A. Space, time and motion

Syllabus
First assessment 2025
Section
—
Level
HL

A.1 Kinematics

Syllabus
First assessment 2025
Topic
—
Level
HL

Describe Motion with Position, Velocity and Acceleration

Choose a reference

Position r⃗\vec r specifies where an object is relative to a chosen origin. A position is not meaningful without a reference frame and coordinate direction.

Track change in position

Velocity v⃗\vec v describes how position changes with time. It is a vector: its direction is the direction of motion at that instant, and on a curved path the velocity arrow is tangent to the path.

Track change in velocity

Acceleration a⃗\vec a describes how velocity changes with time. A change in speed, direction, or both is acceleration; an object can accelerate even while its instantaneous speed is zero.

Common trap

Do not use “velocity” as a synonym for speed. Speed gives only magnitude; velocity also requires direction relative to the chosen coordinate system.

A.1.1 Exam Analysis

[ 1 ]

the velocity of the ball at P . Label this arrow v.

Drawing canvas

Relate Velocity and Acceleration to Rates of Change

Velocity is a rate

Velocity is the rate of change of position:

v⃗=dr⃗dt\vec v=\frac{d\vec r}{dt}

Over a finite interval, average velocity is displacement divided by elapsed time.

Acceleration changes velocity

Acceleration is the rate of change of velocity:

a⃗=dv⃗dt\vec a=\frac{d\vec v}{dt}

A constant acceleration gives equal changes in velocity during equal time intervals.

Read the gradient

On a position–time graph, the gradient represents velocity. On a velocity–time graph, the gradient represents acceleration. The graph’s slope, not its height alone, carries the rate-of-change meaning.

Common trap

Distance divided by time gives average speed, not instantaneous velocity. Likewise, a large velocity does not imply a large acceleration unless the velocity is changing rapidly.

A.1.2 Exam Analysis

[ 1 ]

Instantaneous velocity is defined as...

Define Displacement as Change in Position

Displacement is a vector

Displacement is the change in position:

Δr⃗=r⃗final−r⃗initial\Delta\vec r=\vec r_{final}-\vec r_{initial}

It has a magnitude and a direction from the initial position to the final position.

Ignore the route for displacement

The path taken between the two positions does not determine displacement. A curved or complicated journey can still have a straight-line displacement between its endpoints.

Use components when needed

For perpendicular changes, resolve displacement into components and combine them vectorially. A signed one-dimensional displacement is positive or negative according to the chosen axis.

Common trap

A return to the starting point gives zero displacement even though the distance travelled is non-zero.

A.1.3 Exam Analysis

[ 1 ]

A stone is kicked horizontally at a speed of 1.5 ms−11.5 \mathrm{~ms}^{-1} from the edge of a cliff on one of Jupiter's moons. It hits the ground 2.0 s later. The height of the cliff is 4.0 m .
Air resistance is negligible.
What is the magnitude of the displacement of the stone?

Distinguish Distance and Displacement

Distance

Distance is the total path length travelled. It is a scalar, so it has magnitude only and cannot be negative.

Displacement

Displacement is the vector change in position from start to finish. Its magnitude is the shortest endpoint-to-endpoint separation, not generally the length of the route.

Match the average quantity

Average speed uses total distance divided by total time. Average velocity uses displacement divided by total time. A route with turns can therefore have average speed greater than the magnitude of average velocity.

Common trap

For a complete oscillation, the displacement is zero but the distance is four times the amplitude. Choose the quantity named in the question before substituting.

A.1.4 Exam Analysis

[ 1 ]

A person walks 40 m due west and then 30 m due north. The total walking time is 100 s . What are the average speed and the magnitude of the average velocity of the person?

Average speed/m s −1{ }^{-1}

Magnitude of average
velocity /ms−1/ \mathrm{m} \mathrm{s}^{-1}

0.5

0.5

0.5

0.7

0.7

0.5

0.7

0.7

Distinguish Instantaneous and Average Motion

Average values use an interval

Average speed is total distance divided by total time. Average velocity is displacement divided by elapsed time. Average acceleration is change in velocity divided by elapsed time.

Instantaneous values use one moment

Instantaneous velocity is the tangent gradient on a position–time graph; instantaneous speed is its magnitude and is what an ideal speedometer reports. Instantaneous acceleration is the tangent gradient on a velocity–time graph. Average values instead use a finite interval.

Connect graph quantities

The gradient of a velocity–time graph is acceleration, and the area under it is displacement. A constant acceleration therefore produces a straight-line velocity–time graph.

Common trap

Do not use the average gradient when a question asks for an instantaneous value. Use the tangent at the specified time.

A.1.5 Exam Analysis

[ 1 ]

The graph shows the variation of the acceleration a with time t of an object moving in a straight line.

Which graph shows the variation of the velocity v of the object with time t ?

Apply SUVAT Equations to Uniform Acceleration

Uniform-acceleration model

SUVAT equations apply when acceleration is constant along the chosen one-dimensional axis:

v=u+at,s=ut+12at2,v2=u2+2as,s=u+v2tv=u+at,\quad s=ut+\frac12at^2,\quad v^2=u^2+2as,\quad s=\frac{u+v}{2}t

Choose an equation

List the known and unknown quantities s,u,v,a,ts,u,v,a,t. Select an equation containing the required unknown and only known quantities; keep signs consistent with the positive direction.

Check the model

A constant acceleration means equal changes in velocity in equal time intervals. Use separate horizontal and vertical equations only when the motion has been resolved into independent components.

Worked example from local Question Bank row 22687

A glider accelerates uniformly from rest to 27.0 m s−127.0\,\mathrm{m\,s^{-1}} in 11.0 s11.0\,\mathrm{s}. Use s=u+v2ts=\frac{u+v}{2}t:

s=0+27.02×11.0=148.5 m≈149 ms=\frac{0+27.0}{2}\times 11.0=148.5\,\mathrm{m}\approx149\,\mathrm{m}

The result is the launch-run displacement; the constant-acceleration assumption is essential.

Common trap

Do not use SUVAT when acceleration varies significantly with time or position. A formula can produce a neat number while still violating the model’s constant-acceleration assumption.

A.1.6 Exam Analysis

[ 3 ]

Determine g using the photograph.

Recognize Uniform and Non-Uniform Acceleration

Uniform acceleration

Acceleration is uniform when the velocity changes by equal amounts in equal time intervals. The velocity–time graph is a straight line with constant gradient.

Non-uniform acceleration

Acceleration is non-uniform when its magnitude or direction changes. The velocity–time graph then has a changing gradient, and a single SUVAT value cannot describe the entire interval.

Model versus reality

A constant-acceleration model can be useful over a limited interval even when real forces vary. State the approximation and identify the neglected force or changing condition.

Common trap

A curved trajectory does not by itself prove that acceleration is non-uniform: projectile motion without drag has constant downward acceleration while its velocity direction changes.

A.1.7 Exam Analysis

[ 1 ]

State one reason why the acceleration of the spacecraft will not be constant.

Resolve Projectile Motion into Components

Separate the axes

With negligible fluid resistance, projectile motion is independent horizontal and vertical motion. Resolve the launch velocity:

ux=ucos⁡θ,uy=usin⁡θu_x=u\cos\theta,\qquad u_y=u\sin\theta

Horizontal motion

There is no horizontal acceleration in the ideal model, so vx=uxv_x=u_x and x=uxtx=u_xt. Use the horizontal displacement to find time or horizontal speed.

Vertical motion

Use one-dimensional constant-acceleration equations vertically, usually with ay=−ga_y=-g if upward is positive. The horizontal and vertical equations share the same time tt.

Worked example from local Question Bank row 31723

A tennis ball travels 11.9 m11.9\,\mathrm{m} horizontally after launch at 64.0 m s−164.0\,\mathrm{m\,s^{-1}} and 7∘7^\circ to the horizontal.

ux=64.0cos⁡7∘=63.52 m s−1u_x=64.0\cos7^\circ=63.52\,\mathrm{m\,s^{-1}}
t=xux=11.963.52=0.187 st=\frac{x}{u_x}=\frac{11.9}{63.52}=0.187\,\mathrm{s}

The same 0.187 s0.187\,\mathrm{s} must then be used in the vertical equation.

Common trap

Do not use the launch speed as the horizontal speed. Resolve it first, and do not use the horizontal time independently of the vertical motion.

A.1.8 Exam Analysis

[ 2 ]

The ball leaves the ground at an angle of 22∘22^{\circ}. The horizontal distance from the initial position of the edge of the ball to the wall is 11 m . Calculate the time taken for the ball to reach the wall.

Explain How Fluid Resistance Changes Projectile Motion

Drag opposes instantaneous velocity

Fluid resistance acts opposite the projectile's velocity and usually grows with speed. Its direction changes through the flight, so the resultant acceleration is not the constant downward gg of the ideal model.

Quantity Qualitative effect of fluid resistance
Trajectory No longer a symmetric parabola; descent is typically steeper
Horizontal velocity Decreases because drag has a component opposite horizontal motion
Vertical acceleration On ascent, downward drag makes downward acceleration greater than gg; on descent, upward drag makes it less than gg
Maximum height and range Both are reduced for the same launch conditions
Time of flight Ascent is shortened, while descent can be lengthened by upward drag; the total change is not universally one direction
Terminal speed During a long fall, increasing drag can balance weight so resultant force and acceleration become zero

Use the force direction

Before the peak, drag has horizontal and downward components; after the peak, it has horizontal and upward components. Therefore acceleration is not determined by velocity alone and changes continuously.

Terminal-speed condition

For vertical descent, terminal speed is reached when upward drag (and any buoyancy included in the model) balances weight. The object then continues at constant downward velocity.

Common trap

Zero acceleration at terminal speed does not mean zero velocity. At the top of a projectile path, vertical velocity may be zero while acceleration remains non-zero.

A.1.9 Exam Analysis

[ 1 ]

The diagram shows the path of a ball in the absence of air resistance. Q is the highest point of the ball's trajectory and a is the vertical acceleration at Q . At impact the velocity makes an angle θ\theta to the horizontal.

Three statements about the actual motion of the ball when there is air resistance are:

I. Q is lower.
II. a remains the same.
III. θ\theta increases.

Which statements are correct?

Retrieve the A.1 Kinematics Model

Describe motion

Position locates the object, velocity is the rate of change of position, and acceleration is the rate of change of velocity. Distance and speed are scalar; displacement and velocity are directed quantities.

Use the right model

For uniform acceleration:

v=u+at,\quad s=ut+ rac12at^2,\quad v^2=u^2+2as

For projectiles without drag, solve horizontal and vertical components with a shared time. Do not use these equations when acceleration is non-uniform.

Check the boundary

Ask whether the quantity is average or instantaneous, whether the route or endpoints matter, whether acceleration is constant, and whether a neglected force such as drag changes the model.

A.2 Forces and momentum

Syllabus
First assessment 2025
Topic
—
Level
HL

Use Newton’s Three Laws

Three linked laws

  1. If the resultant force is zero, velocity is constant.
  2. A resultant force changes momentum; for constant mass, F⃗net=ma⃗\vec F_{net}=m\vec a.
  3. Forces between two bodies are equal in magnitude and opposite in direction, acting on different bodies.

Choose the system

Draw forces acting on the chosen object, then use the resultant force to predict its acceleration. For action–reaction pairs, identify the two different bodies before applying the third law.

Use interactions to explain motion

A rocket pushes gas backward; the gas exerts an equal and opposite force on the rocket. The rocket can therefore accelerate even in the absence of a supporting surface.

Common trap

The forces in a third-law pair do not cancel in one free-body diagram because they act on different objects.

A.2.1 Exam Analysis

[ 3 ]

As the probe approaches the surface of the asteroid, a rocket engine is fired to slow its descent. Explain how the engine changes the speed of the probe.

Treat Force as an Interaction Between Bodies

A force needs an interaction

A force is an interaction between bodies. One body exerts the force and another body experiences it. Contact, gravitational, electric and magnetic interactions can all change momentum.

Name both bodies

When explaining a force, state the interacting pair and the direction of the force on the chosen body. The reaction force acts on the other body, not back on the same free-body diagram.

Fields can mediate interaction

Bodies do not need to touch for gravitational, electric or magnetic forces. For example, current-carrying coils interact through their magnetic fields, producing attraction or repulsion depending on the field arrangement.

Common trap

Do not describe a force as a property that an isolated object “has” without naming the other body or field involved.

A.2.2 Exam Analysis

[ 2 ]

Explain why, when there is a current in the coil, the separation of X and Y decreases.

Draw a Labelled Free-Body Diagram

Isolate one body

A free-body diagram shows only the chosen body and the external forces acting on it. Replace the body with a point or simple shape and choose useful axes.

Draw actual forces

Use arrows from the body, label each interaction and draw the direction physically. Typical labels include weight mgmg, normal force NN, tension TT, friction and drag.

Resolve only when needed

If a force is angled, resolve it into the chosen axes. Then apply ∑Fx=max\sum F_x=ma_x and ∑Fy=may\sum F_y=ma_y to the same body.

Common trap

Do not draw velocity, acceleration or a force exerted by the chosen body on its surroundings as forces acting on the chosen body.

A.2.3 Exam Analysis

[ 2 ]

Draw a labelled free-body diagram of the forces on the ball.

Drawing canvas

Find the Resultant Force from a Diagram

Add force components

The resultant force is the vector sum of all forces on the chosen body:

F⃗net=∑F⃗\vec F_{net}=\sum\vec F

Resolve angled forces into perpendicular components before adding.

Connect to acceleration

For constant mass, apply Newton’s second law along each axis:

∑Fx=max,∑Fy=may\sum F_x=ma_x,\qquad \sum F_y=ma_y

Use equilibrium correctly

If the resultant force is zero, acceleration is zero, but the object may still have constant non-zero velocity. A balanced vertical component does not imply every force is absent.

Common trap

Do not add force magnitudes without their directions. A component that balances another contributes zero only along the same axis.

A.2.4 Exam Analysis

[ 2 ]

Determine the acceleration of the truck.

Classify Contact Forces

Contact-force family

Contact forces arise when bodies or a body and fluid interact: normal force, friction, tension, elastic restoring force, viscous drag and buoyancy.

Use the interaction geometry

Normal force is perpendicular to the surface; friction acts along the surface opposing relative motion or attempted motion; tension acts along a taut string; drag opposes motion through a fluid; buoyancy acts upward due to fluid pressure differences.

Check the condition

Friction can be static or kinetic, drag depends on speed and shape, and buoyancy depends on displaced fluid. The magnitudes are determined by the interaction and constraints, not by a memorized universal value.

Common trap

Do not include every possible contact force. Include only interactions actually present in the described situation.

A.2.5 Exam Analysis

[ 1 ]

A ball is thrown from an aircraft in flight.

Which of the following shows the correct free-body diagram for the forces acting on the ball when terminal velocity is reached?

Model Normal Force Perpendicular to the Surface

Normal means perpendicular

The normal force NN is the contact force exerted by a surface perpendicular to that surface. Its direction follows the local surface normal, not necessarily the vertical direction.

Find it from the force balance

Use the component of Newton’s second law perpendicular to the surface. In a curved path, the normal force may combine with a component of weight to provide the required centripetal resultant.

Do not assume N=mgN=mg

N=mgN=mg applies only in situations where the perpendicular acceleration and other perpendicular force components make that balance valid. Inclines, lifts, loops and vertical acceleration change the normal force.

A.2.6 Exam Analysis

[ 3 ]

Determine the normal force exerted by the loop on the car at P .

Model Static and Dynamic Friction

Friction follows the contact

Friction acts parallel to the contact surface and opposes relative motion or the tendency of surfaces to move relative to each other.

Static friction adapts

Before slipping, static friction has whatever value is needed up to a maximum:

Ff≤μsNF_f\leq\mu_sN

It is not automatically equal to μsN\mu_sN; that value occurs at impending motion.

Dynamic friction during sliding

Once surfaces slide, the model gives

Ff=μdNF_f=\mu_dN

Use the normal force for the actual contact and combine friction with the other forces along the surface.

Common trap

Do not use the dynamic coefficient before motion begins, or assume static friction is always at its maximum.

A.2.7 Exam Analysis

[ 2 ]

Show that the minimum force needed to accelerate the box is about 4 N .

Trace Tension Along a String

Tension is a pull

Tension is the force exerted by a taut string, cable or rope on an attached body. It acts along the string and pulls away from the body.

Use the ideal-string model carefully

For a light, inextensible string over a frictionless pulley, tension has the same magnitude throughout. If the string, pulley or contact is non-ideal, tension can vary and must be found from each body’s force balance.

Connect tension to motion

Draw tension in the string direction, then use ∑F=ma\sum F=ma. A body can have non-zero tension while at rest if other forces balance it.

Common trap

A string can pull but not push. Do not draw tension toward the string’s far end through the body or assume its value equals the weight without a force balance.

A.2.8 Exam Analysis

[ 1 ]

Calculate the maximum tension in the string.

Apply Hooke’s Law to Elastic Restoring Force

Restoring force

For an ideal elastic element within its proportional range,

F⃗H=−kx⃗\vec F_H=-k\vec x

The minus sign means the force acts opposite the displacement from equilibrium.

Use extension correctly

For a spring, xx is extension or compression relative to its natural length. In a vertical equilibrium, the spring tension can balance weight, but the extension is not the total spring length.

Respect the model boundary

Hooke’s law is a linear approximation. Beyond the limit of proportionality, the force–extension graph is no longer linear and the same kk cannot be used.

A.2.9 Exam Analysis

[ 1 ]

A spring of negligible mass and length l0l_{0} hangs from a fixed point. When a mass m is attached to the free end of the spring, the length of the spring increases to l. The tension in the spring is equal to kΔxk \Delta x, where k is a constant and Δx\Delta x is the extension of the spring. What is k ?

Model Viscous Drag on a Small Sphere

Stokes drag

For a small sphere moving slowly through a viscous fluid,

Fd=6πηrvF_d=6\pi\eta r v

where η\eta is viscosity, rr is sphere radius and vv is speed relative to the fluid.

Drag opposes motion

The drag force points opposite the sphere’s velocity. As speed increases, drag increases linearly in this model, reducing the resultant force when the driving force is fixed.

Approach to terminal speed

For a falling sphere, weight drives the motion and viscous drag grows with speed. When drag balances the effective weight, acceleration becomes zero and terminal speed is reached.

Common trap

Do not treat viscosity η\eta as the same quantity as drag force, and do not forget that the formula applies to the stated small-sphere, viscous-flow model.

A.2.10 Exam Analysis

[ 2 ]

Describe why the acceleration of the oil droplet changes.

Calculate Buoyant Force from Displaced Fluid

Buoyancy from pressure difference

A fluid exerts a net upward buoyant force on an immersed object because pressure is greater at greater depth. In the IB model,

Fb=ρfVdispgF_b=\rho_fV_{disp}g

where VdispV_{disp} is the displaced fluid volume.

Separate buoyancy from net force

The buoyant force is one force in the free-body diagram. The net force is found after combining it with weight, tension, drag or other forces.

Floating condition

For an object at rest on the fluid, buoyancy balances its weight. This gives a useful density or submerged-volume relationship, but only after the equilibrium assumption is stated.

Common trap

Use the density of the displaced fluid and the displaced volume, not automatically the object’s total volume or density.

A.2.11 Exam Analysis

[ 1 ]

Show that FbF_{\mathrm{b}} is about 2 mN .

Separate Gravitational, Electric and Magnetic Forces

Three field interactions

Gravitational, electric and magnetic forces are field forces: bodies can interact without contact. Identify the source of the field, the object acted on and the force direction.

Keep the mechanisms distinct

Gravity acts on mass, electric force acts on charge, and magnetic force acts on moving charges or currents in a magnetic field. Their equations and direction rules are not interchangeable.

Use the force relevant to the system

A free-body diagram may contain more than one field force. Add them as vectors and apply Newton’s second law to the selected body.

Common trap

Do not call every non-contact force “electromagnetic”; gravitational attraction is a separate interaction.

A.2.12 Exam Analysis

[ 1 ]

What are three fundamental forces listed in decreasing order of strength?

Calculate Weight from Mass

Weight is a force

Weight is the gravitational force on a mass:

Fg=mgF_g=mg

The direction is toward the local gravitational field source.

Use local gg

The value of gg depends on location. Use the value stated or the local field strength appropriate to the body’s position; mass does not change when the object is moved.

Common trap

Mass is measured in kilograms and is not a force. Weight is measured in newtons and can change when gg changes.

A.2.13 Exam Analysis

[ 1 ]

The probe is carried to the asteroid on board a spacecraft.

Calculate the weight of the probe when close to the surface of the asteroid.

Identify Electric Force

Electric interaction

Electric force acts between charged bodies. Its direction depends on the signs of the charges: like charges repel and unlike charges attract.

Use the electric field

A positive test charge is pushed in the electric-field direction; a negative charge experiences force opposite to the field. Keep field direction and force direction separate when the charge sign matters.

Common trap

Do not reverse the force direction for a positive charge, and do not treat electric force as a contact force.

A.2.14 Exam Analysis

This exam question is unavailable.

Identify Magnetic Force

Magnetic interaction

A magnetic force acts on a moving charge or current in a magnetic field. Its direction is perpendicular to the relevant velocity/current and magnetic-field directions.

Apply the direction rule

Use the stated right-hand rule or vector relationship, then reverse the result for a negative charge. Parallel motion and field give zero magnetic force in the ideal model.

Common trap

A magnetic field can change the direction of velocity without doing work on an ideal moving charge; do not automatically infer a speed change from a magnetic force.

A.2.15 Exam Analysis

This exam question is unavailable.

Conserve Linear Momentum

Momentum

Linear momentum is

p⃗=mv⃗\vec p=m\vec v

It is a vector. For an isolated system, total momentum is conserved before and after an interaction.

Check the system

Momentum is conserved when the resultant external impulse on the chosen system is negligible. Internal forces can change individual momenta while leaving the vector total unchanged.

Use signs or components

Choose a positive direction and conserve momentum component-by-component. A negative final velocity means motion opposite to the chosen positive direction.

Common trap

Do not conserve kinetic energy automatically. Momentum conservation and kinetic-energy conservation are separate claims.

A.2.16 Exam Analysis

[ 1 ]

Cart X , of mass 2 kg , is moving at a speed of 3 m s−13 \mathrm{~m} \mathrm{~s}^{-1} to the right and collides on a horizontal track with cart Y of mass 1 kg.Y1 \mathrm{~kg} . Y is initially stationary.

The velocity of Y immediately after the collision is 4 m s−14 \mathrm{~m} \mathrm{~s}^{-1} to the right. What is the velocity of X immediately after the collision?

Calculate Impulse from Force and Time

Impulse changes momentum

Impulse is the integral of resultant force over time. For a constant average force,

J⃗=F⃗netΔt=Δp⃗\vec J=\vec F_{net}\Delta t=\Delta\vec p

Use the momentum change

Calculate Δp⃗=p⃗f−p⃗i\Delta\vec p=\vec p_f-\vec p_i, including direction. A rebound reverses the velocity component and can make the momentum change larger than either momentum magnitude alone.

Average force

If the force varies, FΔtF\Delta t represents average resultant force over the contact interval. Use consistent units for impulse in N s or kg m s⁻¹.

Common trap

Do not use the initial momentum alone when the object rebounds or ends with a non-zero final velocity.

A.2.17 Exam Analysis

[ 2 ]

The ball rebounds from the ground with speed 7.8 ms−17.8 \mathrm{~ms}^{-1}. The ball is in contact with the ground for a time T. The average resultant force on the ball during this time is 1.1 N .
Determine T.

Link External Impulse to Momentum Change

Impulse is external to the system

For a chosen system, the net external impulse equals the system’s change in total momentum:

J⃗ext=Δp⃗system\vec J_{ext}=\Delta\vec p_{system}

Same momentum change, different force

If an object must undergo the same Δp\Delta p, increasing the stopping time reduces the average resultant force:

Favg=ΔpΔtF_{avg}=\frac{\Delta p}{\Delta t}

Apply to safety systems

A flexible safety net, airbag or crumple zone extends the interaction time while producing the required momentum change, reducing the average force on the person or vehicle.

Common trap

Extending the stopping time does not make the momentum change disappear; it changes the rate at which that change occurs.

A.2.18 Exam Analysis

[ 2 ]

Explain, with reference to change in momentum, why a flexible safety net is less likely to harm the skier than a rigid barrier.

Choose the Momentum Form of Newton’s Second Law

Constant mass

For a body of constant mass, Newton’s second law becomes

F⃗net=ma⃗\vec F_{net}=m\vec a

Use the resultant force, not one arbitrarily selected force.

General momentum form

The broader statement is

F⃗net=Δp⃗Δt\vec F_{net}=\frac{\Delta\vec p}{\Delta t}

or its instantaneous form. This is the safer form when mass changes or when momentum is the quantity given.

Check what changes

If mass is constant, Δp=mΔv\Delta p=m\Delta v, so the two forms agree. If mass enters or leaves the system, include the momentum carried by that mass and define the system carefully.

Common trap

Do not double the acceleration simply because an applied force doubles when a fixed resistive force remains; calculate the new resultant force first.

A.2.19 Exam Analysis

[ 2 ]

Calculate the magnitude of the initial acceleration of the electron.

Distinguish Elastic and Inelastic Collisions

Momentum first

In an isolated collision, total linear momentum is conserved for both elastic and inelastic collisions.

Kinetic energy distinguishes them

In an elastic collision, total kinetic energy is also conserved. In an inelastic collision, some kinetic energy is transferred to internal energy, sound or deformation; in a perfectly inelastic collision the bodies move together afterward.

Use the right conservation law

Apply momentum conservation to find final velocities, then compare initial and final kinetic energy if the collision type is required.

Common trap

“Inelastic” does not mean momentum is lost. It means kinetic energy is not conserved.

A.2.20 Exam Analysis

[ 2 ]

Calculate the speed of the ship after the collision.

Ice in a still lake will usually form in a single layer on the surface.

Model an Explosion with Momentum Conservation

Explosion model

An explosion is an interaction in which an initially combined system separates into parts. If the external impulse is negligible, total momentum before and after is equal.

Use a sign convention

For an object initially at rest, the vector momenta after the explosion sum to zero. In one dimension, equal and opposite momenta can give different speeds when the masses differ.

Energy is separate

The chemical, elastic or other internal energy released can increase total kinetic energy while momentum remains conserved.

Common trap

Do not assume the fragments have equal speeds. Momentum magnitudes are equal and opposite only when the initial total momentum is zero.

A.2.21 Exam Analysis

This exam question is unavailable.

Track Energy in Collisions and Explosions

Track the energy store

Total energy is conserved, but kinetic energy may be transferred to internal energy, sound, deformation or chemical energy during an interaction.

Collision comparison

Elastic collisions conserve total kinetic energy as well as momentum. Inelastic collisions conserve momentum but have a lower final total kinetic energy.

Explosion comparison

An explosion can convert internal energy into kinetic energy, so final kinetic energy can exceed the initial kinetic energy while total momentum remains conserved.

Common trap

“Kinetic energy is lost” is shorthand for transferred to other stores; it is not destroyed.

A.2.22 Exam Analysis

[ 3 ]

Show that the collision is inelastic.

Calculate Centripetal Acceleration

Radial acceleration

For uniform circular motion, the centripetal acceleration is directed toward the centre:

ac=v2r=ω2r=4π2rT2a_c=\frac{v^2}{r}=\omega^2r=\frac{4\pi^2r}{T^2}

Velocity can be constant in magnitude

Even when speed is constant, the velocity direction changes continuously. That directional change produces inward acceleration.

Choose the matching data

Use v2/rv^2/r when speed and radius are given, ω2r\omega^2r when angular speed is given, or 4π2r/T24\pi^2r/T^2 when period is given.

Common trap

Centripetal acceleration is not tangential and does not point along the instantaneous velocity.

A.2.23 Exam Analysis

[ 2 ]

The fan is rotating at 120 revolutions every minute. Calculate the centripetal acceleration of the tip of a fan blade.

Find the Centripetal Force

Centripetal force is a resultant

Centripetal force is the name for the net inward force required for circular motion:

Fc=mac=mv2rF_c=ma_c=\frac{mv^2}{r}

Identify its physical source

Centripetal force is not an extra force. It may be supplied by tension, gravity, friction, normal force, electric force or a combination of forces.

Keep the direction clear

The required resultant points toward the centre and is perpendicular to instantaneous velocity in uniform circular motion.

Common trap

Do not add a separate “centripetal force” arrow to a free-body diagram unless the question explicitly uses it as a shorthand for the inward resultant.

A.2.24 Exam Analysis

[ 2 ]

Explain why a centripetal force is needed for the planet to be in a circular orbit.

Explain How Centripetal Force Changes Direction

Velocity direction changes

In circular motion, the inward centripetal acceleration changes the direction of the velocity. If speed is constant, the magnitude of velocity stays constant while its direction changes.

What happens if the inward force disappears

If the centripetal interaction is removed, the object continues along the tangent at the release point, consistent with Newton’s first law.

Maintain contact

In a vertical loop, the inward resultant must be sufficient to maintain the required radial acceleration. At the limiting contact condition, the normal force can fall to zero.

Common trap

The released object does not move along the radius; its instantaneous path is tangent to the circle.

A.2.25 Exam Analysis

[ 1 ]

A mass at the end of a string is swung in a horizontal circle at increasing speed until the string breaks.

The subsequent path taken by the mass is a

Link Angular and Linear Speed

Connect the descriptions

For uniform circular motion,

v=2πrT=ωrv=\frac{2\pi r}{T}=\omega r

Angular speed ω\omega is the same for all points on a rigid rotating body, while linear speed increases with distance from the axis.

Use the period

One revolution takes period TT, so ω=2π/T\omega=2\pi/T. Keep radians and seconds consistent.

Compare points on one disk

If one point is twice as far from the centre, its linear speed is twice as large at the same angular speed; its centripetal acceleration is also twice as large.

Common trap

Do not assume equal linear speeds for all points on a rotating disk. Equal angular speed does not mean equal tangential speed.

A.2.26 Exam Analysis

[ 1 ]

A disk of radius R rotates about its axis with angular speed ω\omega. Point X is at a distance of R2\frac{R}{2} from the centre and point Y is on the circumference.

What are the ratios of the linear speeds and the centripetal acceleration of X to Y.
The linear speed of X is vXv_{X} and its acceleration is aXa_{X}; the linear speed of Y is vYv_{Y} and its acceleration is aYa_{Y}.

Linear speeds vXvY\frac{\boldsymbol{v}_{\mathbf{X}}}{\boldsymbol{v}_{\mathbf{Y}}}

Acceleration aXaY\frac{\mathbf{a}_{\mathbf{X}}}{\mathbf{a}_{\mathbf{Y}}}

12\frac{1}{2}

14\frac{1}{4}

12\frac{1}{2}

12\frac{1}{2}

1

14\frac{1}{4}

1

12\frac{1}{2}

Retrieve the A.2 Forces and Momentum Model

Build the force model

Choose the system, draw a labelled free-body diagram, classify the interactions and resolve components. Apply Newton’s laws with the correct boundary: contact forces, field forces, friction, tension, buoyancy and restoring forces each have their own direction and conditions.

Track momentum

Use ec p=m ec v, ec J=\Delta ec p and momentum conservation only after checking external impulse. Distinguish elastic and inelastic collisions, explosions and energy transfer.

Track circular motion

The inward resultant provides ac=v2/r=ω2ra_c=v^2/r=\omega^2r. It may come from tension, gravity, normal, friction or a field force. Angular and linear descriptions are linked by v=ωr=2πr/Tv=\omega r=2\pi r/T.

Final checks

Ask: Which body is the system? Which forces are external? Is mass constant? Is acceleration uniform or radial? Is kinetic energy conserved, transferred or increased?

A.3 Work, energy and power

Syllabus
First assessment 2025
Topic
—
Level
HL

Conserve Energy in a System

Energy is conserved

Energy cannot be created or destroyed. In a defined system, energy is transferred between stores or across the system boundary, so the total energy accounting remains balanced.

Define the system first

Name the objects included and identify transfers by work, heating, radiation or electrical means. A falling object may transfer gravitational potential energy to kinetic energy, internal energy or sound.

Follow the chain

Write the initial store, the useful output store and any dissipated or transferred energy. A Sankey diagram or energy-flow statement should account for all significant branches.

Common trap

Energy “lost” from a useful store has been transferred elsewhere; it has not disappeared.

A.3.1 Exam Analysis

[ 2 ]

Outline, with reference to energy changes, the operation of a pumped storage hydroelectric system.

Relate Work to Energy Transfer

Work transfers energy

Work done by a force is the energy transferred by that force. For a constant force,

W=Fscos⁡θW=Fs\cos\theta

where θ\theta is the angle between force and displacement.

Use the sign

Positive work transfers energy into the object’s relevant store; negative work transfers energy out of it. A force perpendicular to displacement does zero work.

Follow the physical process

Wind can transfer kinetic energy to a turbine through work, while resistive forces can transfer mechanical energy to internal energy of the surroundings.

Common trap

Do not call every force an energy transfer. Check whether the force has a component along the displacement.

A.3.2 Exam Analysis

[ 2 ]

Describe the energy transfers taking place in a wind generator.

Read a Sankey Diagram

Read the width as energy

A Sankey diagram shows an input energy flowing into useful output and other transfers. Arrow width is proportional to energy, so the branches must account for the whole input.

Identify useful output

Label the useful branch before calculating efficiency. Other branches may represent heating, sound or unwanted mechanical transfers.

Connect to efficiency

The useful fraction of the input is

η=EusefulEinput=PusefulPinput\eta=\frac{E_{useful}}{E_{input}}=\frac{P_{useful}}{P_{input}}

Common trap

Do not compare branch widths without checking whether the diagram uses the same scale and whether the requested quantity is energy or power.

A.3.3 Exam Analysis

[ 1 ]

The Sankey diagram shows the energy input from fuel that is eventually converted to useful domestic energy in the form of light in a filament lamp.

What is true for this Sankey diagram?

Calculate Work by a Constant Force

Constant-force work

For a force FF acting through displacement ss,

W=Fscos⁡θW=Fs\cos\theta

Only the component parallel to displacement transfers energy by work.

Area under a force–distance graph

For a variable force, the area under an FF-against-ss graph gives work. A negative area represents work against the chosen displacement direction.

Check the angle

Use the angle between force and displacement, not the angle between the force and an unrelated axis unless the component has first been resolved.

Worked example from local Question Bank row 39177

A kite pulls a ship with force 2.50×105 N2.50\times10^5\,\mathrm{N} at 39∘39^\circ to its 1.00 km1.00\,\mathrm{km} displacement. Convert 1.00 km=1.00×103 m1.00\,\mathrm{km}=1.00\times10^3\,\mathrm{m}, then

W=Fscos⁡θ=(2.50×105)(1.00×103)cos⁡39∘=1.94×108 J≈1.9×108 JW=Fs\cos\theta=(2.50\times10^5)(1.00\times10^3)\cos39^\circ=1.94\times10^8\,\mathrm{J}\approx1.9\times10^8\,\mathrm{J}

Only the force component along the ship's displacement transfers energy.

A.3.4 Exam Analysis

[ 1 ]

State what is represented by the area under the graph.

Relate Resultant Work to Energy Change

Work–energy theorem

The net work done by the resultant force on a system equals its change in kinetic energy:

Wnet=ΔEkW_{net}=\Delta E_k

Use force–distance area

For a variable resultant force, the signed area under the force–distance graph gives the work and therefore the kinetic-energy change.

Include all resultant forces

Friction, applied forces and gravity may each do work. Add their signed contributions before relating the result to the final kinetic energy.

Worked example from local Question Bank row 31356

A constant net force of 100 N100\,\mathrm{N} moves an object from rest through 2.0 m2.0\,\mathrm{m} until its speed is 10 m s−110\,\mathrm{m\,s^{-1}}.

Wnet=Fs=(100)(2.0)=200 JW_{net}=Fs=(100)(2.0)=200\,\mathrm{J}
200=ΔEk=12m(10)2−0200=\Delta E_k=\frac12m(10)^2-0
m=4.0 kgm=4.0\,\mathrm{kg}

The positive net work is exactly the object's kinetic-energy gain.

Common trap

Do not use the work of one force as the net work unless all other force contributions are zero or already included.

A.3.5 Exam Analysis

[ 3 ]

A force of 14.0 N acts on the box for 0.35 m as shown. The force is then removed and the box continues to move. The box comes to rest after a further displacement d.

Determine d.

Identify Mechanical Energy

Mechanical energy stores

Mechanical energy is the sum of translational kinetic energy, gravitational potential energy and elastic potential energy:

Emech=Ek+Ep,g+Ep,elasticE_{mech}=E_k+E_{p,g}+E_{p,elastic}

Use the chosen system

Mechanical energy describes these stores within the system. Internal energy, chemical energy and sound may also be present in the full energy account but are not mechanical energy.

Common trap

Do not call all conserved energy mechanical energy; classify the store before applying a mechanical-energy equation.

A.3.6 Exam Analysis

[ 1 ]

show that the speed of the ball is about 4.3 ms−14.3 \mathrm{~ms}^{-1}.

Conserve Mechanical Energy Without Resistive Forces

Condition for conservation

Mechanical energy is conserved when only conservative forces transfer energy within the system and friction or other resistive transfers are absent or negligible.

Write the balance

Ek,i+Ep,i=Ek,f+Ep,fE_{k,i}+E_{p,i}=E_{k,f}+E_{p,f}

Choose a convenient zero for potential energy and keep the same reference throughout.

When it is not conserved

Friction, drag or deformation transfer mechanical energy to internal energy. Total energy is still conserved, but the mechanical-energy equation needs an additional transfer term.

A.3.7 Exam Analysis

[ 1 ]

An object is released from rest and slides down a frictionless ramp. The object then leaves the ramp and slides along a rough horizontal surface. The object stops in a distance s along the ramp.

The coefficient of dynamic friction between the object and the rough horizontal surface is μ\mu.
What is the height of the ramp?

Transform Mechanical Energy Between Stores

Conservative transformations

When mechanical energy is conserved, energy can move between translational kinetic, gravitational potential and elastic potential stores without changing their sum.

Use the endpoints

For a car descending a frictionless track, gravitational potential energy decreases while kinetic energy increases. For a spring system, elastic potential energy can become kinetic energy and then return.

Add non-conservative transfers

If friction or drag acts, part of the mechanical energy transfers to internal energy. The endpoint equation must include that loss from the mechanical stores.

A.3.8 Exam Analysis

[ 2 ]

Show that the speed of the car at P is 1.7 ms−11.7 \mathrm{~ms}^{-1}.

Calculate Translational Kinetic Energy

Kinetic-energy forms

Translational kinetic energy is

Ek=12mv2=p22mE_k=\frac12mv^2=\frac{p^2}{2m}

Choose the known quantity

Use 12mv2\frac12mv^2 when mass and speed are given, or p2/(2m)p^2/(2m) when momentum is given. Kinetic energy is scalar and cannot be negative.

Worked example from local Question Bank row 35674

For m=0.14 g=1.4×10−4 kgm=0.14\,\mathrm{g}=1.4\times10^{-4}\,\mathrm{kg} and v=3.1 m s−1v=3.1\,\mathrm{m\,s^{-1}},

Ek=12(1.4×10−4)(3.1)2=6.7×10−4 J=0.67 mJE_k=\frac12(1.4\times10^{-4})(3.1)^2=6.7\times10^{-4}\,\mathrm{J}=0.67\,\mathrm{mJ}

Converting grams to kilograms before substitution keeps the energy unit in joules.

Common trap

Doubling speed quadruples kinetic energy; do not scale it linearly with speed.

A.3.9 Exam Analysis

[ 2 ]

Calculate the final speed of the car.

Calculate Gravitational Potential Energy Change

Near-Earth gravitational potential energy

For a height change Δh\Delta h in a uniform gravitational field,

ΔEp,g=mgΔh\Delta E_{p,g}=mg\Delta h

Use the height change

Raising an object gives positive change in gravitational potential energy; lowering it gives negative change relative to the chosen reference.

Link to power

If height changes at constant speed, the rate of gravitational potential-energy gain is mgvmgv, before accounting for efficiency or other transfers.

Worked example from local Question Bank row 37039

An object's weight is 6.10×102 N6.10\times10^2\,\mathrm{N} and it rises vertically by 8.0 m8.0\,\mathrm{m}. Since mgmg is its weight,

ΔEp,g=(6.10×102)(8.0)=4.88×103 J≈4.9 kJ\Delta E_{p,g}=(6.10\times10^2)(8.0)=4.88\times10^3\,\mathrm{J}\approx4.9\,\mathrm{kJ}

The positive result means the gravitational potential-energy store increases.

Common trap

Use the local value of gg and the vertical height change, not the distance along a slope.

A.3.10 Exam Analysis

[ 1 ]

A car takes 20 minutes to climb a hill at constant speed. The mass of the car is 1200 kg and the car gains gravitational potential energy at a rate of 6.0 kW . Take the acceleration of gravity to be 10 m s−210 \mathrm{~m} \mathrm{~s}^{-2}. What is the height of the hill?

Calculate Elastic Potential Energy

Elastic store

For a spring within its linear range,

Ep,elastic=12k(Δx)2E_{p,elastic}=\frac12k(\Delta x)^2

where Δx\Delta x is extension or compression from the natural length.

Area under the graph

The elastic potential energy equals the work done in stretching or compressing the spring. On a force–extension graph it is the area under the graph.

Worked example from local Question Bank row 31357

A spring with k=100 N m−1k=100\,\mathrm{N\,m^{-1}} is compressed by 0.10 m0.10\,\mathrm{m}.

Ep,elastic=12(100)(0.10)2=0.50 JE_{p,elastic}=\frac12(100)(0.10)^2=0.50\,\mathrm{J}

This is the energy available for transfer when the ideal spring is released.

Common trap

Do not use the total spring length as Δx\Delta x, and remember that doubling extension quadruples the stored energy in the ideal model.

A.3.11 Exam Analysis

[ 1 ]

0.25 J\quad 0.25 \mathrm{~J} of work is done to compress a spring by a distance of 0.10 m from its unstretched length. What is the spring constant?

Calculate Power as a Transfer Rate

Power is rate

Power is the rate of work or energy transfer:

P=ΔWΔt=ΔEΔtP=\frac{\Delta W}{\Delta t}=\frac{\Delta E}{\Delta t}

Mechanical shortcut

For a constant force parallel to velocity,

P=FvP=Fv

Keep energy and power distinct

Energy is measured in joules; power is measured in watts, or joules per second. Multiply power by time to recover transferred energy.

Worked example from local Question Bank row 29322

A student of weight 600 N600\,\mathrm{N} climbs 6.0 m6.0\,\mathrm{m} vertically in 8.0 s8.0\,\mathrm{s}.

ΔW=(600)(6.0)=3.6×103 J\Delta W=(600)(6.0)=3.6\times10^3\,\mathrm{J}
P=3.6×1038.0=4.5×102 W=450 WP=\frac{3.6\times10^3}{8.0}=4.5\times10^2\,\mathrm{W}=450\,\mathrm{W}

The result is the average rate of energy transfer against gravity.

A.3.12 Exam Analysis

[ 1 ]

A student of mass m initially at rest takes t seconds to run up stairs of height h. At the top of the stairs the student has a velocity v.

What is the average power supplied by the student during the climb?

Calculate Efficiency

Useful fraction

Efficiency is the ratio of useful output to total input:

η=EusefulEinput=PusefulPinput\eta=\frac{E_{useful}}{E_{input}}=\frac{P_{useful}}{P_{input}}

Choose matching quantities

Use energy ratios for the same process and time interval, or power ratios when input and output are rates. Efficiency is dimensionless and is often reported as a percentage.

Worked example from local Question Bank row 29709

Solar intensity is 240 W m−2240\,\mathrm{W\,m^{-2}} over 2.50×104 m22.50\times10^4\,\mathrm{m^2}, so input power is

Pin=(240)(2.50×104)=6.0×106 W=6.0 MWP_{in}=(240)(2.50\times10^4)=6.0\times10^6\,\mathrm{W}=6.0\,\mathrm{MW}

For a useful output of 1.6 MW1.6\,\mathrm{MW},

η=1.66.0=0.27=27%\eta=\frac{1.6}{6.0}=0.27=27\%

The remaining input is transferred through non-useful pathways.

Common trap

Do not invert the ratio or use the total output, including unwanted transfers, as the useful output.

A.3.13 Exam Analysis

[ 1 ]

An electric motor of efficiency 75 % raises a mass of 120 kg at a constant speed of 0.50 ms−10.50 \mathrm{~ms}^{-1}. What is the power input to the motor?

Compare Fuel Energy Density

Energy per volume

For the current IB Physics definition, fuel energy density uu is the transferable energy per unit volume:

u=EVu=\frac{E}{V}

Its SI unit is J m−3\mathrm{J\,m^{-3}}. This lets fuels be compared when storage volume is the constraint.

Connect it to a fuel flow

If fuel flows at volume rate V˙\dot V, its input power is Pin=uV˙P_{in}=u\dot V. Apply efficiency only after finding the input energy or power.

Worked example from local Question Bank row 36970

An engine produces 20 kW20\,\mathrm{kW} useful power at 50%50\% efficiency while consuming 1.0×10−5 m3 s−11.0\times10^{-5}\,\mathrm{m^3\,s^{-1}} of fuel.

Pin=20 kW0.50=40 kWP_{in}=\frac{20\,\mathrm{kW}}{0.50}=40\,\mathrm{kW}
u=PinV˙=4.0×1041.0×10−5=4.0×109 J m−3=4.0 GJ m−3u=\frac{P_{in}}{\dot V}=\frac{4.0\times10^4}{1.0\times10^{-5}}=4.0\times10^9\,\mathrm{J\,m^{-3}}=4.0\,\mathrm{GJ\,m^{-3}}

Common trap

Specific energy is energy per unit mass, measured in J kg−1\mathrm{J\,kg^{-1}}. Some sources use the words loosely, so let the stated definition and units determine whether to divide by volume or mass.

A.3.14 Exam Analysis

[ 2 ]

At the end of the 30-day period, rockets are fired to bring the ISS back to its initial height. The energy density of liquid hydrogen rocket fuel is 8.5×103MJm−38.5 \times 10^{3} \mathrm{MJ} \mathrm{m}^{-3}.

Estimate the volume of fuel needed.

Retrieve the A.3 Work, Energy and Power Model

Account for energy

Define the system, identify energy stores and describe transfers. Work done by a force transfers energy; total energy is conserved even when mechanical energy is not.

Use the mechanical model

E_k= rac12mv^2,\quad \Delta E_{p,g}=mg\Delta h,\quad E_{p,elastic}= rac12k(\Delta x)^2

Conserve their sum only when resistive transfers are absent or included explicitly.

Use rates and ratios

P= rac{\Delta E}{\Delta t}=Fv,\qquad \eta= rac{E_{useful}}{E_{input}}= rac{P_{useful}}{P_{input}}

Fuel energy density connects available input energy to a chosen volume.

Final checks

Check the system boundary, signs of work and potential-energy changes, the reference height, extension from natural length, and whether the quantity is energy, power, efficiency or energy density.

A.4 Rigid body mechanics

Syllabus
First assessment 2025
Topic
—
Level
HL

Calculate Torque About an Axis

HL only

Torque is a turning effect

The torque of a force about an axis is

τ=Frsin⁡θ\tau=Fr\sin\theta

where rr is the distance from the axis to the point of application and θ\theta is the angle between r⃗\vec r and F⃗\vec F.

Use the perpendicular lever arm

Equivalently, torque equals force multiplied by the perpendicular distance from the axis to the force’s line of action.

Choose a rotation sign

Clockwise and anticlockwise torques have opposite signs. Add torques about the specified axis rather than adding their magnitudes blindly.

Worked example from local Question Bank row 37867

Two forces produce the same rotational sense: 50 N50\,\mathrm{N} at a perpendicular distance 0.50 m0.50\,\mathrm{m} and 40 N40\,\mathrm{N} at 0.20 m0.20\,\mathrm{m}.

τnet=(50)(0.50)+(40)(0.20)=25+8=33 N m≈30 N m\tau_{net}=(50)(0.50)+(40)(0.20)=25+8=33\,\mathrm{N\,m}\approx30\,\mathrm{N\,m}

If one force acted in the opposite sense, its torque would enter with the opposite sign.

Common trap

A force through the axis has zero torque, even if its magnitude is large.

A.4.1 Exam Analysis

HL only

[ 2 ]

Calculate the torque that acts on the disk while it accelerates.

Test Rotational Equilibrium

HL only

Equilibrium condition

A rigid body is in rotational equilibrium when the resultant torque about any chosen axis is zero:

∑τ=0\sum\tau=0

Balance clockwise and anticlockwise effects

Choose an axis, assign signs, and set the sum of clockwise torques equal to the sum of anticlockwise torques. A body can still have translational equilibrium as a separate condition.

Common trap

Zero resultant torque means no angular acceleration; it does not by itself prove that the net force is zero.

A.4.2 Exam Analysis

HL only

[ 1 ]

State the condition for rotational equilibrium.

Turn Unbalanced Torque into Angular Acceleration

HL only

Rotational second law

A non-zero resultant torque causes angular acceleration:

∑τ=Iα\sum\tau=I\alpha

Use the chosen axis

Calculate signed torques about the specified axis and use the moment of inertia about that same axis. The direction of α\alpha follows the resultant torque.

Common trap

Do not use translational F=maF=ma for a purely rotational equation or mix an inertia about one axis with torque about another.

A.4.3 Exam Analysis

HL only

[ 3 ]

Calculate the angular acceleration of the disk.

Describe Angular Motion

HL only

Three angular quantities

Angular displacement θ\theta describes change in orientation, angular velocity ω=dθ/dt\omega=d\theta/dt describes how fast orientation changes, and angular acceleration α=dω/dt\alpha=d\omega/dt describes how angular velocity changes.

Link to linear motion

At radius rr, tangential speed is v=rωv=r\omega. Keep angular quantities in radians when using these relationships.

Common trap

Angular velocity is not automatically the same as linear speed; the radius is needed to connect them.

A.4.4 Exam Analysis

HL only

[ 1 ]

Calculate the angular velocity ω\omega of P.

Apply Rotational SUVAT

HL only

Uniform angular acceleration

When α\alpha is constant, use rotational SUVAT:

ω=ω0+αt,θ=ω0t+12αt2,ω2=ω02+2αθ\omega=\omega_0+\alpha t,\quad \theta=\omega_0t+\frac12\alpha t^2,\quad \omega^2=\omega_0^2+2\alpha\theta

Choose the equation

List θ,ω0,ω,α,t\theta,\omega_0,\omega,\alpha,t, convert revolutions to radians, and choose the equation containing the required unknown and known quantities.

Worked example from local Question Bank row 39408

A bar starts from rest and turns through six revolutions with constant α=0.110 rad s−2\alpha=0.110\,\mathrm{rad\,s^{-2}}. Convert Δθ=6(2π)=12π rad\Delta\theta=6(2\pi)=12\pi\,\mathrm{rad}, then

ωf2=ωi2+2αΔθ=0+2(0.110)(12π)\omega_f^2=\omega_i^2+2\alpha\Delta\theta=0+2(0.110)(12\pi)
ωf=2.88 rad s−1≈2.9 rad s−1\omega_f=2.88\,\mathrm{rad\,s^{-1}}\approx2.9\,\mathrm{rad\,s^{-1}}

The equation is valid because angular acceleration is constant.

Common trap

Do not use rotational SUVAT when angular acceleration varies, and do not insert degrees or revolutions where radians are required.

A.4.5 Exam Analysis

HL only

[ 1 ]

A wheel, initially at rest, rolls without slipping down an incline for 4.0 s . The final angular velocity of the wheel is 5πrads−15 \pi \mathrm{rads}^{-1}.

How many revolutions did the wheel complete?

Understand Moment of Inertia

HL only

Rotational inertia

Moment of inertia measures resistance to angular acceleration about an axis. It depends on total mass and how far that mass is distributed from the axis.

Compare distributions

For the same mass and outer radius, more mass farther from the axis gives larger II. A ring therefore has greater rotational inertia than a disk of the same mass and radius.

Common trap

Moment of inertia is not determined by mass alone; always specify the rotation axis and distribution.

A.4.6 Exam Analysis

HL only

[ 3 ]

The disk and a ring, with the same mass and radius, are released from the top of the slope at the same time. Explain, without numerical calculation, which one will reach the bottom of the inclined plane first.

Calculate Point-Mass Moment of Inertia

HL only

Point-mass model

For discrete masses rotating about an axis,

I=∑mr2I=\sum mr^2

where each rr is the perpendicular distance from the axis.

Build the sum

Treat each small sphere, blade or mass element separately, calculate mr2mr^2, and add the contributions. Use symmetry when identical masses have equal radii.

Worked example from local Question Bank row 128743

Two 10 kg10\,\mathrm{kg} point masses are 8.0 m8.0\,\mathrm{m} apart and rotate about the midpoint. Each is 4.0 m4.0\,\mathrm{m} from the axis:

I=∑mr2=2(10)(4.0)2=320 kg m2I=\sum mr^2=2(10)(4.0)^2=320\,\mathrm{kg\,m^2}

The full 8.0 m8.0\,\mathrm{m} separation is not the radius of either mass.

Common trap

Do not use the distance between two masses as rr for both; use each mass’s distance to the rotation axis.

A.4.7 Exam Analysis

HL only

[ 1 ]

A two-blade propeller can be modelled using the two-cylinder arrangement in (a)(iii).

The following data for the two-blade propeller are available:
Length of each blade: 0.60 m
Mass of each blade: 2.2 kg
Show that the moment of inertia of the two-blade propeller is about 0.5 kg m20.5 \mathrm{~kg} \mathrm{~m}^{2}.

Apply Rotational Newton’s Second Law

HL only

Torque–inertia relation

For rotation about a fixed axis,

τnet=Iα\tau_{net}=I\alpha

Connect translation and rotation

When a force drives a rotating body or pulley, write both the translational force balance and the rotational torque balance if the system has translating and rotating parts.

Worked example from local Question Bank row 31942

A 50 N50\,\mathrm{N} tangential force acts 2.0 m2.0\,\mathrm{m} from the axis of a system with I=450 kg m2I=450\,\mathrm{kg\,m^2}.

τ=Fr=(50)(2.0)=100 N m\tau=Fr=(50)(2.0)=100\,\mathrm{N\,m}
α=τI=100450=0.22 rad s−2\alpha=\frac{\tau}{I}=\frac{100}{450}=0.22\,\mathrm{rad\,s^{-2}}

The acceleration direction follows the signed resultant torque.

Common trap

Do not treat torque as force or use a moment of inertia that does not match the rotation axis.

A.4.8 Exam Analysis

HL only

[ 1 ]

The graph shows how the angular acceleration α\alpha of a flywheel varies with torque τ\tau applied to the flywheel.

What is the moment of inertia of the flywheel?

Calculate Angular Momentum

HL only

Rotational momentum

For a rigid body rotating about a fixed axis,

L=IωL=I\omega

Angular momentum is directed along the rotation axis by the right-hand convention.

Use the matching inertia

The moment of inertia must be calculated about the same axis used for LL. A larger II at the same angular speed means larger angular momentum.

Worked example from local Question Bank row 31945

For I=450 kg m2I=450\,\mathrm{kg\,m^2} and ω=1.66 rad s−1\omega=1.66\,\mathrm{rad\,s^{-1}},

L=Iω=(450)(1.66)=7.47×102 kg m2 s−1≈750 kg m2 s−1L=I\omega=(450)(1.66)=7.47\times10^2\,\mathrm{kg\,m^2\,s^{-1}}\approx750\,\mathrm{kg\,m^2\,s^{-1}}

The sign or axis direction must match the chosen rotational convention.

Common trap

Do not substitute translational momentum mvmv for angular momentum when the question describes rotation.

A.4.9 Exam Analysis

HL only

[ 2 ]

the angular momentum.

Conserve Angular Momentum

HL only

Conservation condition

Angular momentum remains constant when the resultant external torque about the chosen axis is zero:

Li=LfL_i=L_f

Redistribute the mass

When a skater pulls their arms inward, II decreases. With angular momentum conserved, ω\omega increases.

Worked example from local Question Bank row 34033

A 0.200 kg0.200\,\mathrm{kg} particle moving at 12.0 m s−112.0\,\mathrm{m\,s^{-1}} strikes 0.60 m0.60\,\mathrm{m} from an axis. Its initial angular momentum is

Li=mvr=(0.200)(12.0)(0.60)=1.44 kg m2 s−1L_i=mvr=(0.200)(12.0)(0.60)=1.44\,\mathrm{kg\,m^2\,s^{-1}}

If the combined system has If=0.252 kg m2I_f=0.252\,\mathrm{kg\,m^2} and external torque is negligible,

Ifωf=Li⇒ωf=1.440.252=5.71 rad s−1I_f\omega_f=L_i\Rightarrow\omega_f=\frac{1.44}{0.252}=5.71\,\mathrm{rad\,s^{-1}}

Common trap

Angular momentum conservation does not require rotational kinetic energy to remain constant when the moment of inertia changes.

A.4.10 Exam Analysis

HL only

[ 1 ]

An ice skater is spinning with their arms extended in a fixed position at a constant angular velocity. The ice skater then quickly pulls their arms closer to their body. Frictional effects are negligible.

Three statements are made about the ice skater's motion.

I. The angular momentum of the ice skater remains constant.
II. The rotational kinetic energy of the ice skater remains constant.
III. The net torque acting on the ice skater is zero.

Which of the statements are correct?

Calculate Angular Impulse

HL only

Angular impulse

A torque acting for a time changes angular momentum:

ΔL=τΔt=Δ(Iω)\Delta L=\tau\Delta t=\Delta(I\omega)

Area under a torque–time graph

If torque varies, the signed area under a τ\tau-against-time graph gives angular impulse and therefore the change in angular momentum.

Common trap

Angular impulse has units N m s, not N s; keep it distinct from linear impulse.

A.4.11 Exam Analysis

HL only

[ 1 ]

What is the unit of angular impulse?

Calculate Rotational Kinetic Energy

HL only

Rotational energy

For a rigid body rotating about a fixed axis,

Ek=12Iω2=L22IE_k=\frac12I\omega^2=\frac{L^2}{2I}

Combine forms of motion

A rolling object may have translational kinetic energy of its centre of mass and rotational kinetic energy about its centre. Include both when accounting for total kinetic energy.

Worked example from local Question Bank row 31644

A rod of weight 36.0 N36.0\,\mathrm{N} lowers its centre of mass by 5.00/2=2.50 m5.00/2=2.50\,\mathrm{m} and has I=30.6 kg m2I=30.6\,\mathrm{kg\,m^2}. If the gravitational transfer becomes rotational kinetic energy,

Ek=(36.0)(2.50)=90.0 JE_k=(36.0)(2.50)=90.0\,\mathrm{J}
90.0=12(30.6)ω2⇒ω=2.43 rad s−190.0=\frac12(30.6)\omega^2\Rightarrow\omega=2.43\,\mathrm{rad\,s^{-1}}

The energy result is in joules; angular speed is in radians per second.

Common trap

Do not use 12mv2\frac12mv^2 alone for a rotating body when its rotational motion contributes energy.

A.4.12 Exam Analysis

HL only

[ 1 ]

A car of total mass M is travelling with a constant speed v. Each of the four wheels of the car has a mass m and a radius R and rolls without slipping.

The moment of inertia of each wheel is I=12mR2I=\frac{1}{2} m R^{2}.
What is  sum of the rotational kinetic energy of all four wheels  translational kinetic energy of the car ?\frac{\text { sum of the rotational kinetic energy of all four wheels }}{\text { translational kinetic energy of the car }} ?

Retrieve the A.4 Rigid Body Mechanics Model

HL only

Torque and rotation

Use au=Frsin⁡hetaau=Fr\sin heta, ∑au=0\sum au=0 for rotational equilibrium and \sum au=Ilpha for angular acceleration. Always state the axis and use the matching moment of inertia.

Describe angular motion

Use angular displacement, angular velocity and angular acceleration; rotational SUVAT applies only for uniform lpha. Point-mass inertia is I=∑mr2I=\sum mr^2.

Track angular momentum

L=Iω,ΔL=auΔtL=I\omega,\quad \Delta L= au\Delta t

Conserve angular momentum only when external resultant torque is negligible.

Track rotational energy

E_{rot}= rac12I\omega^2

For rolling or coupled systems, include translational and rotational energy separately.

A.5 Galilean and special relativity

Syllabus
First assessment 2025
Topic
—
Level
HL

Choose a Reference Frame

HL only

Define the frame

A reference frame is a coordinate system, with a chosen origin and axes, together with a way of assigning time to events. Position and time are coordinates: they describe an event only after the observer’s frame has been stated.

Describe the same event in two frames

For an event, record its position xx and time tt in frame S, then x′x′ and t′t′ in frame S′. If S′ moves at constant velocity relative to S, both frames are inertial. The event is the same physical occurrence even though its coordinates may differ.

Check the frame type

An inertial reference frame is non-accelerating. Newton’s laws can be used in their usual form in such a frame. If the frame accelerates or rotates, extra apparent forces may be needed and it is not an inertial frame for this syllabus treatment.

Common trap

A frame is not just a camera viewpoint. It specifies the spatial axes and the time measurement used to assign coordinates; therefore “at rest” or “moving” has meaning only relative to a stated frame.

A.5.1 (HL) Exam Analysis

HL only

[ 1 ]

Explain why observer Y is at rest in the reference frame of the electron.

Apply Galilean Relativity

HL only

State the principle

Galilean relativity says that Newton’s laws have the same form in every inertial reference frame. An observer moving at constant velocity therefore uses the same Newtonian mechanics, provided speeds are far below the speed of light and the frame is non-accelerating.

Relate the observations

The same event occurs in both frames, but the observers can assign different positions. In the classical model, time is absolute: both observers use the same tt, while the moving frame changes the position coordinate according to x′=x−vtx′=x-vt.

Check the boundary

Use Galilean relativity for inertial frames in the non-relativistic limit. It is not the correct model for measurements involving speeds comparable with cc, where the assumptions of absolute time and unchanged light speed fail.

Common trap

“Same laws” does not mean that all observers measure the same position or velocity. It means the equations of Newtonian mechanics keep the same form after changing between inertial frames.

A.5.2 (HL) Exam Analysis

HL only

[ 1 ]

Write down the length of the space station according to Galilean relativity.

Apply Galilean Transformations

HL only

Transform event coordinates

For frames S and S′ that are coincident at t=t′=0t=t′=0, with S′ moving at velocity vv in the positive xx-direction relative to S, the Galilean transformations are x′=x−vtx′=x-vt and t′=tt′=t.

Use the sign convention

Start with the event coordinates (x,t)(x,t) in S. Substitute the frame velocity with its signed value, calculate x′x′, and carry the unchanged time t′=tt′=t into S′. A positive x′x′ means the event is on the positive side of S′’s origin.

Check the assumptions

These equations describe the classical model: inertial frames, common synchronized time, and an origin coincidence at t=0t=0. They are not the Lorentz transformations and do not preserve the speed of light between frames.

Symbolic example from local Question Bank row 31622

An event has x′=Lx'=L and t′=L/ct'=L/c in S′. Galilean time is absolute, so t=t′=L/ct=t'=L/c. Using the inverse position transformation,

x=x′+vt=L+vLcx=x'+vt=L+v\frac{L}{c}

The extra vL/cvL/c is the distance travelled by the S′ origin during the shared time interval.

Common trap

Do not change tt using t′=t−vx/c2t′=t-vx/c^2; that belongs to the relativistic transformation. In a Galilean transformation, time is shared: t′=tt′=t.

A.5.3 (HL) Exam Analysis

HL only

[ 1 ]

The Lorentz transformations assume that the speed of light is constant. Outline what the Galilean transformations assume.

Add Velocities Galilean-Style

HL only

Use the classical addition rule

If an object has velocity uu in frame S and frame S′ moves at velocity vv relative to S, the velocity measured in S′ is u′=u−vu′=u-v. Both uu and vv are signed velocities along the chosen axis.

Calculate in two steps

Choose the positive direction, write the velocity of the object and the relative frame velocity with signs, then subtract. If the object and S′ move in the same direction, the relative speed is reduced; if they move in opposite directions, the signed relative velocity has greater magnitude.

Check the model

Galilean addition assumes inertial frames, common time, and non-relativistic speeds. It can predict a resultant speed greater than cc, which signals that special relativity—not the arithmetic—is required for a high-speed light problem.

Worked example from local Question Bank row 31297

In the classical model, two spacecraft moving in opposite directions at 0.80c0.80c have signed velocities u=−0.80cu=-0.80c and v=+0.80cv=+0.80c.

u′=u−v=−0.80c−0.80c=−1.60cu'=u-v=-0.80c-0.80c=-1.60c

The magnitude 1.60c1.60c shows why Galilean addition cannot describe relativistic relative velocity; the sign only gives direction in S′.

Common trap

Do not subtract speed magnitudes before deciding the direction. The sign of u′u′ tells you the object’s direction in S′; dropping signs can reverse the physical interpretation.

A.5.4 (HL) Exam Analysis

HL only

[ 1 ]

State, using Galilean relativity, the speed of the radio signal relative to Q .

State the Two Relativity Postulates

HL only

Postulate 1: relativity

The laws of physics have the same form in all inertial reference frames. No inertial observer is privileged by uniform motion; an experiment performed entirely within a frame cannot reveal its constant velocity relative to another inertial frame.

Postulate 2: invariant light speed

Every inertial observer measures the same speed of light in vacuum, cc, independent of the motion of the source or observer. This replaces the Galilean expectation that measured velocities simply add.

Use the consequence

Together, the postulates require space and time coordinates to transform differently from the Galilean model. They lead to Lorentz transformations, time dilation, length contraction and relativity of simultaneity. The syllabus does not require deriving those equations.

Common trap

The second postulate does not say that every object moves at cc, or that light speed is the same in every material. It refers to light in vacuum measured by inertial observers.

A.5.5 (HL) Exam Analysis

HL only

[ 3 ]

Explain, by reference to the equivalence principle, why the frequency of the photon measured at B will be larger than f0f_{0}.

Apply Lorentz Transformations

HL only

Set the relativistic factor

For two inertial frames with relative speed vv, use γ=1/1−v2/c2\gamma=1/\sqrt{1-v^2/c^2}. At ordinary speeds γ≈1\gamma\approx1; as vv approaches cc, the difference from Galilean coordinates becomes significant.

Transform one event

For an event with coordinates (x,t)(x,t) in S, the syllabus equations are x′=γ(x−vt)x′=\gamma(x-vt) and t′=γ(t−vx/c2)t′=\gamma(t-vx/c^2) in S′. Use the same signed direction for xx and vv, and calculate both coordinates from the same event.

Show the coordinate method

Write γ\gamma first, substitute the given x,t,vx,t,v, then report x′x′ and t′t′ with units. If the question provides a space–time diagram, reading the coordinates is an alternative only when the axes and scale are correctly interpreted.

Worked example from local Question Bank rows 31630–31631

For v=0.745cv=0.745c, γ=1/1−0.7452=1.499\gamma=1/\sqrt{1-0.745^2}=1.499. An event at x=1.0 mx=1.0\,\mathrm{m} and t=0t=0 transforms to

x′=γ(x−vt)=1.499(1.0)=1.50 mx'=\gamma(x-vt)=1.499(1.0)=1.50\,\mathrm{m}
ct′=γ(ct−vcx)=1.499(0−0.745×1.0)=−1.12 mct'=\gamma(ct-\tfrac{v}{c}x)=1.499(0-0.745\times1.0)=-1.12\,\mathrm{m}

Thus t′=−1.12/c st'=-1.12/c\,\mathrm{s}; the negative coordinate is valid and reflects the chosen origins.

Respect the syllabus boundary

Know and apply the transformation equations; their derivation is not required. The frames must be inertial, and the relative speed must satisfy v<cv<c so that γ\gamma is real.

A.5.6 (HL) Exam Analysis

HL only

[ 3 ]

Determine the spacetime coordinates of the event according to observer B.

Add Velocities Relativistically

HL only

Use the relativistic rule

For an object with velocity uu in S and a frame S′ moving at velocity vv relative to S, use u′=(u−v)/(1−uv/c2)u′=(u-v)/(1-uv/c^2). The numerator is the classical relative velocity; the denominator is the correction required by special relativity.

Substitute signed velocities

Choose one positive direction, write signed values for uu and vv, calculate uv/c2uv/c^2, and evaluate the full fraction. Report the magnitude if the question asks for speed; retain the sign if it asks for velocity or direction.

Check the limiting cases

When u≪cu\ll c and v≪cv\ll c, the denominator is close to 1 and the result approaches u−vu-v. If u=cu=c, the equation gives u′=cu′=c for any sub-light vv, so light does not gain or lose speed between inertial frames.

Worked example from local Question Bank row 31056

A train has u=−0.70cu=-0.70c in the ground frame and observer P moves at v=+0.60cv=+0.60c.

u′=−0.70c−0.60c1−(−0.70)(0.60)=−1.30c1.42=−0.915c≈−0.92cu'=\frac{-0.70c-0.60c}{1-(-0.70)(0.60)}=\frac{-1.30c}{1.42}=-0.915c\approx-0.92c

The negative sign means the train moves opposite P's positive direction; its speed remains below cc.

Common trap

Do not use u−vu-v for a high-speed signal. Also do not report a result above cc; a sign error or an omitted denominator usually caused it.

A.5.7 (HL) Exam Analysis

HL only

[ 2 ]

Determine, using relativistic velocity addition, the speed of the radio signal relative to Q .

Use the Invariant Space-Time Interval

HL only

Define the interval

For two events separated by Δt\Delta t and Δx\Delta x, the space–time interval is (Δs)2=(cΔt)2−(Δx)2(\Delta s)^2=(c\Delta t)^2-(\Delta x)^2. Although observers can measure different Δt\Delta t and Δx\Delta x, the value of (Δs)2(\Delta s)^2 is invariant between inertial frames.

Calculate carefully

Read the time and position differences between the same two events. Convert Δt\Delta t into the distance cΔtc\Delta t, square both terms, and subtract the spatial term: (cΔt)2−(Δx)2(c\Delta t)^2-(\Delta x)^2. Keep the sign; a negative result is physically meaningful.

Compare frames

Calculate the interval from either frame’s coordinates. Matching values demonstrate invariance and provide a check on transformed coordinates. For a light signal, (Δs)2=0(\Delta s)^2=0; this null interval is consistent with Δx=cΔt\Delta x=c\Delta t.

Worked example from local Question Bank row 32720

For two events with cΔt=100 lyc\Delta t=100\,\mathrm{ly} and Δx=20 ly\Delta x=20\,\mathrm{ly},

(Δs)2=(100)2−(20)2=10,000−400=9,600 ly2(\Delta s)^2=(100)^2-(20)^2=10{,}000-400=9{,}600\,\mathrm{ly^2}

Any inertial frame must calculate the same 9,600 ly29{,}600\,\mathrm{ly^2} from its own coordinate differences.

Common trap

Do not replace the subtraction with addition, and do not take an absolute value before reporting. The sign distinguishes the interval type and is part of the answer.

A.5.8 (HL) Exam Analysis

HL only

[ 2 ]

Calculate the space-time interval (Δs)2(\Delta s)^{2} between P and Q .

Identify Proper Time and Length

HL only

Identify proper time

The proper time interval Δt0\Delta t_0 is measured between two events that occur at the same position in the observer’s frame. It is the shortest time interval measured for those events. For a clock at rest in the frame, successive ticks occur at one location, so the clock measures Δt0\Delta t_0.

Identify proper length

The proper length L0L_0 is the length measured in the rest frame of the object. Its endpoints are measured simultaneously in that frame. It is the maximum length assigned to the object by inertial observers.

Choose from the event conditions

For time, ask: do the two events happen at the same place in this frame? For length, ask: is the object at rest in this frame, and are both endpoints measured at the same time? These conditions, not the observer’s label, determine whether the measurement is proper.

Common trap

Proper time is not simply the time measured by the “main” observer, and proper length is not the shortest measured length. The proper length is the rest-frame, longest length; moving observers measure a contracted length.

A.5.9 (HL) Exam Analysis

HL only

[ 1 ]

Define what is meant by proper length.

Calculate Time Dilation

HL only

Use the time-dilation equation

When Δt0\Delta t_0 is the proper time between two events, an observer for whom the events occur at different positions measures Δt=γΔt0\Delta t=\gamma\Delta t_0, where γ=1/1−v2/c2\gamma=1/\sqrt{1-v^2/c^2}.

Identify the proper interval first

Find the frame in which the two events occur at the same place; that frame measures Δt0\Delta t_0. Calculate γ\gamma using the relative speed, then multiply by Δt0\Delta t_0 to obtain the longer interval measured in the other inertial frame.

Check the direction of the effect

Because γ≥1\gamma\ge1, the non-proper observer measures a time interval at least as large as the proper interval. At v=0v=0, γ=1\gamma=1 and the two measurements agree.

Worked example from local Question Bank rows 30639–30640

A spacecraft crosses 1.80×1011 m1.80\times10^{11}\,\mathrm{m} at 0.750c0.750c. The station-frame interval is

Δt=1.80×10110.750(3.00×108)=800 s\Delta t=\frac{1.80\times10^{11}}{0.750(3.00\times10^8)}=800\,\mathrm{s}

With γ=1/1−0.7502=1.51\gamma=1/\sqrt{1-0.750^2}=1.51, the spacecraft clock measures the proper time

Δt0=8001.51=530 s\Delta t_0=\frac{800}{1.51}=530\,\mathrm{s}

The events occur at one place on the spacecraft, so its interval is proper.

Common trap

Do not multiply the proper time by 1/γ1/\gamma when finding the dilated interval. The inverse is used only when the question gives the larger interval and asks for the proper time.

A.5.10 (HL) Exam Analysis

HL only

[ 2 ]

S arrives at P after 50 years according to Earth. Calculate the time at which S arrives at P according to S clocks.

Calculate Length Contraction

HL only

Use the contraction equation

If L0L_0 is the proper length measured in the object’s rest frame, an observer who sees the object moving at speed vv measures L=L0/γL=L_0/\gamma, with γ=1/1−v2/c2\gamma=1/\sqrt{1-v^2/c^2}.

Select the proper length

Find the frame in which the object is at rest; that frame measures L0L_0. Calculate γ\gamma, then divide the proper length by γ\gamma. The endpoints must be measured simultaneously in the observer’s frame.

Check the result

Since γ≥1\gamma\ge1, a moving observer measures L≤L0L\le L_0. At low speed the contraction is negligible; as vv approaches cc, the measured length along the direction of motion becomes substantially smaller.

Worked example from local Question Bank row 30450

A rocket's proper length is L0=450 mL_0=450\,\mathrm{m} and γ=5/3\gamma=5/3. An observer who sees it moving measures

L=L0γ=4505/3=270 mL=\frac{L_0}{\gamma}=\frac{450}{5/3}=270\,\mathrm{m}

Only the dimension parallel to the relative motion is contracted.

Common trap

Do not contract a length perpendicular to the motion, and do not multiply by γ\gamma when the requested quantity is the moving-frame length.

A.5.11 (HL) Exam Analysis

HL only

[ 2 ]

Calculate the length of the space station according to observer B, with reference to special relativity.

Explain Relativity of Simultaneity

HL only

State the idea

Two events that are simultaneous in one inertial reference frame need not be simultaneous in another frame moving relative to it. Simultaneity is therefore not an absolute property of separated events.

Use the transformed time

For two events, Δt′=γ(Δt−vΔx/c2)\Delta t'=\gamma(\Delta t-v\Delta x/c^2). If Δt=0\Delta t=0 in S but Δx≠0\Delta x\neq0, then Δt′≠0\Delta t'\neq0 in a relatively moving frame.

Worked example from local Question Bank row 30453

Two lamps are simultaneous in S and separated by 9.00×103 m9.00\times10^3\,\mathrm{m}. For v=0.80cv=0.80c and γ=5/3\gamma=5/3,

Δt′=53(0−(0.80c)(9.00×103)c2)=−4.0×10−5 s\Delta t'=\frac53\left(0-\frac{(0.80c)(9.00\times10^3)}{c^2}\right)=-4.0\times10^{-5}\,\mathrm{s}

The negative sign fixes the event order in S′; it is not an error.

Keep the order test local

To decide which event occurs first in a frame, calculate or read the sign of Δt′\Delta t′ using the same pair of events. A negative time difference means the event assigned as the second reference event occurs earlier in that frame.

Common trap

The relativity of simultaneity concerns spatially separated events. Events at the same place cannot be simultaneous in one frame and ordered differently in another inertial frame.

A.5.12 (HL) Exam Analysis

HL only

[ 2 ]

According to observer B, event E occurs before observer A and observer B meet. Justify this statement using the spacetime diagram.

Read a Space-Time Diagram

HL only

Read the axes

A space–time diagram plots position horizontally and ctct vertically; the time axis is labelled ctct, so both axes have distance units. An event is a point (x,ct)(x,ct). A world line joins the events of one object through time.

Interpret a world line

A vertical world line represents an object at rest in that frame. A straight tilted line represents constant velocity. A light ray has v=cv=c and lies on the 45° light line when the axes use equal scales; no physical world line may be steeper toward the x-axis than the light line.

Read simultaneity and coordinates

To find an event’s time, project horizontally to the ctct axis; to find position, project vertically to the xx axis. Lines parallel to an observer’s x′x′ axis represent equal t′t′, while lines parallel to ct′ct′ represent equal x′x′.

Common trap

Do not treat the slope as an ordinary x/tx/t graph slope without accounting for the ctct axis and the diagram’s scale. Always identify which frame’s axes are being used.

A.5.13 (HL) Exam Analysis

HL only

[ 2 ]

Identify, with lines and labels on the spacetime diagram, the difference between t1t_{1} and t2t_{2}.

Relate World-Line Angle to Speed

HL only

Use the angle relation

On a space–time diagram with equal scales, the angle θ\theta between a particle’s world line and the time axis satisfies tan⁡θ=v/c\tan\theta=v/c. Therefore v=ctan⁡θv=c\tan\theta.

Read the line

A vertical line has θ=0\theta=0 and represents rest. As the line tilts toward the x-axis, θ\theta and the speed increase. The light line has θ=45∘\theta=45^\circ on equal scales and represents v=cv=c.

Calculate from a diagram

Measure or read the angle from the time axis, evaluate tan⁡θ\tan\theta, and multiply by cc. If the diagram gives a rise/run ratio, use that ratio as tan⁡θ\tan\theta only after confirming the axes and angle definition.

Worked example from local Question Bank row 31477

For a world line representing v=0.80cv=0.80c on equal-scale axes,

θ=tan⁡−1(v/c)=tan⁡−1(0.80)=38.7∘≈39∘\theta=\tan^{-1}(v/c)=\tan^{-1}(0.80)=38.7^\circ\approx39^\circ

The angle is measured from the ctct axis, not the xx axis.

Common trap

Do not measure the angle from the x-axis, and do not assume every diagram uses equal visual scales. The syllabus relation is tied to the stated world-line angle and labelled axes.

A.5.14 (HL) Exam Analysis

HL only

[ 1 ]

Rocket R travels away from an observer on Earth at a speed of 0.80 c . A space-time diagram shows four world lines.

What is the correct world line of R in the reference frame of Earth?

Use Muon Decay Evidence

HL only

Start from the observation

Muons created high in Earth’s atmosphere have a short proper lifetime, yet many are detected at the ground while travelling at speeds close to cc. Without relativistic effects, the flight time through the atmosphere would exceed the muon lifetime and far fewer would survive.

Explain it in the Earth frame

In the Earth frame the moving muon’s lifetime is dilated: Δt=γΔt0\Delta t=\gamma\Delta t_0. The increased lifetime allows more muons to travel the atmospheric distance before decaying. This is experimental evidence for time dilation.

Explain it in the muon frame

In the muon’s frame, the atmosphere is moving and its thickness is length-contracted: L=L0/γL=L_0/\gamma. The shorter distance can be crossed within the muon’s proper lifetime. Both frames predict the same detection rate; together they support time dilation and length contraction.

Evidence calculation from local Question Bank row 30447

Muons are produced 2.0 km2.0\,\mathrm{km} above ground, move at 0.98c0.98c, have proper lifetime 2.2 μs2.2\,\mu\mathrm{s} and γ=5.0\gamma=5.0.

tflight=20000.98(3.0×108)=6.8 μst_{flight}=\frac{2000}{0.98(3.0\times10^8)}=6.8\,\mu\mathrm{s}
tEarth=γt0=(5.0)(2.2)=11 μst_{Earth}=\gamma t_0=(5.0)(2.2)=11\,\mu\mathrm{s}

The dilated Earth-frame lifetime exceeds the flight time, explaining why many more muons reach the ground than the non-relativistic model predicts.

Common trap

Do not claim that the muon’s own clock runs slow in its rest frame. The proper lifetime is measured by the muon; the Earth observer measures the dilated lifetime, while the muon observer measures a contracted atmosphere.

A.5.15 (HL) Exam Analysis

HL only

[ 3 ]

Muons are detected at the Earth's surface.

Explain, with supporting calculations, why this is evidence for time dilation.

Retrieve the A.5 Galilean and Special Relativity Model

HL only

Choose the model

State the inertial reference frame first. Galilean relativity uses x′=x−vt, t′=t and u′=u−v. Special relativity uses the two postulates, Lorentz transformations and u′=(u−v)/(1−uv/c²).

Track what changes and what is invariant

In special relativity, use γ=1/√(1−v²/c²), the invariant interval (Δs)²=(cΔt)²−(Δx)², proper time, proper length, Δt=γΔt0 and L=L0/γ. Separate measurements of space and time can change between frames, while the interval and vacuum light speed do not.

Read the evidence

On a space–time diagram, world-line angle gives tanθ=v/c, frame axes determine simultaneity, and no world line exceeds the light line. Muon survival provides experimental evidence: time dilation explains the longer Earth-frame lifetime, while length contraction explains the shorter atmospheric distance in the muon frame.

Final retrieval check

For every calculation, identify the frame, select the proper quantity if one is given, keep signed velocities and units consistent, and check the result against c, γ≥1, or the invariant interval. The syllabus requires applying the transformations and equations, not deriving them.