AP Physics

Unit 1 - Vectors and Kinematics

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Step Reasoning
Identify that the question asks for the maximum angle \(\theta\) reached by the system, which can be found by relating the kinetic energy immediately after the collision to the change in gravitational potential energy.
\[ K_{rot} = \Delta U_g \]
The maximum angle is reached when all rotational kinetic energy has been converted into gravitational potential energy.
Determine the angular velocity \(\omega\) immediately after the collision using conservation of angular momentum about the pivot point.
\[ L_i = L_f \implies m v_0 L = I_{sys} \omega \]
External forces act at the pivot during the collision, so linear momentum is not conserved, but torque about the pivot is zero, so angular momentum is conserved.
Calculate the rotational inertia \(I_{sys}\) of the rod-projectile system.
\[ I_{sys} = I_{rod} + I_{mass} = \dfrac{1}{3}ML^2 + mL^2 = \left( \dfrac{M+3m}{3} \right)L^2 \]
The system consists of a uniform rod pivoted at its end and a point mass at its far end.
Solve for the rotational kinetic energy \(K_{rot}\) immediately after the collision using the results from steps 2 and 3.
\[ K_{rot} = \dfrac{L_f^2}{2I_{sys}} = \dfrac{(m v_0 L)^2}{2 \left( \frac{M+3m}{3} \right) L^2} = \dfrac{3m^2 v_0^2}{2(M+3m)} \]
This is the total mechanical energy that will be converted into potential energy.
Calculate the change in gravitational potential energy \(\Delta U_g\) as a function of \(\theta\).
\[ \Delta U_g = Mg \Delta y_{rod} + mg \Delta y_{mass} = Mg \frac{L}{2}(1 – \cos\theta) + mgL(1 – \cos\theta) \\
\Delta U_g = \left( \frac{M}{2} + m \right) gL (1 – \cos\theta) = \frac{(M+2m)gL}{2}(1 – \cos\theta) \]
Both the rod and the projectile increase in height. The rod’s center of mass is at \(L/2\) and the projectile is at \(L\).
Equate the kinetic and potential energy and solve for \(\cos\theta\).
\[ \dfrac{3m^2 v_0^2}{2(M+3m)} = \dfrac{(M+2m)gL}{2}(1 – \cos\theta) \\
1 – \cos\theta = \dfrac{3m^2 v_0^2}{(M+3m)(M+2m)gL} \\
\cos\theta = 1 – \dfrac{3m^2 v_0^2}{(M+3m)(M+2m)gL} \]
Conservation of energy between the state immediately after collision and the state at maximum height.

Why each choice is correct or incorrect:

(A) This is the correct answer.

(B) This result occurs if one forgets to include the rod’s potential energy term \(Mg(L/2)(1-\cos\theta)\), only accounting for the point mass.

(C) This result occurs if one incorrectly uses linear momentum conservation (treating the system as if it were not pivoted) and then uses the resulting energy in the pendulum equation.

(D) This result occurs if the student uses the rotational inertia of the rod alone (\(1/3 ML^2\)) for the system’s kinetic energy, ignoring the mass of the embedded projectile in the inertia calculation.

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KinematicsForces
\(\Delta x = v_i t + \frac{1}{2} at^2\)\(F = ma\)
\(v = v_i + at\)\(F_g = \frac{G m_1 m_2}{r^2}\)
\(v^2 = v_i^2 + 2a \Delta x\)\(f = \mu N\)
\(\Delta x = \frac{v_i + v}{2} t\)\(F_s =-kx\)
\(v^2 = v_f^2 \,-\, 2a \Delta x\) 
Circular MotionEnergy
\(F_c = \frac{mv^2}{r}\)\(KE = \frac{1}{2} mv^2\)
\(a_c = \frac{v^2}{r}\)\(PE = mgh\)
\(T = 2\pi \sqrt{\frac{r}{g}}\)\(KE_i + PE_i = KE_f + PE_f\)
 \(W = Fd \cos\theta\)
MomentumTorque and Rotations
\(p = mv\)\(\tau = r \cdot F \cdot \sin(\theta)\)
\(J = \Delta p\)\(I = \sum mr^2\)
\(p_i = p_f\)\(L = I \cdot \omega\)
Simple Harmonic MotionFluids
\(F = -kx\)\(P = \frac{F}{A}\)
\(T = 2\pi \sqrt{\frac{l}{g}}\)\(P_{\text{total}} = P_{\text{atm}} + \rho gh\)
\(T = 2\pi \sqrt{\frac{m}{k}}\)\(Q = Av\)
\(x(t) = A \cos(\omega t + \phi)\)\(F_b = \rho V g\)
\(a = -\omega^2 x\)\(A_1v_1 = A_2v_2\)
ConstantDescription
[katex]g[/katex]Acceleration due to gravity, typically [katex]9.8 , \text{m/s}^2[/katex] on Earth’s surface
[katex]G[/katex]Universal Gravitational Constant, [katex]6.674 \times 10^{-11} , \text{N} \cdot \text{m}^2/\text{kg}^2[/katex]
[katex]\mu_k[/katex] and [katex]\mu_s[/katex]Coefficients of kinetic ([katex]\mu_k[/katex]) and static ([katex]\mu_s[/katex]) friction, dimensionless. Static friction ([katex]\mu_s[/katex]) is usually greater than kinetic friction ([katex]\mu_k[/katex]) as it resists the start of motion.
[katex]k[/katex]Spring constant, in [katex]\text{N/m}[/katex]
[katex] M_E = 5.972 \times 10^{24} , \text{kg} [/katex]Mass of the Earth
[katex] M_M = 7.348 \times 10^{22} , \text{kg} [/katex]Mass of the Moon
[katex] M_M = 1.989 \times 10^{30} , \text{kg} [/katex]Mass of the Sun
VariableSI Unit
[katex]s[/katex] (Displacement)[katex]\text{meters (m)}[/katex]
[katex]v[/katex] (Velocity)[katex]\text{meters per second (m/s)}[/katex]
[katex]a[/katex] (Acceleration)[katex]\text{meters per second squared (m/s}^2\text{)}[/katex]
[katex]t[/katex] (Time)[katex]\text{seconds (s)}[/katex]
[katex]m[/katex] (Mass)[katex]\text{kilograms (kg)}[/katex]
VariableDerived SI Unit
[katex]F[/katex] (Force)[katex]\text{newtons (N)}[/katex]
[katex]E[/katex], [katex]PE[/katex], [katex]KE[/katex] (Energy, Potential Energy, Kinetic Energy)[katex]\text{joules (J)}[/katex]
[katex]P[/katex] (Power)[katex]\text{watts (W)}[/katex]
[katex]p[/katex] (Momentum)[katex]\text{kilogram meters per second (kgm/s)}[/katex]
[katex]\omega[/katex] (Angular Velocity)[katex]\text{radians per second (rad/s)}[/katex]
[katex]\tau[/katex] (Torque)[katex]\text{newton meters (Nm)}[/katex]
[katex]I[/katex] (Moment of Inertia)[katex]\text{kilogram meter squared (kgm}^2\text{)}[/katex]
[katex]f[/katex] (Frequency)[katex]\text{hertz (Hz)}[/katex]

Metric Prefixes

Example of using unit analysis: Convert 5 kilometers to millimeters. 

  1. Start with the given measurement: [katex]\text{5 km}[/katex]

  2. Use the conversion factors for kilometers to meters and meters to millimeters: [katex]\text{5 km} \times \frac{10^3 \, \text{m}}{1 \, \text{km}} \times \frac{10^3 \, \text{mm}}{1 \, \text{m}}[/katex]

  3. Perform the multiplication: [katex]\text{5 km} \times \frac{10^3 \, \text{m}}{1 \, \text{km}} \times \frac{10^3 \, \text{mm}}{1 \, \text{m}} = 5 \times 10^3 \times 10^3 \, \text{mm}[/katex]

  4. Simplify to get the final answer: [katex]\boxed{5 \times 10^6 \, \text{mm}}[/katex]

Prefix

Symbol

Power of Ten

Equivalent

Pico-

p

[katex]10^{-12}[/katex]

Nano-

n

[katex]10^{-9}[/katex]

Micro-

µ

[katex]10^{-6}[/katex]

Milli-

m

[katex]10^{-3}[/katex]

Centi-

c

[katex]10^{-2}[/katex]

Deci-

d

[katex]10^{-1}[/katex]

(Base unit)

[katex]10^{0}[/katex]

Deca- or Deka-

da

[katex]10^{1}[/katex]

Hecto-

h

[katex]10^{2}[/katex]

Kilo-

k

[katex]10^{3}[/katex]

Mega-

M

[katex]10^{6}[/katex]

Giga-

G

[katex]10^{9}[/katex]

Tera-

T

[katex]10^{12}[/katex]

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