Periodic Motion & Basics of SHM
In SHM a body moves to and fro about a mean position, under a restoring force that is proportional to the displacement.
16.1.1 Periodic and oscillatory motion
- Periodic: repeats after a fixed interval. Example: the earth around the sun.
- Oscillatory: to and fro about a fixed point, within limits on both sides.
- Every oscillatory motion is periodic. Not every periodic motion is oscillatory.
- Examples: wall clock pendulum, load on a spring, liquid in a U-tube, loaded wood floating on a liquid.
16.1.2 Harmonic and non-harmonic
- Harmonic: a single sine or cosine, y = a sin ωt or y = a cos ωt.
- Non-harmonic: a mix of harmonic functions, such as y = a sin ωt + b sin 2ωt.
- sin ωt + cos ωt is still harmonic: both terms have the same ω.
- e−ωt and log ωt are not periodic.
- A ball bouncing elastically is periodic but not SHM.
16.1.3 Condition for SHM
- k = force constant, unit N/m, dimension [MT⁻²].
- Minus sign: F is opposite to the displacement.
- Angular SHM: restoring torque τ = −cθ.
16.1.4 Reading ω directly
- Any equation in this form is SHM.
- Read ω² from the coefficient of y.
- Then T = 2πω
16.1.5 T, n and ω
| Quantity | Meaning | Unit |
|---|---|---|
| time period T | least time after which motion repeats | s |
| frequency n | oscillations per second | Hz |
| angular frequency ω | ω = 2πn | rad/s |
16.1.6 Where the particle is, and which way it is going
- (ωt + φ₀) is the phase at time t.
- φ₀ is the initial phase, or epoch.
- One full oscillation changes the phase by 2π.
- Phase change in time Δt: Δφ = 2πT Δt.
| Phase difference | Time difference | |
|---|---|---|
| same phase | 0, 2π, 4π … | 0, T, 2T … |
| opposite phase | π, 3π, 5π … | T2, 3T2 … |
- Same phase: the particles cross the mean position together, in the same direction.
- Opposite phase: they cross it together, in opposite directions.
- First write both equations with the same function: cos ωt = sin(ωt + π2).
- Two SHMs of the same a and ω: maximum separation = 2a sin(φ2).
Equation of SHM, Time & Distance
SHM is the projection of uniform circular motion on a diameter. This gives its equation and all its timing results.
16.2.1 SHM from circular motion
- P moves on a circle of radius a with angular speed ω.
- The foot N of the perpendicular on a diameter performs SHM.
- a = amplitude, ω = angular frequency of the SHM.
- Displacement is always measured from the mean position.
16.2.2 Choosing the right equation
| Time noted from | Equation |
|---|---|
| mean position | y = a sin ωt |
| extreme position | y = a cos ωt |
| phase φ ahead | y = a sin(ωt + φ) |
16.2.3 Use the sign of the velocity
- Put t = 0 in y = a sin(ωt + φ) to get sin φ.
- Moving along +y: cos φ is positive.
- Moving along −y: cos φ is negative.
| Start at | Moving | φ |
|---|---|---|
| a2 | +y | π6 |
| a2 | −y | 5π6 |
| a | at rest | π2 |
16.2.4 Given y and v at one instant
16.2.5 One SHM in disguise
- The resultant is an SHM of the same ω.
- A constant term, y = A₀ + a sin ωt, only shifts the mean position.
- The amplitude does not change with such a constant.
16.2.6 Between two positions
| From | To | Time |
|---|---|---|
| mean | A2 | T12 |
| A2 | extreme | T6 |
| mean | A√2 | T8 |
| mean | extreme | T4 |
| −A | +A | T2 |
- Motion is fastest near the mean position.
- So mean → A2 takes less time than A2 → extreme.
- General: from the mean position t = T2π sin⁻¹(yA).
16.2.7 Starting from the mean position
| Time | Distance | Displacement |
|---|---|---|
| T4 | A | A |
| T2 | 2A | 0 |
| T | 4A | 0 |
- Path length = 2A.
- Average velocity over a full cycle = 0.
- Distance in the nth second: use y = A sin ωt at both ends of that second.
- Over a full cycle average speed = 4AT = 2Aωπ
Velocity & Acceleration in SHM
Velocity is largest at the mean position. Acceleration is largest at the extremes and always points to the mean position.
16.3.1 From the displacement equation
- Mean position (y = 0): vmax = aω.
- Extreme position (y = ±a): v = 0.
- Velocity at y: use the second form directly.
16.3.2 An ellipse
- For ω = 1 the ellipse becomes a circle.
- A momentum–displacement graph is also an ellipse.
16.3.3 Always towards the mean position
- Mean position: A = 0.
- Extreme position: |Amax| = ω²a.
- A is not constant, so equations of uniform acceleration do not apply.
- A is always opposite to the displacement.
16.3.4 At the two key positions
| Quantity | Formula | Mean | Extreme |
|---|---|---|---|
| displacement | a sin ωt | 0 | ±a |
| velocity | ω√(a² − y²) | aω | 0 |
| acceleration | −ω²y | 0 | ω²a |
| force | −ky | 0 | ka |
16.3.5 Phase relations
- All have the same period T.
- v leads y by π2
- A leads v by π2
- A leads y by π. F and A are in phase.
- Velocity amplitude = ω × displacement amplitude.
- Acceleration amplitude = ω² × displacement amplitude.
16.3.6 Quick links
- Path length = 2a = 2vmax²Amax
- vmax ∝ aT. Doubling a and making T one-third gives 6 times.
- |v| = |A| at y when √(a² − y²) = ωy.
16.3.7 Given v at two displacements
- Distance between positions = v₁² − v₂²A₁ + A₂, where A₁ and A₂ are the accelerations there.
16.3.8 Vertical SHM of a platform
- A block leaves the platform at the top when the downward acceleration reaches g.
- Largest amplitude for contact: A = gω²
- Least period for contact: T = 2π√(Ag).
Energy in SHM
Energy keeps changing between kinetic and potential, but the total stays constant and depends on a².
16.4.1 Stored against the restoring force
- U is minimum (zero) at the mean position.
- U is maximum at the extremes, equal to the total energy.
16.4.2 From the velocity
- K is maximum at the mean position, equal to the total energy.
- K is zero at the extremes.
16.4.3 Same at every point
- E does not depend on y or t.
- E ∝ a² and E ∝ n², for a given mass.
- Doubling a and halving n leaves E unchanged.
- E does not vary periodically; y, v, A, U and K all do.
16.4.4 U and K against displacement
16.4.5 Asked again and again
| y | U | K |
|---|---|---|
| 0 | 0 | E |
| a2 | E4 | 3E4 |
| a√2 | E2 | E2 |
| √3a2 | 3E4 | E4 |
| a | E | 0 |
16.4.6 Fast method
- U = nK gives y = a√(nn + 1).
- E = nK gives y² = a²(n − 1n).
- Since √U ∝ y: at y = y₁ + y₂, √U = √U₁ + √U₂.
- Force and energy: U = F²2k, or U = ½Fy.
16.4.7 Starting from the mean position
| t | ωt | K : U |
|---|---|---|
| T12 | π6 | 3 : 1 |
| T8 | π4 | 1 : 1 |
| T6 | π3 | 1 : 3 |
| T4 | π2 | 0 : 1 |
- From an extreme position the two columns swap, so K : U = tan²ωt.
- K = 75% of E at T12. K = 50% of E at T8
- U and K change with double the frequency of the motion.
Corner
- If the SHM has frequency n, then U and K vary with frequency 2n.
- Their period is T2
- K − U = E cos 2ωt also has frequency 2n.
- Total energy E does not vary at all.
- Averages are taken over one complete cycle.
- K = 0 and U = 0 never happen together.
Simple Pendulum
For small angles the pendulum performs SHM, and its period depends only on length and g.
16.5.1 Small angle needed
- Ideal pendulum: point mass on a weightless, inextensible string.
- mg cos θ balances the tension (with the centripetal part).
- mg sin θ is the restoring force.
16.5.2 What T does not depend on
- T does not depend on amplitude, while the motion is SHM.
- For a larger angle θ₀, T is slightly more: T = T₀(1 + θ₀²16).
- T does not depend on the mass of the bob.
- Hollow or solid bob of the same size: same T.
- A second child joining on a swing: same T.
16.5.3 Measured to the centre of mass
- l runs from the support to the centre of mass of the bob.
- T ∝ √l: making l four times doubles T.
- A child stands up on a swing: centre of mass rises, l falls, T falls.
- A clock running slow: reduce l. A clock running fast: increase l.
- Thread on two supports: use the vertical distance from the support line to the bob.
16.5.4 Sand or water flowing out
- Hollow bob full of water, hole at the bottom.
- As it empties, the centre of mass first falls: l and T increase.
- Near the end the centre of mass comes back to the centre: l and T decrease.
- So T first increases and then decreases.
- Empty and full bobs have the same T.
16.5.5 Using T² ∝ l
- n oscillations in the same time: l₁l₂ = (n₂n₁)².
- T increases by 20% ⇒ l becomes (1.2)² = 1.44 times.
16.5.6 Least common time
- Find the smallest time that holds a whole number of both periods.
- T₁ and 43T₁: in phase again after 4T₁.
- Lengths 121 cm and 100 cm: 10 swings of the long = 11 of the short.
16.5.7 Height and speed
- For a given A, E ∝ 1l. Making l one-third makes E three times.
- U at the extreme = mgA²2l
- Maximum speed: vmax = Aω = A√(gl).
- Work done by the bob in one complete oscillation is zero, with no resistance.
16.5.8 Largest at the mean position
Pendulum in Different Situations
Replace g by the effective g of the situation, and use the same formula.
16.6.1 One formula
- T ∝ 1√geff
- Find geff as the acceleration of the bob relative to its support, when the string is cut.
16.6.2 Support accelerating vertically
| Lift | geff | T |
|---|---|---|
| no a | g | unchanged |
| a upward | g + a | decreases |
| a downward | g − a | increases |
| free fall | 0 | no oscillation |
- T₁: at rest. T₂: going up with a. T₃: going down with a.
- Lift up at g4: geff = 5g4
- Lift down at g4: geff = 3g4
- Period halved ⇒ geff = 4g ⇒ a = 3g.
- If support follows y = kt², then a = 2k.
- A satellite or the centre of the earth: geff = 0, so no oscillation.
16.6.3 Support accelerating horizontally
- T = 2π√(l√(g² + a²)).
- Car on a circular track: a = v²r
- Free slide down an incline of angle α: geff = g cos α.
- The new mean position is the tilted one.
16.6.4 Buoyancy reduces g
- ρ = density of the bob, σ = density of the liquid.
- T increases inside a liquid.
- σ = ρ4: T′ = 2√3T.
- Liquid assumed non-viscous.
Corner
- g falls on going up or down inside the earth, so T increases.
- A pendulum clock on a hill runs slow.
- At height h = R: g′ = g4, so T′ = 2T.
- On a planet: g′ = g(M′M)(RR′)².
- l changes by n%: T changes by +n2%.
- g changes by n%: T changes by −n2%.
- Valid for small changes only (up to about 5%).
- T = 2 s; extreme to extreme takes 1 s.
- l = 99.3 cm (nearly 1 m) on the earth.
- On the moon: l = 16 m nearly.
- l ≪ R: T = 2π√(lg).
- l = R: T = 2π√(R2g) ≈ 1 hour.
- l → ∞: T = 2π√(Rg) = 84.6 minutes, the largest possible T.
Spring Constant & Spring-Mass System
A mass on a spring performs SHM of period 2π√(m ÷ k), which does not depend on g.
16.7.1 Hooke’s law
- k measures stiffness. Unit N/m, dimension [MT⁻²].
- Massless spring: the tension is the same everywhere.
- Stored energy U = ½kx².
16.7.2 k × length = constant
- Half the length: double the k.
- n equal parts: each has constant nk.
- Each part then has period T√n
- Ratio l₁ : l₂ = n : 1 gives k₂ = k(n + 1) and k₁ = k(n + 1n).
16.7.3 Spring-mass system
- T ∝ √m and T ∝ 1√k
- Same period on a hill, on the moon, in a satellite, or in a liquid (without damping).
- Same period whether horizontal, vertical or on an incline.
- Mass suspended m to 4m: T doubles.
16.7.4 Using T² ∝ m
- Period doubled: m + Δm = 4m.
- T² adds with mass: T = √(T₁² + T₂²) for m₁ + m₂ on the same spring.
- Massive spring of mass M: use m + M3 as the effective mass.
16.7.5 Static extension gives the period
- Equilibrium in a vertical spring is at extension y₀; in a horizontal one, at natural length.
- T does not depend on g: y₀ changes with g so that y₀g stays constant.
- Spring from which m is removed shortens by y₀ = mgk
- Extra mass Δm gives extra stretch x: k = Δm gx
16.7.6 A common twist
- If the spring is unstretched at the highest point, then A = y₀.
- A = gω²
16.7.7 Compare using ω
| Same | Result |
|---|---|
| maximum velocity | A₁A₂ = √(k₂k₁) |
| amplitude | v₁v₂ = √(k₁k₂) |
| maximum energy | A₁A₂ = √(k₂k₁) |
- Different masses: use vmax = A√(km).
Spring Combinations & Added Mass
Series springs share the force; parallel springs share the extension. Find keq, then use T = 2π√(m ÷ keq).
16.8.1 Same force, extensions add
- n identical springs: keq = kn
- keq is less than the smallest k.
- k, 2k, 4k, 8k, … in series: keq = k2
16.8.2 Same extension, forces add
- n identical springs: keq = nk.
- keq is more than the largest k.
- The same law holds when two forces act together on a body: T₁ for one, T₂ for the other.
16.8.3 This is parallel
- Both springs pull the mass the same way, so it is a parallel case.
- Removing one of two identical springs: k halves.
- Frequency then falls by a factor of √2.
- Springs inclined to the motion: use components, or the given figure’s symmetry.
16.8.4 A sure method
- Reduce side by side: first the springs that end on one mass together.
- Same extension? Add k. Same force? Add 1k
- For a disc on two springs, or a block held by several: same extension, so parallel.
- A spring of constant k cut as 1 : 2 : 3 gives 6k, 3k, 2k. Series gives back k; parallel gives 11k.
| Identical springs k | keq | T |
|---|---|---|
| one | k | T₀ |
| two in series | k2 | √2 T₀ |
| two in parallel | 2k | T₀√2 |
| n parts in parallel | n²k | T₀n |
16.8.5 Momentum is conserved
- Mass m is placed gently on M as it crosses the mean position.
- Speed drops, so the energy falls.
- ω′ = ω√(MM + m).
16.8.6 Amplitude unchanged
- At the extreme the speed is zero, so nothing changes in the energy.
- A stays the same; only the period changes.
16.8.7 At the mean position
- The remaining part keeps the same speed.
- If half the mass is lost, ω′ = √2 ω and A′ = A√2
16.8.8 Reduced mass
Other SHM Systems
Find the restoring force, read off k and m, then use T = 2π√(m ÷ k), with the right inertia and spring factors.
16.9.1 Four steps
- Locate the equilibrium position.
- Displace slightly by y and find the net restoring force.
- Write it as F = −ky.
- Then T = 2π√(mk).
16.9.2 Buoyancy is the spring
- l = depth under the liquid at rest. A = area of cross-section.
- l = ρσ × height of the body.
- Same as a pendulum of length l.
- T ∝ 1√σ for a given body.
16.9.3 Weight of the extra column
- L = total length of the liquid column (L = 2h).
- h = height of the undisturbed liquid in each limb.
- If mass M of density d is poured into a tube of area A: L = MAd
16.9.4 Like a pendulum
- Small sphere in a watch glass (r ≪ R): T = 2π√(Rg).
- Rolling with friction adds a factor: T = 2π√(7(R − r)5g).
16.9.5 Gas as a spring
- Adiabatic: use γP in place of P.
- In terms of volume V₀ = Ah: n = 12π√(γP₀A²MV₀).
16.9.6 Along any chord
- T is the same along any chord.
- Same as the period of a satellite just above the earth.
16.9.7 Longitudinal oscillations
- Y = Young’s modulus, A = area of cross-section.
- Pendulum wire with added mass M: (TMT)² − 1 = MgAY
Corner
- l = distance of the centre of mass from the pivot.
- I = IG + ml² by the parallel axis theorem.
- k = radius of gyration about the centre of mass.
| Body | T |
|---|---|
| bar, length l | 2π√(2l3g) |
| ring, radius R | 2π√(2Rg) |
| disc, radius R | 2π√(3R2g) |
- I = moment of inertia of the disc.
- C = torsional constant of the wire.
- η = modulus of rigidity, r = radius of the wire.
Damped & Forced Oscillations, Superposition
In real life, damping makes the amplitude fall exponentially. An outside force can keep the oscillation going.
16.10.1 Natural frequency
- Only the restoring force acts.
- Amplitude, frequency and energy stay constant.
- The natural frequency depends on the body itself.
16.10.2 Amplitude dies out
- b = damping constant. Unit kgs, or N s/m.
- Damping comes from friction and viscosity.
- Damped frequency is slightly less than the natural one.
- Energy falls twice as fast as amplitude.
16.10.3 Quick method
- In equal time intervals, A falls by the same factor.
- A → A3 in 2 s means A → A27 in 6 s.
- A → A3 in 100 oscillations means A → A9 in 200.
- A → 0.9A in 5 s means A → (0.9)³A in 15 s.
- Half-life of amplitude: t = 2m ln 2b
Corner
- A periodic external force F₀ cos ωdt keeps the body oscillating.
- After a while the body oscillates at the frequency of the driver.
- Resonance: the driving frequency equals the natural frequency.
- Amplitude becomes large but stays finite, because of damping.
- Power absorbed is largest at resonance.
- Sharpness of resonance depends on the damping.
- At resonance the velocity is in phase with the driving force.
- Energy lost in each cycle is supplied from outside.
- Amplitude stays constant, as in a clock.
- The resultant is an SHM of the same frequency.
- φ = 0: A = a₁ + a₂. φ = π: A = |a₁ − a₂|.
| φ | Path |
|---|---|
| 0 | straight line, slope a₂a₁ |
| π4 | oblique ellipse |
| π2 | circle if a₁ = a₂, else ellipse |
| π | straight line, slope −a₂a₁ |
Just see this before the exam
Whole chapter on one page
a = −ω²y, ω = 2πT
y = a sin(ωt + φ)
a sin + b cos: A = √(a² + b²)
mean → A2: T12; A2 → A: T6
v = ω√(a² − y²)
vmax = aω, Amax = ω²a
ω = Amaxvmax
contact lost: ω²A = g
E = ½mω²a² = ½ka²
U = ½ky²
K = ½k(a² − y²)
K = U at y = a√2
T = 2π√(lgeff)
lift: g ± a; car: √(g² + a²)
liquid: g(1 − σρ)
Tmax = mg[1 + (Al)²]
T = 2π√(mk), k ∝ 1l
series: 1k = 1k₁ + 1k₂
parallel: k = k₁ + k₂
added at mean: AA′ = √(M + mM)
floating: T = 2π√(lg)
U-tube: T = 2π√(hg)
bowl: T = 2π√(R − rg)
damped: A = A₀e−bt ÷ 2m
Avoid these = easy marks
Using v = u + at in SHM
K = U at y = a2
Period of a spring depends on g
Mass between two springs taken as series
A is not constant: use v = ω√(a² − y²)
K = U at y = a√2
T = 2π√(mk): no g
Both pull the same way: parallel, k₁ + k₂