John. A.
The tests are closed book and will cover the material from Jones and Childers and the lectures. If you have a question about a test or the date of a test, you can email me at jshaw@lsmsa.edu .
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· Sample test solutions below:
· 1. a) a = -g sin q - mu_k g cos q = -9.8 sin (40) -0.45 9.8 cos(40) = -9.68 m/s^2
· b) v^2=vo^2 + 2 a d, and v=0 at top so d = -vo^2/(2a) = +3^2/(2*9.68)=0.465 meters
· c) if mu_k=0, then a = -gsinq so d=3^2/(2*6.3)= 0.71 meters
· 2. a) tanq=T_1/T_2, so find T_1 and T_2 first. T_1 =m_a g =20*9.8=196N,
· T_2 = mu_s m_b g =0.25*50*9.8=122.5N, q=32 degrees.
· b) T_3 = m_a g /cosq = 231 N
· c) T_1=196, and T_2 = 123 N from above
· 3. a) T^2 = 4pi^2/(GM) r^3, so M=4pi^2/(GT^2) r^3 = 4(3.14159)^2/(6.67x10^-11*16^2*86400^2) (1.22x10^9)^3 = 5.6x10^26 kg.
· b) T = 2 pi /(G M)^0.5 r^1.5 = 1.65x10^5 seconds = 1.9 days
· 4. a) diagram will give mu_s g = v^2/r, for v maximum
· b) v=(mu_s g r )^0.5 = (0.32*32 ft/s^2 68 ft)^0.5 = 27.6 ft/s
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· Sample Test solutions below:
· 1.a) -127 Joules, friction opposite displacement
· b) +254 Joules, gravity has component along displacement
· c) +118 Joules
· d) 6.9 m/s
· 2. a) v1f=0.7 m/s, v2f=2.2 m/s, both positive
· b) pf-pi=-3.6 kgm/s for m1, +3.6 for m2, equal and opposite
· c) -3600 N for m1, +3600 N for m2, equal and opposite (N3L!)
· 3. a) vf/v1=0.4 or v1/vf=2.5 if inverted
· b) vf=1.62 m/s after collision
· c) v1=4.05 m/s before collision
· 4. a) 10.3 km/s
· b) 11.2 km/s
· Solutions to last year's final (large non-text file, ca. 200kB)
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Final Exam Solutions (from ’02, sorry, you still have to take the ’03 version!):
I. Short answer section
1.E=7200 V/m
2. V=0 halfway between equal and opposite charges
3. E=V/d = 90,000 V/m
4. Q=CV = 7.97x10^-8 C
5. Ctotal = 6.67 pF or 6.67x10^-12 F
6. Rtotal=13.2 Ohms
7. i = 0.45 Amps through 10 Ohm resistor. At node i splits into 0.36 Amps through the 4 Ohm and 0.09 Amps through the 16 Ohm resistors respectively. Note the sum is 0.45 as it must be.
8. r =1.6 cm or 1.6x10^-2 meters
9. B=6.28x10^-5 Tesla
10. Tau = RC = 5x10^-7 seconds
11. Lambda’ = Lambda/n so n=5/4=1.25 (dimensionless ratio)
12. n = 1.59 (dimensionless ratio).
13. theta_2 = 14.9 degrees from the normal
14. i = 12 cm
15. M = +2/3, upright and smaller
16. angular separation = 6.6x10^-3 radians
II. Longer responses:
1. a) Read book for a detailed discussion of Gauss’ law. You need a closed surface surrounding the charge. The surface should be perpendicular to the electric field lines so the normal and the electric field are parallel. This is easy for a point charge if you surround the charge by a sphere with radius r. E is a constant so summing over the surface just gives E (A) = q/e_o since q is inside the sphere. A = 4pi r^2 for a sphere so solving for E gives Coulomb’s law.
b) Gauss just says that the flux of the field through a closed surface is proportional the amount of charge inside the surface. No charge inside, no flux. Charge inside, then positive or negative flux depending on the sign of the net charge enclosed.
2. a) 6-i_2 10 – 3 – i_1 10 = 0 and 3 +i_2 10 – i_3 20 – i_3 30 = 0
b) i_1 – i_2 –i_3 =0 at A ( i_1 flows in from left and i_2 and i_3 go down and to right respectively).
c) haven’t worked this out, but you can do it on a calculator TI-84 or higher…
3. a) read book for detailed discussion of Ampere’s Law. You need a closed curve going around the wire. The curve should be parallel to the magnetic field so B and the tangent to the curve are parallel. This is easy for a wire if you surround the wire by a circle. B has a constant magnitude on the curve so summing B dS around the curve just gives B (L) = mu_o i since i in the wire is enclosed by the curve. L = 2 pi r for a circle so solving for B gives B = mu_o i/(2 pi r).
b) The magnetic field is proportional to the enclosed current. No current enclosed, no B. The sum of B dS around the curve (technically the line integral of B along the curve C) doesn’t have a neat name like “flux.”
4. See book for details on ray tracing.
a) If o > f but o< 2f then the image is enlarged, inverted, and real. The rays intersect to form an image on the far side of the lens: e.g. o=1.5f gives i =+3 f so M =-3/(3/2) = -2 => real, enlarged, and inverted as in ray trace..
b) If o =f then there is no image formed. The rays are parallel: e.g. o=f gives 1/i = 0 so i is infinitely large => no intersection, no image. Ray trace should give almost exactly parallel lines.
c) If o < f then the image is enlarged, upright, and virtual. The rays intersect to form an image on the same side of the lens as the object: e. g. o = 0.5f gives i= -f so M = +2 => virtual, enlarged, and upright as in ray trace.
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