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Forces and Momentums

motion

Position

The position (xx) is a vector quantity representing a point in space from a reference origin position.

Time Derivatives of motions

Displacement

The displacement (ss or Δx\Delta x) is a vector quantity representing the change in position as a translation:

\begin`\{aligned}` s = \Delta x = x_f - x_i \end`\{aligned}`

Velocity

The velocity (vv) is a vector quantity representing the change in displacement with time:

\begin`\{aligned}` v = \frac`\{ds}``\{dt}` \end`\{aligned}`

Acceleration

The acceleration (aa) is a vector quantity representing the change in velocity with time:

\begin`\{aligned}` a = \frac`\{dv}``\{dt}` \end`\{aligned}`

Rigid Body

A rigid body is a solid with no deformation regardless of any external forces or moments applied.

Angular Motion

Unit vector for Radial Coordinates

The radial unit vector (r^\bm{\hat{r}}) is the directional vector with magnitude 11 from the center radially outside.

\begin`\{aligned}` \bm{\hat{r}} = \frac{\bm{r}}{|\bm{r}|} \end`\{aligned}`

Centripetal acceleration

The centripetal acceleration (aa) is the acceleration directed radially to the center (r^-\bm{\hat{r}}), keeping the body in circular motion:

\begin`\{aligned}` a = -\frac{v^2}{r}\bm{\hat{r}} = -\omega^2 r\bm{\hat{r}} = -\frac{4\pi^2r}{T^2}\bm{\hat{r}} \end`\{aligned}`
warning

The IB only consider the magnitude of centripetal acceleration, therefore is shown in the equation booklet as:

\begin`\{aligned}` a = \frac{v^2}{r} = \omega^2 r = \frac{4\pi^2r}{T^2} \end`\{aligned}`

Centripetal Force

The centripetal force is any force applied on a mass towards the center (r^-\bm{\hat{r}}), leading to a centripetal acceleration a\bm{a}:

\begin`\{aligned}` F = m\bm{a} = -\frac{mv^2}{r}\bm{\hat{r}} = -m\omega^2 r\bm{\hat{r}} = -\frac{4\pi^2mr}{T^2}\bm{\hat{r}} \end`\{aligned}`
warning

As mentioned above, IB only consider the magnitude of centripetal force:

\begin`\{aligned}` F = ma = \frac{mv^2}{r} = m\omega^2 r = \frac{4\pi^2mr}{T^2} \end`\{aligned}`

Angular Position

The angular position (θ\theta) of a rigid body is a representation of the object's orientation by the angle between a reference position and the current position.

Time Derivatives of Angular Motions

Angular Displacement

The angular displacement (Δθ\Delta \theta) of a rigid body is the change in angular position θ\theta measured from the center:

\begin`\{aligned}` \Delta \theta = \theta_f - \theta_i \end`\{aligned}`

Angular velocity

The angular velocity (ω\omega) is the change of angular displacement Δθ\Delta \theta of a rigid body with time:

\begin`\{aligned}` \omega = \frac{d\theta}`\{dt}` \end`\{aligned}`

Angular acceleration

The angular acceleration (α\alpha) is the change of angular velocity of a rigid body with time:

\begin`\{aligned}` \alpha = \frac{d\omega}`\{dt}` \end`\{aligned}`

Moment of Inertia

The measure of a solid body's resistance to angular acceleration.

warning

The IB syllabus only consider the moment of inertia of rigid body with approximated geometry as a system of discrete particles, as well as moment of inertia that is determined by closed-form expressions.

Angular Momentum

The angular momentum (LL) is the product of moment of inertia II and angular velocity ω\omega:

\begin`\{aligned}` L = I\omega \end`\{aligned}`

Work

The work (WW) done by a force FF on a point mass with a movement of displacement ss is:

\begin`\{aligned}` W = \bm{F} \cdot \bm{s} = |\bm{F}||\bm{s}|\cos\theta \end`\{aligned}`
info

For a force that varies at different position, the line integral of FF across a surface CC is:

\begin`\{aligned}` W = \int_C F \cdot ds \end`\{aligned}`

Wrap Up

A.1 Kinematics & A.2 Forces and Momentum

Problem 1. A 1500 kg car is traveling on a horizontal road at a constant speed of 25.0 m/s. The total resistive force (air drag + friction) is 800 N. The car then begins to accelerate uniformly for 10.0 s, reaching a new constant speed. During the acceleration, the engine provides a constant driving force of 2000 N. a) Calculate the car's acceleration. b) What is the final speed of the car? c) At this new speed, what must the engine's driving force be to maintain it? d) What is the total distance covered during the 10.0 s of acceleration?

Answer
  • Strategy: Apply Newton's Second Law during acceleration and the definition of constant velocity (net force is zero) for the other parts. Use kinematics for the distance.
  • a) Acceleration: During acceleration, the net force is Fnet=FdriveFresistiveF_{\mathrm{net}} = F_{\mathrm{drive}} - F_{\mathrm{resistive}}.
    • Fnet=2000N800N=1200NF_{\mathrm{net}} = 2000 \mathrm{ N} - 800 \mathrm{ N} = 1200 \mathrm{ N}.
    • From Newton's Second Law, Fnet=ma    a=Fnetm=1200N1500kg=0.800m/s2F_{\mathrm{net}} = ma \implies a = \frac{F_{\mathrm{net}}}{m} = \frac{1200 \mathrm{ N}}{1500 \mathrm{ kg}} = 0.800 \mathrm{ m/s}^2.
  • b) Final Speed: Use the kinematic equation v=u+atv = u + at.
    • v=25.0m/s+(0.800m/s2)(10.0s)=25.0+8.0=33.0m/sv = 25.0 \mathrm{ m/s} + (0.800 \mathrm{ m/s}^2)(10.0 \mathrm{ s}) = 25.0 + 8.0 = 33.0 \mathrm{ m/s}.
  • c) New Driving Force: To maintain a constant speed of 33.0 m/s, the car must be in equilibrium (zero acceleration). This means the net force is zero.
    • Fnet=FdriveFresistive=0F_{\mathrm{net}} = F_{\mathrm{drive}} - F_{\mathrm{resistive}} = 0.
    • Therefore, Fdrive=Fresistive=800NF_{\mathrm{drive}} = F_{\mathrm{resistive}} = 800 \mathrm{ N}. (This assumes resistive force is constant, a simplification.)
  • d) Distance: Use the kinematic equation s=ut+12at2s = ut + \frac{1}{2}at^2.
    • s=(25.0m/s)(10.0s)+12(0.800m/s2)(10.0s)2=250+0.4(100)=290ms = (25.0 \mathrm{ m/s})(10.0 \mathrm{ s}) + \frac{1}{2}(0.800 \mathrm{ m/s}^2)(10.0 \mathrm{ s})^2 = 250 + 0.4(100) = 290 \mathrm{ m}. If you get this wrong, you should focus on: Applying Newton's First Law (Fnet=0F_{\mathrm{net}}=0 for constant velocity) and Second Law (Fnet=maF_{\mathrm{net}}=ma for acceleration), and correctly linking the resulting acceleration to kinematic equations.

Problem 2. A 2.0 kg firework is launched vertically from rest. Its rocket motor provides a constant upward thrust of 50.0 N for 3.0 s before running out of fuel. Ignore air resistance. a) Calculate the maximum height the firework reaches. b) What is the total time the firework is in the air (from launch until it returns to the ground)?

Answer
  • Strategy: This is a two-stage motion problem. Stage 1 (powered ascent) has a net upward force. Stage 2 (coasting ascent and descent) has only gravity acting on it.
  • Stage 1: Powered Ascent (first 3.0 s)
    • Net force: Fnet=FthrustFg=50.0N(2.0kg)(9.8m/s2)=50.019.6=30.4NF_{\mathrm{net}} = F_{\mathrm{thrust}} - F_g = 50.0 \mathrm{ N} - (2.0 \mathrm{ kg})(9.8 \mathrm{ m/s}^2) = 50.0 - 19.6 = 30.4 \mathrm{ N}.
    • Acceleration: a1=Fnet/m=30.4/2.0=15.2m/s2a_1 = F_{\mathrm{net}}/m = 30.4 / 2.0 = 15.2 \mathrm{ m/s}^2.
    • Height reached in Stage 1: h1=12a1t2=12(15.2)(3.0)2=68.4mh_1 = \frac{1}{2}a_1 t^2 = \frac{1}{2}(15.2)(3.0)^2 = 68.4 \mathrm{ m}.
    • Velocity at end of Stage 1: v1=a1t=15.2×3.0=45.6m/sv_1 = a_1 t = 15.2 \times 3.0 = 45.6 \mathrm{ m/s}.
  • Stage 2: Coasting Motion (after 3.0 s)
    • The firework now has an initial upward velocity of 45.6 m/s and is at a height of 68.4 m. The only acceleration is a2=g=9.8m/s2a_2 = -g = -9.8 \mathrm{ m/s}^2.
    • a) Maximum Height: Find the additional height (h2h_2) it coasts upwards. Use v2=u2+2asv^2 = u^2 + 2as.
      • 02=(45.6)2+2(9.8)h2    h2=45.6219.6=106.0m0^2 = (45.6)^2 + 2(-9.8)h_2 \implies h_2 = \frac{45.6^2}{19.6} = 106.0 \mathrm{ m}.
      • Total max height: H=h1+h2=68.4+106.0=174.4mH = h_1 + h_2 = 68.4 + 106.0 = 174.4 \mathrm{ m}.
    • b) Total Time in Air: We need the time for Stage 2. - Time to coast to peak (tupt_{\mathrm{up}}): v=u+at    0=45.69.8tup    tup=4.65sv = u + at \implies 0 = 45.6 - 9.8 t_{\mathrm{up}} \implies t_{\mathrm{up}} = 4.65 \mathrm{ s}. - Time to fall from peak (tdownt_{\mathrm{down}}): s=12at2    174.4=12(9.8)tdown2    tdown=5.97ss = \frac{1}{2}at^2 \implies 174.4 = \frac{1}{2}(9.8) t_{\mathrm{down}}^2 \implies t_{\mathrm{down}} = 5.97 \mathrm{ s}. - Total time: T=t1+tup+tdown=3.0+4.65+5.97=13.6sT = t_1 + t_{\mathrm{up}} + t_{\mathrm{down}} = 3.0 + 4.65 + 5.97 = 13.6 \mathrm{ s}. If you get this wrong, you should focus on: Breaking multi-stage motion problems into separate parts, calculating net force correctly in each stage, and using the final conditions of one stage as the initial conditions for the next.

Problem 3. A 5.0 kg object is suspended by a rope. A horizontal force is applied, pulling the object to the side until the rope makes an angle of 35° with the vertical. The object is held in static equilibrium. a) Draw a free-body diagram for the object. b) Calculate the magnitude of the applied horizontal force and the tension in the rope.

Answer
  • a) Free-Body Diagram: The diagram should show three forces acting on the object:
    1. Weight (Fg=mgF_g = mg) acting vertically downwards.
    2. Tension (TT) acting upwards along the rope at 35° to the vertical.
    3. Applied Horizontal Force (FaF_a) acting horizontally.
  • b) Calculate Forces: The object is in static equilibrium, so the net force in both the horizontal and vertical directions is zero. Resolve the tension into components.
    • Let the angle with the vertical be θ=35\theta = 35^\circ.
    • Vertical component of tension: Ty=Tcos(θ)T_y = T \cos(\theta).
    • Horizontal component of tension: Tx=Tsin(θ)T_x = T \sin(\theta).
    • Vertical Equilibrium (ΣFy=0\Sigma F_y = 0):
      • Tymg=0    Tcos(35)=(5.0kg)(9.8m/s2)=49NT_y - mg = 0 \implies T \cos(35^\circ) = (5.0 \mathrm{ kg})(9.8 \mathrm{ m/s}^2) = 49 \mathrm{ N}.
      • T=49cos(35)=59.8NT = \frac{49}{\cos(35^\circ)} = 59.8 \mathrm{ N}.
    • Horizontal Equilibrium (ΣFx=0\Sigma F_x = 0): - FaTx=0    Fa=Tsin(35)F_a - T_x = 0 \implies F_a = T \sin(35^\circ). - Fa=(59.8N)sin(35)=34.3NF_a = (59.8 \mathrm{ N}) \sin(35^\circ) = 34.3 \mathrm{ N}. If you get this wrong, you should focus on: The conditions for static equilibrium (ΣF=0\Sigma F = 0), correctly resolving vectors into components using trigonometry, and setting up and solving simultaneous equations for the vertical and horizontal forces.

Problem 4. A 0.20 kg ball traveling at 10 m/s collides with a stationary 0.30 kg ball. After the collision, the 0.20 kg ball moves at 4.0 m/s at an angle of 30° to its original path. a) Determine the speed and direction of the 0.30 kg ball after the collision. b) Was the collision elastic? Justify your answer with a calculation.

Answer
  • Strategy: This is a 2D collision. Apply conservation of momentum separately for the components parallel and perpendicular to the initial direction. Then compare kinetic energy before and after.
  • Let the initial direction be the x-axis. Initial momentum is all in x: pi=(0.20)(10)=2.0p_i = (0.20)(10) = 2.0 kg m/s.
  • a) Conservation of Momentum:
    • x-direction: pix=pfx    2.0=(0.20)(4.0cos30)+(0.30)v2xp_{ix} = p_{fx} \implies 2.0 = (0.20)(4.0 \cos 30^\circ) + (0.30)v_{2x}.
      • 2.0=0.693+0.30v2x    v2x=4.362.0 = 0.693 + 0.30v_{2x} \implies v_{2x} = 4.36 m/s.
    • y-direction: piy=pfy    0=(0.20)(4.0sin30)+(0.30)v2yp_{iy} = p_{fy} \implies 0 = (0.20)(4.0 \sin 30^\circ) + (0.30)v_{2y}.
      • 0=0.40+0.30v2y    v2y=1.330 = 0.40 + 0.30v_{2y} \implies v_{2y} = -1.33 m/s.
    • Speed and Direction of 2nd ball:
      • Speed: v2=v2x2+v2y2=4.362+(1.33)2=4.56v_2 = \sqrt{v_{2x}^2 + v_{2y}^2} = \sqrt{4.36^2 + (-1.33)^2} = 4.56 m/s.
      • Direction: θ=arctan(v2yv2x)=arctan(1.334.36)=17.0\theta = \arctan\left(\frac{v_{2y}}{v_{2x}}\right) = \arctan\left(\frac{-1.33}{4.36}\right) = -17.0^\circ (below the original path).
  • b) Elasticity: Compare initial and final total kinetic energy.
    • Ek,initial=12(0.20)(10)2=10.0E_{k, \mathrm{initial}} = \frac{1}{2}(0.20)(10)^2 = 10.0 J.
    • Ek,final=12(0.20)(4.0)2+12(0.30)(4.56)2=1.6+3.12=4.72E_{k, \mathrm{final}} = \frac{1}{2}(0.20)(4.0)^2 + \frac{1}{2}(0.30)(4.56)^2 = 1.6 + 3.12 = 4.72 J.
    • Since Ek,final<Ek,initialE_{k, \mathrm{final}} \lt{} E_{k, \mathrm{initial}}, kinetic energy was lost, and the collision was inelastic. If you get this wrong, you should focus on: Applying conservation of momentum as a vector equation (i.e., in component form), combining velocity components to find final speed and direction, and the definition of an elastic collision (conservation of kinetic energy).

Problem 5. A 1200 kg car travels at a constant speed of 15 m/s around a flat circular track of radius 50 m. It then moves to a section of the track banked at an angle θ\theta. a) For the flat track, what is the magnitude of the frictional force required to keep the car on the track, and what is the minimum coefficient of static friction required? b) For the banked track, what is the ideal banking angle θ\theta (the "design speed" angle) for the car to navigate the turn at 15 m/s without any reliance on friction?

Answer
  • Strategy: In both cases, a net horizontal force must provide the centripetal force. On the flat track, this is friction. On the ideal banked track, this is the horizontal component of the normal force.
  • a) Flat Track:
    • The centripetal force required is Fc=mv2r=120015250=5400F_c = \frac{mv^2}{r} = \frac{1200 \cdot 15^2}{50} = 5400 N.
    • This force is provided entirely by static friction, so fs=5400f_s = 5400 N.
    • The maximum static friction is fs,max=μsN=μsmgf_{s,\mathrm{max}} = \mu_s N = \mu_s mg.
    • To avoid slipping, we need fsfs,max    5400μs(1200)(9.8)f_s \le f_{s,\mathrm{max}} \implies 5400 \le \mu_s(1200)(9.8).
    • μs540011760=0.46\mu_s \ge \frac{5400}{11760} = 0.46. The minimum coefficient of static friction is 0.46.
  • b) Banked Track (No Friction):
    • Draw a free-body diagram showing only weight (mgmg) down and the normal force (NN) perpendicular to the banked surface.
    • Resolve the normal force into components: Ny=NcosθN_y = N \cos\theta and Nx=NsinθN_x = N \sin\theta.
    • Vertical equilibrium: Ny=mg    Ncosθ=mgN_y = mg \implies N \cos\theta = mg.
    • Horizontal net force: The horizontal component provides the centripetal force: Nx=Fc    Nsinθ=mv2rN_x = F_c \implies N \sin\theta = \frac{mv^2}{r}.
    • Divide the horizontal equation by the vertical equation to eliminate N:
      • NsinθNcosθ=mv2/rmg    tanθ=v2rg\frac{N \sin\theta}{N \cos\theta} = \frac{mv^2/r}{mg} \implies \tan\theta = \frac{v^2}{rg}.
    • tanθ=152509.8=0.459\tan\theta = \frac{15^2}{50 \cdot 9.8} = 0.459.
    • θ=arctan(0.459)=24.7\theta = \arctan(0.459) = 24.7^\circ. If you get this wrong, you should focus on: Identifying the source of the centripetal force in different situations (friction vs. component of normal force), correctly resolving forces on an inclined plane, and solving a system of force equations.

Problem 6. Question (HL Only): A thin hoop of mass M and radius R (I=MR2I=MR^2) rolls without slipping down an incline of angle θ\theta. a) Draw a free-body diagram for the hoop, including the force of static friction. b) By considering both linear and rotational dynamics, derive an expression for the linear acceleration, aa, of the hoop's center of mass. c) How does this acceleration compare to that of a block sliding down the same incline without friction?

Answer
  • a) Free-Body Diagram: The diagram should show:
    1. Weight (MgMg) acting vertically down from the center.
    2. Normal force (NN) acting perpendicular to the incline, from the point of contact.
    3. Static friction (fsf_s) acting up the incline, at the point of contact. (This friction provides the torque to make it rotate).
  • b) Derive Acceleration:
    • Linear Motion (down the incline): Fnet=Ma    Mgsinθfs=MaF_{\mathrm{net}} = Ma \implies Mg \sin\theta - f_s = Ma. (Eq. 1)
    • Rotational Motion (about the center): The only force providing a torque is friction. τnet=Iα    fsR=(MR2)α\tau_{\mathrm{net}} = I\alpha \implies f_s R = (MR^2)\alpha. (Eq. 2)
    • No-slip condition: a=αR    α=a/Ra = \alpha R \implies \alpha = a/R.
    • Substitute the no-slip condition into Eq. 2: fsR=MR2(a/R)    fs=Maf_s R = MR^2(a/R) \implies f_s = Ma.
    • Substitute this expression for fsf_s back into Eq. 1:
      • MgsinθMa=Ma    Mgsinθ=2MaMg \sin\theta - Ma = Ma \implies Mg \sin\theta = 2Ma.
      • a=12gsinθa = \frac{1}{2}g \sin\theta.
  • c) Comparison: A block sliding without friction has only the component of gravity accelerating it, so its acceleration is ablock=gsinθa_{\mathrm{block}} = g \sin\theta. The hoop's acceleration is exactly half of this. This is because some of the initial potential energy must be converted into rotational kinetic energy, leaving less for translational kinetic energy, resulting in a smaller linear acceleration. If you get this wrong, you should focus on: Applying both linear and rotational forms of Newton's second law, correctly identifying static friction as the source of torque for rolling objects, and using the no-slip condition (a=αRa=\alpha R) to connect the two equations.

Problem 7. Question (HL Only): An ice skater is spinning at an angular speed of 10.0 rad/s with her arms outstretched. In this position, her moment of inertia is 4.0 kg m². She then pulls her arms in, reducing her moment of inertia to 1.5 kg m². a) What is her new angular speed? b) Calculate the change in her rotational kinetic energy. c) Where does this change in energy come from?

Answer
  • Strategy: Apply conservation of angular momentum because there is no external torque. Then calculate the kinetic energy before and after.
  • a) New Angular Speed:
    • Conservation of angular momentum: Li=Lf    Iiωi=IfωfL_i = L_f \implies I_i \omega_i = I_f \omega_f.
    • (4.0kgm2)(10.0rad/s)=(1.5kgm2)ωf(4.0 \mathrm{ kg m}^2)(10.0 \mathrm{ rad/s}) = (1.5 \mathrm{ kg m}^2) \omega_f.
    • ωf=40.01.5=26.7\omega_f = \frac{40.0}{1.5} = 26.7 rad/s.
  • b) Change in Rotational Kinetic Energy:
    • Ek,initial=12Iiωi2=12(4.0)(10.0)2=200E_{k, \mathrm{initial}} = \frac{1}{2}I_i \omega_i^2 = \frac{1}{2}(4.0)(10.0)^2 = 200 J.
    • Ek,final=12Ifωf2=12(1.5)(26.7)2=533E_{k, \mathrm{final}} = \frac{1}{2}I_f \omega_f^2 = \frac{1}{2}(1.5)(26.7)^2 = 533 J.
    • ΔEk=Ek,finalEk,initial=533200=333\Delta E_k = E_{k, \mathrm{final}} - E_{k, \mathrm{initial}} = 533 - 200 = 333 J.
  • c) Source of Energy: The kinetic energy increased. This increase comes from the work done by the skater using her muscles to pull her arms inward. She is doing work on her own system, which is not an isolated system in terms of energy (though it is for angular momentum, as the forces are internal). If you get this wrong, you should focus on: The law of conservation of angular momentum and when it applies (no net external torque). Also, understanding that rotational kinetic energy is not necessarily conserved when the moment of inertia changes, and that work must be done to change the configuration of a rotating system.

Problem 8. Question (HL Only): From the perspective of an observer in a laboratory, a muon is created by a cosmic ray at an altitude of 10.0 km. It travels downwards at a speed of 0.995c. The proper half-life of a muon at rest is 1.56 μs. a) From the lab observer's perspective, what is the muon's half-life? b) Will the muon reach the ground before decaying, according to the lab observer? Justify with a calculation. c) Now, analyze the situation from the muon's reference frame. How does the muon "explain" its ability to reach the ground?

Answer
  • Strategy: Use time dilation for the lab frame analysis and length contraction for the muon's frame analysis.
  • a) Dilated Half-Life (Lab Frame):
    • γ=11v2/c2=110.9952=10.01\gamma = \frac{1}{\sqrt{1 - v^2/c^2}} = \frac{1}{\sqrt{1 - 0.995^2}} = 10.01.
    • The dilated half-life is Δt=γΔt0=10.01×(1.56×106s)=1.56×105\Delta t = \gamma \Delta t_0 = 10.01 \times (1.56 \times 10^{-6} \mathrm{ s}) = 1.56 \times 10^{-5} s.
  • b) Survival in Lab Frame:
    • Time for the muon to travel 10.0 km: ttravel=distancespeed=10000m0.995×3.0×108m/s=3.35×105t_{\mathrm{travel}} = \frac{\mathrm{distance}}{\mathrm{speed}} = \frac{10000 \mathrm{ m}}{0.995 \times 3.0 \times 10^8 \mathrm{ m/s}} = 3.35 \times 10^{-5} s.
    • ttravel=33.5t_{\mathrm{travel}} = 33.5 μs. The dilated half-life is 15.6 μs.
    • Since the travel time (33.5 μs) is longer than one dilated half-life (15.6 μs), less than half the muons will survive. Specifically, the number of half-lives passed is 33.5/15.62.1533.5/15.6 \approx 2.15. A significant fraction will reach the ground. (The question is simply "will it reach", implying does it have time. Yes, it has time before it all decays).
  • c) Muon's Reference Frame:
    • In its own frame, the muon's half-life is just the proper half-life, Δt0=1.56\Delta t_0 = 1.56 μs. It "lives" for only a short time.
    • From the muon's perspective, the Earth and its atmosphere are rushing towards it at 0.995c. The distance of 10.0 km is length contracted.
    • Contracted distance: L=L0γ=10.0km10.01=0.999L = \frac{L_0}{\gamma} = \frac{10.0 \mathrm{ km}}{10.01} = 0.999 km or 999 m.
    • Time to travel this contracted distance: t=Lv=999m0.995×3.0×108m/s=3.35×106t' = \frac{L}{v} = \frac{999 \mathrm{ m}}{0.995 \times 3.0 \times 10^8 \mathrm{ m/s}} = 3.35 \times 10^{-6} s = 3.35 μs.
    • From the muon's perspective, it only needs to survive for 3.35 μs to reach the ground. Since this is longer than its proper half-life of 1.56 μs, it has a chance to make it. Both frames agree on the outcome. If you get this wrong, you should focus on: The two key consequences of special relativity. For a stationary observer watching a moving object, time dilates (clocks run slow). For a moving observer, distances in the direction of motion contract (are shorter). Both phenomena must lead to the same physical conclusion.

Worked Example: Connected Bodies on a Frictionless Surface

Problem: Two blocks, m1=3.0m_1 = 3.0 kg and m2=5.0m_2 = 5.0 kg, are connected by a light inextensible string. Block m1m_1 rests on a frictionless horizontal table, and the string passes over a frictionless pulley at the edge so that m2m_2 hangs vertically. The system is released from rest. a) Find the acceleration of the system. b) Find the tension in the string.

Solution:

For m2m_2 (hanging): m2gT=m2am_2 g - T = m_2 a (Eq. 1) For m1m_1 (on table): T=m1aT = m_1 a (Eq. 2, since no friction)

Substitute Eq. 2 into Eq. 1: m2gm1a=m2am_2 g - m_1 a = m_2 a m2g=(m1+m2)am_2 g = (m_1 + m_2) a a=m2gm1+m2=(5.0)(9.8)3.0+5.0=498.0=6.13a = \frac{m_2 g}{m_1 + m_2} = \frac{(5.0)(9.8)}{3.0 + 5.0} = \frac{49}{8.0} = 6.13 m/s2^2

Tension: T=m1a=(3.0)(6.13)=18.4T = m_1 a = (3.0)(6.13) = 18.4 N.


Worked Example: Inclined Plane with Friction

Problem: A 4.0 kg block is placed on a 3030^\circ incline. The coefficient of static friction is μs=0.40\mu_s = 0.40 and the coefficient of kinetic friction is μk=0.30\mu_k = 0.30. a) Will the block slide? Justify with a calculation. b) If a horizontal force of 20 N is applied pushing the block up the incline, find the acceleration.

Solution:

a) Check if block slides: Component of gravity along the incline: mgsin30=(4.0)(9.8)(0.5)=19.6mg\sin 30^{\circ} = (4.0)(9.8)(0.5) = 19.6 N. Maximum static friction: fs,max=μsmgcos30=(0.40)(4.0)(9.8)(0.866)=13.6f_{s,\max} = \mu_s mg\cos 30^{\circ} = (0.40)(4.0)(9.8)(0.866) = 13.6 N. Since mgsin30=19.6mg\sin 30^{\circ} = 19.6 N >fs,max=13.6\gt{} f_{s,\max} = 13.6 N, the block will slide.

b) With applied horizontal force of 20 N up the incline: Resolve the horizontal force into components parallel and perpendicular to the incline: F=20cos30=17.3F_{\parallel} = 20\cos 30^{\circ} = 17.3 N (up the incline). F=20sin30=10.0F_{\perp} = 20\sin 30^{\circ} = 10.0 N (into the incline).

Normal force: N=mgcos30+F=(4.0)(9.8)(0.866)+10.0=33.9+10.0=43.9N = mg\cos 30^{\circ} + F_{\perp} = (4.0)(9.8)(0.866) + 10.0 = 33.9 + 10.0 = 43.9 N. Kinetic friction: fk=μkN=(0.30)(43.9)=13.2f_k = \mu_k N = (0.30)(43.9) = 13.2 N (down the incline).

Net force along the incline: Fnet=Fmgsin30fk=17.319.613.2=15.5F_{\mathrm{net}} = F_{\parallel} - mg\sin 30^{\circ} - f_k = 17.3 - 19.6 - 13.2 = -15.5 N.

The net force is negative (down the incline), meaning the block slides down despite the applied force. The acceleration is: a=Fnetm=15.54.0=3.88a = \frac{|F_{\mathrm{net}}|}{m} = \frac{15.5}{4.0} = 3.88 m/s2^2 down the incline.


Worked Example: Torque and Rotational Equilibrium

Problem: A uniform beam of mass 10 kg and length 4.0 m is pivoted at its left end. A load of 15 kg is hung from the beam at a point 3.0 m from the pivot. The beam is held in horizontal equilibrium by a vertical rope attached 1.0 m from the right end. a) Calculate the tension in the rope. b) Calculate the magnitude and direction of the reaction force at the pivot.

Solution:

a) Take moments about the pivot (clockwise positive):

Clockwise moments:

  • Weight of beam: (10)(9.8)(2.0)=196(10)(9.8)(2.0) = 196 N m (acts at the center, 2.0 m from pivot).
  • Weight of load: (15)(9.8)(3.0)=441(15)(9.8)(3.0) = 441 N m.

Anticlockwise moments:

  • Tension in rope: T(4.01.0)=3.0TT(4.0 - 1.0) = 3.0T.

For equilibrium: 3.0T=196+441=6373.0T = 196 + 441 = 637. T=212.3T = 212.3 N.

b) Vertical equilibrium: Rpivot+T=mgbeam+mgloadR_{\mathrm{pivot}} + T = mg_{\mathrm{beam}} + mg_{\mathrm{load}} Rpivot+212.3=98+147=245R_{\mathrm{pivot}} + 212.3 = 98 + 147 = 245 Rpivot=32.7R_{\mathrm{pivot}} = 32.7 N (upward).


Angular Momentum Conservation: Extended Analysis

The law of conservation of angular momentum states that when no net external torque acts on a system, the total angular momentum remains constant:

Linitial=Lfinal    Iiωi=IfωfL_{\mathrm{initial}} = L_{\mathrm{final}} \implies I_i \omega_i = I_f \omega_f

This principle explains a wide range of phenomena:

  • Spinning ice skater: Pulling arms in reduces II, so ω\omega must increase.
  • Spinning neutron star: When a star collapses, its moment of inertia decreases enormously, causing extremely rapid rotation (pulsars can spin at hundreds of revolutions per second).
  • Orbital mechanics: A planet in an elliptical orbit moves faster at perihelion (closer to the star, smaller effective rr) and slower at aphelion (farther, larger effective rr).

Important distinction: Angular momentum is conserved when the net external torque is zero. Internal forces (like the skater's muscles) can change II and ω\omega, but not the total LL. However, internal forces can change the rotational kinetic energy (as seen in the skater problem where EkE_k increased).


Common Pitfalls

  1. Centripetal force is not a "new" force. It is the net force directed toward the center. Always identify which force(s) provide the centripetal force: tension, friction, component of gravity, normal force, etc.

  2. Confusing centripetal and centrifugal force. Centrifugal force is a fictitious force that appears in a rotating reference frame. In an inertial frame, only centripetal force exists.

  3. Forgetting that rolling involves both translation and rotation. A rolling object has both translational kinetic energy (12mv2\frac{1}{2}mv^2) and rotational kinetic energy (12Iω2\frac{1}{2}I\omega^2). The total is 12mv2(1+Imr2)\frac{1}{2}mv^2(1 + \frac{I}{mr^2}).

  4. Sign conventions in angular momentum. Define a positive direction of rotation and be consistent. Clockwise and counterclockwise torques must be assigned opposite signs.

  5. Using the wrong moment of inertia. For a solid sphere I=25mr2I = \frac{2}{5}mr^2; for a hollow sphere I=23mr2I = \frac{2}{3}mr^2; for a solid cylinder I=12mr2I = \frac{1}{2}mr^2; for a thin hoop I=mr2I = mr^2. These are different and must be used correctly.

  6. Equating centripetal acceleration to gravity. g=v2/rg = v^2/r only applies at the surface of a planet for orbital motion. Do not use it for objects on the surface (unless explicitly stated).


Problem Set

Question 1

A 2.0 kg block slides down a frictionless incline of angle 3535^\circ from a height of 1.5 m. a) Find the speed of the block at the bottom of the incline. b) The block then slides across a rough horizontal surface with μk=0.30\mu_k = 0.30. How far does it travel before stopping?

Answer 1

a) By conservation of energy: mgh=12mv2    v=2gh=2(9.8)(1.5)=29.4=5.42mgh = \frac{1}{2}mv^2 \implies v = \sqrt{2gh} = \sqrt{2(9.8)(1.5)} = \sqrt{29.4} = 5.42 m/s.

b) On the rough surface, friction decelerates the block: fk=μkmg=(0.30)(2.0)(9.8)=5.88f_k = \mu_k mg = (0.30)(2.0)(9.8) = 5.88 N. a=fkm=5.882.0=2.94a = \frac{f_k}{m} = \frac{5.88}{2.0} = 2.94 m/s2^2. Using v2=u2+2asv^2 = u^2 + 2as: 0=(5.42)22(2.94)s    s=29.45.88=5.00 = (5.42)^2 - 2(2.94)s \implies s = \frac{29.4}{5.88} = 5.0 m.

Question 2

A 500 g ball is attached to a string of length 0.80 m and swung in a vertical circle. The minimum speed at the top of the circle is 2.82.8 m/s. a) Calculate the tension in the string at the top of the circle. b) Calculate the speed of the ball at the bottom of the circle (assuming no energy losses).

Answer 2

a) At the top: T+mg=mv2rT + mg = \frac{mv^2}{r}. T=mv2rmg=(0.50)(2.8)20.80(0.50)(9.8)=3.920.804.9=4.94.9=0T = \frac{mv^2}{r} - mg = \frac{(0.50)(2.8)^2}{0.80} - (0.50)(9.8) = \frac{3.92}{0.80} - 4.9 = 4.9 - 4.9 = 0 N. (This confirms the minimum speed condition where tension equals zero at the top.)

b) Conservation of energy: 12mvb2=12mvt2+mg(2r)\frac{1}{2}mv_b^2 = \frac{1}{2}mv_t^2 + mg(2r). vb=vt2+4gr=(2.8)2+4(9.8)(0.80)=7.84+31.36=39.2=6.26v_b = \sqrt{v_t^2 + 4gr} = \sqrt{(2.8)^2 + 4(9.8)(0.80)} = \sqrt{7.84 + 31.36} = \sqrt{39.2} = 6.26 m/s.

Question 3

A disc of mass 0.50 kg and radius 0.20 m (I=12mr2I = \frac{1}{2}mr^2) is rotating at 300 rpm. A frictional torque of 0.030 N m is applied to bring it to rest. a) Calculate the initial angular momentum. b) How long does it take for the disc to stop?

Answer 3

a) ωi=300×2π60=31.4\omega_i = 300 \times \frac{2\pi}{60} = 31.4 rad/s. I=12(0.50)(0.20)2=0.010I = \frac{1}{2}(0.50)(0.20)^2 = 0.010 kg m2^2. Li=Iωi=(0.010)(31.4)=0.314L_i = I\omega_i = (0.010)(31.4) = 0.314 kg m2^2/s.

b) τ=ΔLΔt    Δt=Liτ=0.3140.030=10.5\tau = \frac{\Delta L}{\Delta t} \implies \Delta t = \frac{L_i}{\tau} = \frac{0.314}{0.030} = 10.5 s.

Question 4

A 60 kg person stands at the edge of a rotating platform of mass 100 kg and radius 2.0 m, modeled as a uniform disc (I=12mr2I = \frac{1}{2}mr^2). The system rotates at 1.5 rad/s. The person walks to the center of the platform. What is the new angular speed?

Answer 4

Idisc=12(100)(2.0)2=200I_{\mathrm{disc}} = \frac{1}{2}(100)(2.0)^2 = 200 kg m2^2. Iperson,initial=mr2=(60)(2.0)2=240I_{\mathrm{person, initial}} = mr^2 = (60)(2.0)^2 = 240 kg m2^2. Iperson,final=0I_{\mathrm{person, final}} = 0 (at the center, r=0r = 0).

Ii=200+240=440I_i = 200 + 240 = 440 kg m2^2, ωi=1.5\omega_i = 1.5 rad/s. If=200+0=200I_f = 200 + 0 = 200 kg m2^2.

Conservation: Iiωi=Ifωf    (440)(1.5)=200ωfI_i\omega_i = I_f\omega_f \implies (440)(1.5) = 200\omega_f. ωf=660200=3.3\omega_f = \frac{660}{200} = 3.3 rad/s.

Question 5

A 3.0 kg block on a frictionless table is connected by a string over a pulley to a 2.0 kg block hanging vertically. The pulley has mass 0.50 kg and radius 0.10 m (I=12mr2I = \frac{1}{2}mr^2 for the pulley). a) Derive an expression for the acceleration of the system. b) Calculate the tension on each side of the pulley.

Answer 5

a) Let T1T_1 be the tension on the table side and T2T_2 on the hanging side. For m1m_1 (on table): T1=m1aT_1 = m_1 a (Eq. 1). For m2m_2 (hanging): m2gT2=m2am_2 g - T_2 = m_2 a (Eq. 2). For pulley: (T2T1)R=Iα=(12mpR2)(a/R)=12mpRa(T_2 - T_1)R = I\alpha = (\frac{1}{2}m_p R^2)(a/R) = \frac{1}{2}m_p Ra. So T2T1=12mpaT_2 - T_1 = \frac{1}{2}m_p a (Eq. 3).

From Eq. 1 and Eq. 2: T2=m2(ga)T_2 = m_2(g - a) and T1=m1aT_1 = m_1 a. Substituting into Eq. 3: m2(ga)m1a=12mpam_2(g - a) - m_1 a = \frac{1}{2}m_p a. m2g=(m1+m2+12mp)am_2 g = (m_1 + m_2 + \frac{1}{2}m_p) a. a=m2gm1+m2+12mp=(2.0)(9.8)3.0+2.0+0.25=19.65.25=3.73a = \frac{m_2 g}{m_1 + m_2 + \frac{1}{2}m_p} = \frac{(2.0)(9.8)}{3.0 + 2.0 + 0.25} = \frac{19.6}{5.25} = 3.73 m/s2^2.

b) T1=m1a=(3.0)(3.73)=11.2T_1 = m_1 a = (3.0)(3.73) = 11.2 N. T2=m2(ga)=(2.0)(9.83.73)=(2.0)(6.07)=12.1T_2 = m_2(g - a) = (2.0)(9.8 - 3.73) = (2.0)(6.07) = 12.1 N.

Question 6

A solid sphere of mass MM and radius RR (I=25MR2I = \frac{2}{5}MR^2) rolls without slipping down an incline of angle θ\theta. Derive an expression for the linear acceleration of the sphere in terms of gg and θ\theta.

Answer 6

Linear motion (down the incline): Mgsinθf=MaMg\sin\theta - f = Ma (Eq. 1). Rotational motion: fR=Iα=(25MR2)(a/R)=25MRafR = I\alpha = (\frac{2}{5}MR^2)(a/R) = \frac{2}{5}MRa (Eq. 2). From Eq. 2: f=25Maf = \frac{2}{5}Ma. Substitute into Eq. 1: Mgsinθ25Ma=MaMg\sin\theta - \frac{2}{5}Ma = Ma. Mgsinθ=75MaMg\sin\theta = \frac{7}{5}Ma. a=57gsinθa = \frac{5}{7}g\sin\theta.