Name: Student ID: S13 PHY321: Finalbogner/PHY321/Finalkey2013.pdfS13 PHY321: Final May 1, 2013 NOTE:...

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Name: Student ID: S13 PHY321: Final May 1, 2013 NOTE: Show all your work. No credit for unsupported answers . Turn the front page only when advised by the instructor! The exam consists of 6 problems (60 points) plus one extra credit problem (10 points). Contextual information Damped harmonic oscillator equation: ¨ x +2β ˙ x + ω 2 0 x =0 General solution: x(t)=e βt A 1 exp β 2 ω 2 0 t + A 2 exp β 2 ω 2 0 t Driven harmonic oscillator equation: ¨ x +2β ˙ x + ω 2 0 x = A cos ωt Amplitude of stationary oscillations: D = A (ω 2 0 ω 2 ) 2 +4ω 2 β 2 Phase lag: δ = tan 1 2ωβ ω 2 0 ω 2 Acceleration vector in polar coordinate: a = (¨ r r ˙ θ 2 )e r +(r ¨ θ +2˙ r ˙ θ)e θ G =6.673 × 10 11 m 3 kg s 2 Calculus in spherical coordinates: grad Ψ = e r Ψ r + e θ 1 r Ψ ∂θ + e φ 1 r sin θ Ψ ∂φ div A = 1 r 2 r (r 2 A r )+ 1 r sin θ ∂θ (sin θ A θ )+ 1 r sin θ A φ ∂φ 2 Ψ = 1 r 2 r ( r 2 Ψ r ) + 1 r 2 sin θ ∂θ ( sin θ Ψ ∂θ ) + 1 r 2 sin 2 θ 2 Ψ ∂φ 2 Orbits in a gravitational field: α r =1+ cos θ a = k 2|E| b = 2μ|E| α = 2 μk

Transcript of Name: Student ID: S13 PHY321: Finalbogner/PHY321/Finalkey2013.pdfS13 PHY321: Final May 1, 2013 NOTE:...

Name: Student ID:

S13 PHY321: FinalMay 1, 2013

NOTE: Show all your work. No credit for unsupported answers.

Turn the front page only when advised by the instructor!

The exam consists of 6 problems (60 points) plus one extra creditproblem (10 points).

Contextual information

Damped harmonic oscillator equation: x+ 2βx+ ω20x = 0

General solution: x(t) = e−βt!A1 exp

"#β2 − ω2

0t$+ A2 exp

"−#β2 − ω2

0t$%

Driven harmonic oscillator equation: x+ 2βx+ ω20x = A cosωt

Amplitude of stationary oscillations: D = A!(ω2

0−ω2)2+4ω2β2

Phase lag: δ = tan−1"

2ωβω20−ω2

$

Acceleration vector in polar coordinate: a = (r − rθ2)er + (rθ + 2rθ)eθ

G = 6.673× 10−11 m3

kg s2

Calculus in spherical coordinates:

%gradΨ = %er∂Ψ∂r

+%eθ1r

∂Ψ∂θ

+%eφ1

r sin θ∂Ψ∂φ

%div %A = 1r2

∂∂r

(r2 Ar) +1

r sin θ∂∂θ

(sin θAθ) +1

r sin θ

∂Aφ

∂φ

∇2 Ψ = 1r2

∂∂r

&r2 ∂Ψ

∂r

'+ 1

r2 sin θ∂∂θ

&sin θ ∂Ψ

∂θ

'+ 1

r2 sin2 θ∂2Ψ∂φ2

Orbits in a gravitational field:

α

r= 1 + ε cos θ a =

k

2|E| b =(#

2µ|E|α =

(2

µk

1. Consider the two forces

%FA = (2y, x, 0) , and %FB = (y + 1, x, 0) .

where the force and position components are, respectively, in newtonsand meters.

(a) [2 pts] Find magnitude of the force %FB at the location(x, y, z) = (−2, 3, 0).

(b) [3 pts] Find the angle that the force %FB makes with the positivedirection of the x-axis at the location (x, y, z) = (−2, 3, 0).

(c) [5 pts] Are either of the forces conservative? If so, determine thecorresponding potential(s).

2. A sailboat of mass m is moving on water, in the direction of wind.The sailboat is subject to two forces in the horizontal direction:%F = %Fa + %Fw, where %Fa is due to air and %Fw is due to water. The forceof air is propelling the sailboat and it is proportional to the differencebetween the constant velocity of the wind %v0 and the boat velocity %v,%Fa = A(%v0 − %v). The force of water resists the motion of the boat and

is proportional to the boat velocity, %Fw = −B %v. Here, A and B arepositive proportionality constants.

v0

Fa

Fw

(a) [2 pt] For what velocity %v of theboat is the net horizontal force onthe boat going to be zero?

(b) [8 pts] Find the dependence of theboat’s velocity v on time t, when theboat starts from rest at t = 0.

By taking the limit t → ∞, verify that the expression you found isconsistent with the answer to (a).

3. A small object of mass m is positionedon a smooth plane and attached to wallson its two sides, at x = 0 and x = L,with stretched massless horizontalsprings of spring constants k1 and k2,respectively, as displayed in the figure.

m k1 k2

xL0

The unstretched lengths of both springs are negligible.

(a) [2 pts] Find the equilibrium position x0 for the mass.

(b) [2 pts] What is the net force acting on the mass in the x direction,if the mass is at a location x, x &= x0 and 0 < x < L?

(c) [4 pts] What is the angular frequency of oscillations about theequilibrium position, in absence of friction? Compute the valuefor m = 2.50 kg, k1 = 3.50N/m, k2 = 1.50N/m and L = 0.90m.Are all constants needed?

(d) [2 pt] If a friction force acts on the mass, opposite and propor-tional to velocity, Ff = −b x, with a proportionality constant ofb = 0.80 kg/s, is the motion underdamped, overdamped or ap-proximately critically damped?

4. A spherical planet of radius R has a density ρ that is the largest atits center, and decreases with distance r from the center as ρ(r) =A (2R− r), where A is a constant with the appropriate units.

(a) [4 pts] Determine the mass of the planet.

(b) [6 pts] Determine the gravitational field at distance r from thecenter of the planet.

5. A satellite is in a circular orbit of radius R around Earth (mass M =5.97× 1024 kg).

(a) [2 pt] How is the velocity v of the satellite related to the radius R,mass M and gravitational constant G?

(b) [4 pts] What needs to be the radius R to make the orbit semisyn-chronous, i.e. with a period of 12h? (GPS satellites move on suchorbits.) Obtain a value for R.

(c) [4 pts] Now imagine that the satellite has a parabolic orbit. If thesatellite has the same angular momentum as it did for the circularorbit, how big is rmin (i.e., the perihelion) compared to R in parta.

6. Consider a pendulum consisting of a mass m suspended by a masslessspring. The spring has a unextended length of b, and a spring constantk. The pendulum is in a uniform gravitational field g.

(a) [5pts] Using Newton’s formulation of mechanics (i.e., F = ma),find equations of motion for the mass in terms of the variablesr and θ. (Note: The acceleration vector in polar coordinates isgiven on the formula sheet.)

(b) [5pts] Using the Lagrangian formulation of mechanics, find theEuler-Lagrange equations for r and θ. Should they agree withpart a)?

7. [Extra Credit] A simple pendulum consists of a massless rod offixed length b with a mass m attached to the end. There is a uniformgravitational field g pointing downwards. Starting at t = 0, thependulum is moved upward with uniform acceleration a.

(a) [4 pts] Write down the Lagrangian in the appropriate set ofgeneralized coordinates. (Hint: Start in cartesian coordinates,and write x, y in terms of θ, b, a, and t.)

(b) [3 pts] Derive the Euler-Lagrange equation of motion.

(c) [3 pts] Find the period of oscillations in the limit of small θ.

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