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AP Physics

Unit 6 - Rotational Motion

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(a) Initial Angular Momentum of the System

Step Derivation/Formula Reasoning
1 \[L = I \omega_0\] The angular momentum \(L\) is given by the product of the moment of inertia \(I\) and the angular velocity \(\omega_0\).
2 \[I = m(2l)^2 + 2m(l)^2\] Calculate the moment of inertia \(I\). The moment of inertia for each disk is \(mr^2\), and the total is the sum of each disk’s moment of inertia about point \(P\).
3 \[I = 4ml^2 + 2ml^2 = 6ml^2\] Simplify the expression for the total moment of inertia.
4 \[L = 6ml^2 \omega_0\] Substitute the moment of inertia into the angular momentum formula to find the initial angular momentum.
5 \[\boxed{6ml^2 \omega_0}\] Final expression for the initial angular momentum.

(b) Frictional Torque Acting on the System

Step Derivation/Formula Reasoning
1 \[f_1 = \mu mg\] The frictional force on the disk with mass \(m\) is \(\mu mg\).
2 \[f_2 = \mu (2m)g = 2\mu mg\] The frictional force on the disk with mass \(2m\) is \(2\mu mg\).
3 \[\tau = f_2 \cdot l + f_1 \cdot (2l)\] Calculate the total torque \(\tau\) due to friction using the perpendicular distances \(l\) and \(2l\).
4 \[\tau = (2\mu mg) \cdot l + (\mu mg) \cdot 2l\] Substitute the expressions for the frictional forces.
5 \[\tau = 2\mu mgl + 2\mu mgl = 4\mu mgl\] Simplify to find the total frictional torque.
6 \[\boxed{4\mu mgl}\] Final expression for the frictional torque.

(c) Time \(T\) at Which the System Will Come to Rest

Step Derivation/Formula Reasoning
1 \[\tau = I \alpha\] The torque \(\tau\) is equal to the moment of inertia \(I\) multiplied by the angular deceleration \(\alpha\).
2 \[4\mu mgl = 6ml^2 \alpha\] Substitute the expressions for torque and moment of inertia.
3 \[\alpha = \frac{4\mu g}{6l} = \frac{2\mu g}{3l}\] Solve for angular deceleration \(\alpha\).
4 \[\omega_0 = \alpha T\] Set the initial angular velocity equal to the product of angular deceleration and time to come to rest.
5 \[T = \frac{\omega_0}{\alpha} = \frac{\omega_0 \cdot 3l}{2\mu g}\] Solve for time \(T\).
6 \[\boxed{\frac{3l\omega_0}{2\mu g}}\] Final expression for the time taken to come to rest.

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  1. \(\boxed{6ml^2 \omega_0}\)
  2. \(\tau = 4\mu mgl\). A negative torque is also acceptable.
  3. \(\boxed{\frac{3l\omega_0}{2\mu g}}\)

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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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