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| Step | Derivation/Formula | Reasoning |
|---|---|---|
| 1 | \[10g – T_{2} = 10a\] | For the 10 kg block (which moves downward), the net force is its weight minus the rope tension \(T_{2}\) and equals \(10a\). |
| 2 | \[T_{1} – 5g = 5a\] | For the 5 kg block (which moves upward), the net force is the rope tension \(T_{1}\) minus its weight and equals \(5a\). |
| 3 | \[T_{2}=T_{1}\,e^{\mu\pi}\] | Since the rope slips on the pulley, the capstan relation applies over a contact angle of \(\pi\) radians with \(\mu=0.2\); thus, the tension on the heavy side is \(T_{2}=T_{1}\,e^{0.2\pi}\). |
| 4 | \[T_{1}=5g+5a\] | Solve the 5 kg block equation for \(T_{1}\). |
| 5 | \[10g -e^{0.2\pi}(5g+5a)=10a\] | Substitute \(T_{2}=e^{0.2\pi}(5g+5a)\) into the 10 kg block equation. |
| 6 | \[10g-5e^{0.2\pi}g = a(10+5e^{0.2\pi})\] | Distribute and gather like terms in \(a\) and the constants. |
| 7 | \[a = \frac{5g(2-e^{0.2\pi})}{5(2+e^{0.2\pi})} = \frac{g(2-e^{0.2\pi})}{2+e^{0.2\pi}}\] | Simplify the expression to obtain \(a\) in terms of \(g\) and \(e^{0.2\pi}\). |
| 8 | \[a \approx \frac{9.8(2-1.875)}{2+1.875} \approx \frac{9.8(0.125)}{3.875} \approx 0.32\,\text{m/s}^2\] | Using \(e^{0.2\pi}\approx1.875\) and \(g\approx9.8\,\text{m/s}^2\), we find the acceleration. |
| Step | Derivation/Formula | Reasoning |
|---|---|---|
| 1 | \[T_{1}=5g+5a\] | From the 5 kg block equation, solve for \(T_{1}\); substitute \(a\approx0.32\,\text{m/s}^2\) and \(g=9.8\,\text{m/s}^2\). |
| 2 | \[T_{1}\approx5(9.8)+5(0.32)=49+1.6\approx50.6\,\text{N}\] | Calculate \(T_{1}\) numerically. |
| 3 | \[T_{2}=T_{1}\,e^{0.2\pi}\approx50.6\times1.875\approx94.7\,\text{N}\] | Apply the capstan relation to find \(T_{2}\) on the 10 kg side. |
| Step | Derivation/Formula | Reasoning |
|---|---|---|
| 1 | \[f = T_{2}-T_{1}\] | The difference in tensions is provided by the kinetic friction at the pulley–rope interface. |
| 2 | \[f \approx 94.7-50.6 \approx 44.1\,\text{N}\] | Substitute the computed tensions to find the frictional force magnitude. |
| 3 | \[\text{Direction: Counterclockwise}\] | Since the 10 kg block moves downward (causing clockwise tendency), the kinetic friction acts opposite to the rope’s slip, i.e. it exerts a counterclockwise force on the pulley. |
Just ask: "Help me solve this problem."
Two forces produce equal torques on a door about the door hinge. The first force is applied at the midpoint of the door; the second force is applied at the doorknob. Both forces are applied perpendicular to the door. Which force has a greater magnitude?
A boy is sitting at a distance [katex] d_1 [/katex] from the fulcrum, and girl is sitting at a distance [katex] d_2 [/katex] from the fulcrum, with [katex] d_1 > d_2 [/katex]. The seesaw is level, with the two ends at the same height. Derive an equation for the minimum mass of the seesaw that will keep it balanced with the two children on it.
A system consists of two small disks, of masses \( m \) and \( 2m \), attached to ends of a rod of negligible mass of length \( 3x \). The rod is free to turn about a vertical axis through point \( P \). The first mass, \( m \), is located \( x \) away from point \( P \), and therefore the other mass, of \( 2m \), is \( 2x \) from point \( P \). The two disks rest on a rough horizontal surface; the coefficient of friction between the disks and the surface is \( \mu \). At time \( t = 0 \), the rod has an initial counterclockwise angular velocity \( \omega_i \) about \( P \). The system is gradually brought to rest by friction.
Derive expressions for the following quantities in terms of \( \mu \), \( m \), \( x \), \( g \), and \( \omega_i \).
Which of the following must be true for an object at translational equilibrium?
A friend is balancing a fork on one finger. Which of the following are correct explanations of how he accomplishes this? Select two answers.
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| Kinematics | Forces |
|---|---|
| \(\Delta x = v_i t + \frac{1}{2} at^2\) | \(F = ma\) |
| \(v = v_i + at\) | \(F_g = \frac{G m_1 m_2}{r^2}\) |
| \(v^2 = v_i^2 + 2a \Delta x\) | \(f = \mu N\) |
| \(\Delta x = \frac{v_i + v}{2} t\) | \(F_s =-kx\) |
| \(v^2 = v_f^2 \,-\, 2a \Delta x\) |
| Circular Motion | Energy |
|---|---|
| \(F_c = \frac{mv^2}{r}\) | \(KE = \frac{1}{2} mv^2\) |
| \(a_c = \frac{v^2}{r}\) | \(PE = mgh\) |
| \(T = 2\pi \sqrt{\frac{r}{g}}\) | \(KE_i + PE_i = KE_f + PE_f\) |
| \(W = Fd \cos\theta\) |
| Momentum | Torque 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 Motion | Fluids |
|---|---|
| \(F = -kx\) | \(P = \frac{F}{A}\) |
| \(T = 2\pi \sqrt{\frac{l}{g}}\) | \(P_{\text{total}} = P_{\text{atm}} + \rho gh\) |
| \(T = 2\pi \sqrt{\frac{m}{k}}\) | \(Q = Av\) |
| \(x(t) = A \cos(\omega t + \phi)\) | \(F_b = \rho V g\) |
| \(a = -\omega^2 x\) | \(A_1v_1 = A_2v_2\) |
| Constant | Description |
|---|---|
| [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 |
| Variable | SI 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] |
| Variable | Derived 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] |
General Metric Conversion Chart
Example of using unit analysis: Convert 5 kilometers to millimeters.
Start with the given measurement: [katex]\text{5 km}[/katex]
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]
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]
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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