Unit M3: Mechanics 3
- Syllabus
- 2019
- Section
- —
- Level
- A2

For motion along a straight line, displacement x, signed velocity v and signed acceleration a are linked by derivatives. Choose the form whose independent variable matches the information given; this avoids introducing an unnecessary unknown function.
v=dtdx,a=dtdv=vdxdv
| Information given | Equation to set up | First result after integration |
|---|---|---|
| a=f(t) | dtdv=f(t) | v as a function of t |
| a=f(x) | vdxdv=f(x) | 21v2 as a function of x |
| v=f(x) | dtdx=f(x), so dt=f(x)dx | t as a function of x |
| v=f(t) | dtdx=f(t) | x as a function of t |
The displacement form of acceleration follows from the chain rule:dtdv=dxdvdtdx=vdxdv.Use it when acceleration or velocity is expressed in terms of x. If the required quantity is time and v=f(x), separate variables instead: dt=dx/v(x).
Every indefinite integration needs a constant. Apply a stated condition such as x=x0 and v=v0 at t=t0 only after integrating, or use definite integrals with those values as limits. Keep v signed: a negative velocity represents motion in the negative x-direction, while speed is ∣v∣.
Suppose v=12/(x+2) metres per second and x=1 when t=0. First,a=vdxdv=x+212(−(x+2)212)=−(x+2)3144.At x=4, a=−2/3ms−2. For the elapsed time to reach x=4,t=∫14vdx=∫1412x+2dx=[24x2+6x]14=89 s.The negative acceleration means velocity is decreasing here; the deceleration magnitude is 2/3ms−2.
Check that the final variable matches the question, substitute the initial condition back into the integrated relation, and verify units: v has units ms−1 and a has units ms−2. If a derivation divides by v or by another expression that can be zero, solve on intervals where that division is valid and inspect the zero case separately.
Do not use constant-acceleration formulae when a varies, replace a by dv/dx without the factor v, discard an integration constant, or report a negative acceleration automatically as a positive deceleration. Acceleration and velocity signs must be interpreted together.
An elastic element has natural length l, the length at which it is undeformed. If its current length is L, its extension is x=L−l. Under Hooke's law, the elastic-force magnitude is proportional to this extension.
T=lλx
Here T is tension in newtons and λ is the modulus of elasticity, also measured in newtons. The ratio x/l is dimensionless. When a spring is described using stiffness k instead, the equivalent form is T=kx, with k=λ/l and unit Nm−1.
| Model | When the elastic force acts | Direction |
|---|---|---|
| light elastic string | only while stretched, L>l | tension pulls each attached object along the string |
| string at or below natural length | it is slack, so T=0 | no push is possible |
| elastic spring | when stretched or compressed within the Hooke-law model | restoring force points towards natural length |
First calculate extension from the actual geometry, not from the total length alone. Apply Hooke's law to find tension, then place that force on the free-body diagram and resolve it in the chosen direction. If two equal sections pull symmetrically, include both resolved tensions; do not replace them by one tension.
A particle of mass 1.5 kg hangs from a vertical light elastic string with natural length 0.8 m and modulus 40 N. At an instant the string has length 1.1 m, so x=0.3 m andT=0.840(0.3)=15 N.Taking upward as positive, the particle's acceleration at that instant isa=mT−mg=1.515−1.5(9.8)=0.20ms−2.Hooke's law supplies the force; Newton's second law supplies the acceleration.
Do not substitute the current length for the extension, treat the modulus as a spring constant with unit Nm−1, or let an elastic string push when slack. Hooke's law describes the stated ideal elastic model; geometry and force resolution remain separate steps.
Stretching an elastic string or deforming a spring stores elastic potential energy (EPE). For a Hooke-law element, the force rises linearly from zero, so the stored energy is the area under the force-extension relation.
Ee=2lλx2=21Tx=21kx2
Use the extension x=L−l at the particular state being considered. For an elastic string, Ee=0 whenever the string is slack; for a spring, x2 gives positive stored energy for either extension or compression. Elastic energy is measured in joules.
| Energy term | Expression | What changes it |
|---|---|---|
| kinetic energy | 21mv2 | the particle's speed |
| gravitational potential energy | mgh | vertical height relative to one fixed datum |
| elastic potential energy | λx2/(2l) | the element's extension or compression |
| external work | force component × displacement, or an integral | a non-conservative applied force |
Choose initial and final states, calculate the elastic extension separately at each state, and use one consistent height datum. If only gravity and ideal elastic forces do work,Ki+Ug,i+Ee,i=Kf+Ug,f+Ee,f.Otherwise add the work of any other force with its correct sign. Energy equations compare states; they do not require the acceleration to be constant.
A 1 kg particle is attached below a vertical elastic string of natural length 1 m and modulus 20 N. It is released from rest with extension 0.10 m and falls 0.20 m, so the final extension is 0.30 m. The initial and final EPE values are 0.10 J and 0.90 J. Conservation of mechanical energy gives0+0.10+1(9.8)(0.20)=21v2+0.90,hence 21v2=1.16 and v=1.52ms−1 to three significant figures.
Do not use the same extension at both endpoints, omit elastic energy when the element remains stretched, or write EPE as Tx: because tension changes during deformation, the factor 1/2 is essential. When a string becomes slack, stop using the stretched-string formula beyond that event.
For motion along one signed axis, first write the resultant force with its direction, then choose the acceleration form that matches the variable in the force law. A varying force produces a differential equation rather than a constant-acceleration problem.
Fresultant=ma,a=dtdv=vdxdv
| Force information | Useful equation | Typical result |
|---|---|---|
| F=f(t) | mdv/dt=f(t) | integrate for v(t), then for x(t) if needed |
| F=f(x) | mvdv/dx=f(x) | integrate for v2 as a function of x |
| work is simpler | ∫x0xF(s)ds=21m(v2−v02) | compare two positions directly |
| inverse-square attraction | choose outward positive, so F=−k/x2 | preserve the negative force sign before integrating |
Define the coordinate origin and positive direction before inserting a force. Include every force component in the resultant. Separate variables or integrate with limits, use the supplied motion condition to determine the constant, and accept only positions for which v2≥0 and the force model is defined.
A 2 kg particle moves in the positive x-direction under resultant force F=12−2x N. At x=0, its speed is 1ms−1. Since2vdxdv=12−2x,integration between the initial position and x givesv2=1+12x−x2.At x=3 m, v=28=27ms−1. A turning point requires v=0; the positive solution is x=6+37 m.
For an attractive inverse-square force with outward coordinate x>0, F=−k/x2. Thenmvdxdv=−x2kintegrates to 21mv2=k/x+C. The plus sign on k/x after integration is consistent with differentiating k/x to recover −k/x2.
Do not use constant-acceleration formulae, omit a force from the resultant, drop the factor v in a=vdv/dx, or remove the sign from an attractive inverse-square force. A negative value of v2 signals an inaccessible region, not an imaginary physical speed.
Motion is simple harmonic when acceleration is proportional to displacement from a fixed equilibrium point and always directed back towards that point. With signed displacement x from equilibrium, the defining equation is
x¨=−ω2x
To prove SHM in a mechanical system, write a signed equation of motion and simplify it in terms of displacement from equilibrium. Constant force terms must cancel at equilibrium. Reaching x¨=−cx with c>0 proves SHM and identifies ω=c; merely obtaining a periodic-looking expression is not the required force-law proof.
| Quantity | SHM relation |
|---|---|
| displacement | x=Acos(ωt+ϕ), equivalently a sine form |
| speed at displacement x | v2=ω2(A2−x2) |
| period | T=2π/ω |
| maximum speed, at equilibrium | vmax=ωA |
| maximum acceleration, at an endpoint | ∣a∣max=ω2A |
Choose the phase from the initial state. Release from rest at x=A allows x=Acosωt; starting at equilibrium in the positive direction allows x=Asinωt. For time spent in a region, solve the boundary displacement within one cycle and use the symmetry of the cosine or sine curve without double-counting endpoints.
If x=0.12cos(5t) metres, then A=0.12 m, ω=5rads−1 and T=2π/5 s. The maximum speed is 0.60ms−1. Starting at the positive endpoint, the first time the particle reaches x=0.06 m satisfies cos(5t)=1/2, so t=π/15 s.
Displacement must be measured from equilibrium, not an arbitrary origin. The minus sign is essential: x¨=+ω2x drives motion away from equilibrium and is not SHM. Amplitude is a non-negative distance, whereas x, v and acceleration are signed.
A particle attached to an ideal spring or taut elastic string can perform SHM along the element's direction. Measure displacement from the equilibrium position: doing so makes the constant weight term cancel and exposes the restoring force.
mx¨=−kx,ω=mk,k=lλ
For a vertical element, let its equilibrium extension be e. Equilibrium gives ke=mg. If downward displacement from equilibrium is x, the extension is e+x andmx¨=mg−k(e+x)=−kx.Gravity shifts the equilibrium position but does not appear in ω after this cancellation.
| Arrangement | Condition for the SHM model to remain valid |
|---|---|
| spring | deformation stays within the stated Hooke-law model |
| one elastic string | its extension never becomes negative; for equilibrium extension e and amplitude A, require e−A≥0 |
| particle between two elastic strings | calculate both extensions at each extreme and require both strings to remain taut |
| string reaches natural length | tension becomes zero; subsequent motion is not governed by the same SHM equation |
A 0.5 kg particle oscillates vertically on an elastic element with stiffness 18Nm−1. Then ω=18/0.5=6rads−1 and T=π/3 s. If its amplitude is 0.08 m, its speed at displacement 0.04 m isv=60.082−0.042=0.416ms−1.If the element is a string, this calculation applies for the whole oscillation only after checking that the minimum extension remains non-negative.
Do not measure elastic extension and SHM displacement from the same origin without defining both, leave the equilibrium weight term in the final restoring equation, or claim one continuous SHM cycle after a string goes slack. The specified oscillation is along the string or spring, not transverse to it.
Angular speed ω measures the rate at which angular position changes. Angles in circular-motion formulae are measured in radians, so one complete revolution is 2π radians.
ω=dtdθ,ω=T2π=2πf
For a point at radius r, arc length is s=rθ. Differentiating gives tangential speed v=rω. All points on one rigid rotating body have the same angular speed, but a point farther from the axis has a larger linear speed.
| Quantity | Meaning | Unit |
|---|---|---|
| θ | angular displacement | radians |
| ω | angular speed | rads−1 |
| T | time for one revolution | seconds |
| f | revolutions per second | hertz, s−1 |
| v | distance travelled per second along the circle | ms−1 |
A wheel completes 15 revolutions in 6 minutes. Its period is 360/15=24 s andω=242π=12πrads−1.A point 8 m from the axis therefore moves at v=8(π/12)=2π/3ms−1.
Do not insert degrees into s=rθ or v=rω, confuse revolutions per minute with radians per second, or assume equal angular speed means equal tangential speed at different radii.
A particle moving in a circle accelerates even when its speed is constant, because its velocity direction changes. The acceleration points radially inward, towards the centre of the circle.
ar=rv2=rω2
The inward acceleration is not an extra force. Choose inward as the positive radial direction and resolve the actual forces:∑Finward=mrv2=mrω2.Forces pointing away from the centre enter with a negative sign.
| Component | Direction | What changes it describes |
|---|---|---|
| radial acceleration | towards the centre | direction of velocity |
| tangential acceleration | along or opposite the motion | magnitude of speed |
| uniform circular motion | radial component present, tangential component zero | constant speed but changing velocity |
A 0.40 kg particle moves at 3.0ms−1 in a circle of radius 1.5 m. Thenar=1.53.02=6.0ms−2,so the resultant inward force must be 0.40(6.0)=2.4 N. Individual forces need not each equal 2.4 N; their inward components must have that resultant.
Do not draw radial acceleration tangentially, call mv2/r a separate 'centripetal force', or write a radial force balance without defining which direction is inward. The speed may be constant while velocity and acceleration are not zero.
For uniform motion in a horizontal circle, vertical acceleration is zero while the horizontal resultant towards the centre is mrω2. Draw every real force, resolve vertically for equilibrium, and resolve horizontally inwards for circular motion.
∑Fvertical=0,∑Finward=mrω2
| Context | Forces and modelling decision |
|---|---|
| conical pendulum | tension has vertical and inward components; r=lsinθ if θ is from the vertical |
| smooth banked surface | normal reaction supplies vertical and inward components |
| rough banked surface | friction acts along the surface; choose its direction from the tendency to slip and use ∣F∣≤μR |
| elastic string | calculate extension and tension with Hooke's law before resolving |
| contact with a floor | require normal reaction R≥0; at loss of contact, R=0 |
Mark the circle's horizontal radius before resolving. Geometry determines r and the angles of strings or reactions. Use limiting friction only when the speed is at a limiting value; otherwise the friction magnitude is an unknown no greater than μR. Check that every tension and reaction is non-negative.
A 0.50 kg particle is a conical pendulum on a string of length 1.2 m at 30∘ to the vertical. Its circle has radius r=1.2sin30∘=0.60 m. FromTcos30∘=mg,Tsin30∘=mrω2,division gives tan30∘=rω2/g. Hence ω=3.07rads−1 and T=mg/cos30∘=5.66 N using g=9.8ms−2.
Do not put mrω2 into the vertical balance, use the sloping string length as the circle radius, assume friction has magnitude μR away from limiting motion, or ignore the non-negative contact/tension conditions that restrict possible angular speeds.
In a vertical circle, speed changes with height while the required inward resultant remains mv2/r. Use conservation of energy to find speed at a position, then use a separate radial equation to find tension or reaction.
Let θ be measured from the lowest point and let the bottom speed be u. The height above the bottom is r(1−cosθ). With no non-conservative work,v2=u2−2gr(1−cosθ).For a particle on a taut string, resolving inward gives
T−mgcosθ=rmv2
| Position | θ | Radial equation for a string |
|---|---|---|
| bottom | 0 | T−mg=mv2/r |
| side | π/2 | T=mv2/r |
| top | π | T+mg=mv2/r |
A string must satisfy T≥0; a smooth contact must satisfy reaction R≥0. At the first loss of constraint, set the relevant force to zero. For a string to complete a full vertical circle, the limiting top condition is vtop2=gr, which with energy gives the minimum bottom speed u=5gr. A rigid rod can push as well as pull, so it does not use the string-tension condition.
A particle on a string enters the bottom with u2=6gr. At the top, energy gives v2=6gr−4gr=2gr, soT+mg=2mg⇒T=mg>0.The string remains taut there. At the bottom, T−mg=6mg, so T=7mg; the larger bottom tension supplies both the inward acceleration and opposition to the downward weight.
Do not use one constant speed around a vertical circle, mix the energy equation with the radial force equation, reverse the inward weight component, or continue constrained circular motion after tension/reaction becomes negative. After a string goes slack, the particle follows unconstrained projectile motion until another interaction.
The centre of mass is the point at which the body's total mass may be treated as concentrated when calculating moments. For a uniform body, symmetry locates every coordinate that lies on an axis or plane of symmetry; integration is needed for a remaining coordinate when the shape varies.
xˉ=M1∫xdm,yˉ=M1∫ydm,M=∫dm
| Uniform body | Suitable mass element |
|---|---|
| thin rod or wire | dm=λds |
| lamina | dm=ρAdA |
| solid | dm=ρVdV |
| solid of revolution about the x-axis | dV=πy2dx |
Choose axes that exploit symmetry. Write both the total mass and its first moment using the same density model and limits, then divide first moment by total mass. For a simple composite body, treat each part as a point mass at its own centre of mass:xˉ=∑mi∑mixi,yˉ=∑mi∑miyi.A removed piece is entered with negative mass (or negative area or volume when density is common).
A uniform 6×4 rectangular lamina has a 2×2 square removed from its top-right corner. Taking the lower-left corner as the origin, use the full rectangle minus the hole:xˉ=24−424(3)−4(5)=2.6,yˉ=24−424(2)−4(3)=1.8.The centre shifts left and down, away from the removed mass, which checks the result.
Use mass, not geometric area or volume, unless uniform density makes them proportional. Keep every coordinate relative to one origin, use the perpendicular distance required by the chosen moment, and never assume that the centre of mass lies inside a hollow or concave body.
A rigid body is in equilibrium only when the resultant force is zero and the resultant moment about any point is zero. Its weight acts vertically through its centre of mass, so the position of that vertical line controls suspension and toppling.
∑F=0,∑MP=0
| Situation | Equilibrium condition |
|---|---|
| freely suspended from a fixed point | the centre of mass lies vertically below the suspension point in stable equilibrium, so the weight has zero moment about the point |
| body on a horizontal plane | the vertical through the centre of mass must meet the contact base; at limiting toppling it passes through an edge |
| body on an inclined plane | provided sliding is prevented, the same vertical line must meet the contact base; increasing inclination moves its intersection towards the downhill edge |
First find the centre of mass in body-fixed coordinates. For suspension, rotate the body until the line joining the suspension point to the centre of mass is vertical. For a supported body, identify the possible pivot edge and take moments about it. At the instant of toppling the reaction at the opposite side has fallen to zero and the resultant contact force acts through the pivot edge.
A uniform rectangular block has base length b measured up the line of greatest slope and its centre of mass is a perpendicular distance h above the plane. On a rough plane inclined at θ, the vertical through the centre of mass meets the plane htanθ downhill from the middle of the base. It is stable against toppling whilehtanθ<2b,and is on the point of toppling when htanθ=b/2. This test assumes the available friction prevents sliding first.
Do not align the centre of mass with the plane's normal: weight is vertical. Do not set friction equal to μR unless sliding is limiting, and do not assume toppling occurs before sliding; both conditions must be checked when the friction information is available.