force per unit length on the other line charge at a distance d is F/L = (^2) π^10 λ
2 d. From Ampere’s law, the magnetic field from a current-carrying wire is B = μ 2 π^0 Ir. The force per unit length on the other wire at a distance d is F/L = μ 20 πI
2 d. When these forces balance, we have
1 2 π 0
λ^2 d
μ 0 2 π
d
λ^2 = μ 0 I^2.
But, I = λv, and so (^) ^10 λ^2 = μ 0 λ^2 v^2 , or
v =
μ 0 0
Plugging in the values gives v ≈ 2. 99 × 108 m/s = c, which is the speed of light! So, the wires would need to be moving at the speed of light for the forces to exactly balance out! So, this means that the two wires will always repel each other electrically.
Solution
If the dust has a velocity v and makes a circular orbit of radius r, then it takes a time
2 πr v to do so. Now, the magnetic force makes it go in a circle and so, since the orbit is perpendicular to the field,
qvB =
mv^2 r
r v
m qB
where q is the charge. Plugging this back into the time equation gives
2 πm qB
Plugging in the numbers gives
2 πm qB
2 π × 10 × 10 −^6
= 2. 1 × 1011 seconds,
which is about 6,640 years! Notice that the velocity and radius of the dust doesn’t make any difference.
The following is worth 15 extra credit points!
The figure to the right shows the actual produc- tion of the antimatter partner to the electron, the positron, in a bubble chamber immersed in a uniform magnetic field. The positron has ex- actly the same mass as an electron, but opposite charge. The different tracks show the trajecto- ries of the different particles. In the reaction at the top, a high-energy gamma ray (just a high- frequency light wave) is absorbed by an electron, which scatters away to the right, producing an electron-positron pair though the reaction
γ + e−^ → e−^ + e+^ + e−,
where γ is the incident gamma ray. A similar ef- fect occurs in the bottom reaction, but the original electron very likely had little final velocity. Let’s see what we can tell about this reaction.
(a) Is charged conserved in this reaction? Explain. (b) Why do the electrons and positrons curve in different directions? (c) In what direction (into or out of the page) is the magnetic field? How can you tell? (d) How does the velocity of the spiraling electron compare to that of the spiraling positron? How can you tell? (e) Accelerating charges radiate energy. Explain why this leads to the spiraling mo- tion for the particles. (f) Positrons and electrons can come together and annihilate, releasing two photons in the process e−^ + e+^ → γ + γ. Explain why we get two photons, and not one. Hint: consider the the two particles initially at rest right next to each other.
————————————————————————————————————
Solution
A more colorful picture is seen to the right, where the positrons are shown in red, and the electrons in green.
(a) Initially we have an electron and a photon. Since the photon isn’t charged, the initial charge is just that on the electron, −e. After the reaction, we’ve produced an electron and positron pair. The net charge of the pair is −e + e = 0, and since we still have an electron the net charge after the reaction is −e, and so charge is conserved.
(b) The electrons and positrons are oppositely charged, and so experience opposite forces in the magnetic field. This leads to motion in different directions. (c) The electron is curving in the counterclockwise direction, while the positron is curving in the clockwise direction. From the magnetic force law, F^ ~ = q~v × B~, for the positively charged positron the velocity is down, and the force is initially to the left, and so the direction of the magnetic field is out of the page.
(d) The faster the speed of the particle, the bigger the radius of the curve. Since the positron has a bigger spiral, it has a bigger speed. (e) As the charges radiate, they lose energy. The only place that they can lose it from is their kinetic energy, and so, they slow down. The slower they move, the smaller the radius of their curvature. So, the curve tightens as they slow down, leading to the spiral. (f) Suppose we had an electron and a positron at rest and just brought them together. In this case the initial momentum is zero, but the photon carries momentum. So, a single photon would violate momentum conservation. Two photons, emitted back-to-back, would conserve momentum. This means we need two photons.