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Theme A — Space, Time and Motion

A.2 Forces and Momentum — IB Physics HL Revision Notes & Topical Questions

5 min read 10 parts Lesson 11 of 63 1 quiz

📚 IB Physics HL Hub / Topical Revision
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Curriculum Equation Key قوانين الرقم الهيدروجيني والاتزان الأيوني - pH & Acid-Base Equilibrium FormulasFast Exam Solution
pH = -log[H⁺] | pOH = -log[OH⁻] | pH + pOH = 14 | [H⁺][OH⁻] = 10⁻¹⁴
Word Equation & Conditions: الرقم الهيدروجيني = -لوغاريتم تركيز أيون الهيدروجين | pH + pOH = 14
Location & Specifications: الاتزان الأيوني، كيمياء 3 ثانوي، التحصيلي، و AP Chemistry.
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Lesson summary

A.2 Forces and Momentum — IB PHYSICS HL notes: Apply Newton's laws, types of force, momentum, impulse, collisions and circular motion to problems of force and motion.A free-body diagram shows all the forces on one object, drawn as arrows from a point mass at the centre of mass.Ar…

  • Common forces
  • Resultant (net) force
  • Second law
  • What the symbols mean
  • Contact forces act between touching objects
  • Use the symbol given in the question

Part 1 of 8Free-body diagrams and resultant force

A free-body diagram shows all the forces on one object, drawn as arrows from a point mass at the centre of mass.
  • Arrow length shows magnitude and direction shows the direction of the force.
  • Label each force by name or symbol and include only forces acting on the object.
Common forces
  • Common forces weight Fg , tension FT (away from the mass), normal reaction FN (perpendicular to the surface) and friction Ff (opposite to motion).
    • (towards the planet)
Resultant (net) force
Resultant (net) force the vector sum of the forces on a body.
  • Balanced forces give zero resultant; unbalanced forces give a non-zero resultant.
  • In one dimension add forces with signs; in two dimensions resolve with Pythagoras and trigonometry.

Part 2 of 8Newton's laws of motion

1
First law
  • First law a body stays at rest or moves with constant velocity unless acted on by a resultant force.
  • Zero resultant force means translational equilibrium: at rest or constant velocity.
2
Second law
  • Second law the resultant force is proportional to acceleration, F = ma, in the direction of the force.
  • Equivalent form — resultant force equals rate of change of momentum, F = Δp/Δt, valid for changing mass.
    What the symbols mean: F = force (N) · Δt = time the force acts (s) · Δp = change in momentum (kg m s−1); FΔt is the impulse (N s)
  • A force opposing motion causes deceleration, not reversal of motion.
3
Third law
  • Third law if A exerts a force on B, B exerts an equal and opposite force on A.
  • A third-law pair must be the same type of force, equal in magnitude, opposite in direction and on different objects.
  • Book on tablethe weight and the normal force are not a pair — the pair of weight is the book's gravitational pull on Earth.

Part 3 of 8Contact and non-contact forces

Contact and non-contact forces
Contact forces act between touching objects
  • Contact forces act between touching objects friction, fluid resistance (drag), tension and the normal force.
Non-contact forces act at a distance through a field.
  • Gravitational force, with weight Fg = mg on Earth.
  • Electrostatic force, attractive or repulsive.
  • Magnetic force between poles or on moving charges.
Use the symbol given in the question
  • Fg is the syllabus symbol for weight, though W is often used.

Part 4 of 8Friction

1Friction opposes motion or prevents it
  • Friction opposes motion or prevents it and transfers energy by heating.
2
Surface friction acts parallel to the contact plane and depends on the normal force.
3Static friction matches the applied force up to a maximum
  • Ff ≤ μsFN.
4Dynamic friction acts during sliding
  • Ff = μdFN, a definite value.
5The maximum static friction is larger than dynamic friction
  • μs above μd, both between 0 and 1.
6
Fluid resistance (viscous drag) acts on bodies moving through a gas or liquid.

Part 5 of 8Hooke's law, Stokes' law and buoyancy

1Hooke's law
  • F = kΔx, for extension or compression of a spring or material up to its limit.
    What the symbols mean: F = force (N) · k = spring constant (N m−1) · x or e = extension (m)
  • k is the spring constant, the gradient of the straight part of a force–extension graph.
  • Use extension, not total length, and check which axis holds force.
2Stokes' law
  • Stokes' law viscous drag on a sphere Fd = 6πηrv.
  • η is the fluid viscosity, r the radius and v the speed.
3Buoyancy (upthrust)
  • Fb = ρVg, with ρ the fluid density and V the volume of fluid displaced.
  • A body floats when buoyancy equals its weight.
4Terminal speed of a sphere
  • Terminal speed of a sphere weight = drag + buoyancy, giving v = 2r2g(ρs − ρf) / 9η.
  • v is proportional to r2 and inversely proportional to η.

Part 6 of 8Momentum, impulse and force

Momentum, impulse and force
Momentum p
Momentum p mv — a vector in kg m s-1.
Conservation of linear momentum
  • Conservation of linear momentum total momentum before equals total momentum after, unless an external resultant force acts.
  • Take the direction of initial motion as positive; a rebound has negative velocity.
Impulse J
FΔt = Δp = mv − mu — in N s, in the direction of the force.
  • The equations apply for a constant force.
  • 1 N = 1 kg m s-2.
Increasing the time of impact reduces the force
  • Increasing the time of impact reduces the force a fielder's hands move back on catching a cricket ball.
Hail exerts more impulse on an umbrella than rain
  • Hail exerts more impulse on an umbrella than rain because it rebounds with a larger change in momentum.

Part 7 of 8Collisions and explosions

1Collision
  • Collision objects come together and exert forces for a short time;
    • explosion — objects initially at rest are propelled apart.
2Momentum is always conserved
  • Momentum is always conserved kinetic energy may not be.
TypeKinetic energyExample
ElasticConservedParticle collisions (ideal)
InelasticNot conservedAll macroscopic collisions
Totally inelasticMaximum lost; bodies stick togetherMoving as one mass
ExplosionNever conserved; starts at restGun recoil, alpha emission
Collisions and explosions
Check the type
  • Check the type compare kinetic energy Ek = ½mv2 before and after.
Kinetic energy is a scalar and never negative.
Two dimensions
  • Two dimensions conserve each component of momentum separately.
  • For an elastic collision with one body initially at rest, the final directions are 90° apart.

Part 8 of 8Circular motion

Circular motion
Uniform circular motion
  • Uniform circular motion constant speed with changing velocity, so there is acceleration.
Period T and frequency f
1/T — speed v = 2πr/T.
Angular displacement θ
Angular displacement θ s/r in radians — 2π rad = 360°.
Angular speed ω
Δθ/Δt = 2π/T = 2πf, in rad s-1 — linear speed v = ωr.
Centripetal acceleration a
Centripetal acceleration a v2/r = ω2r = 4π2r/T2, towards the centre.
Centripetal force F
Centripetal force F mv2/r = mω2r — the resultant force towards the centre.
  • It is not a separate force — it is tension, friction, gravity, electrostatic or magnetic force.
  • It does no work because it is perpendicular to the velocity.
Car on a flat bend
  • Car on a flat bend friction provides the force, so vmax = √(μgr).
Banked track
  • Banked track horizontal components of normal force and friction provide the force.
Vertical circle
  • Vertical circle tension is maximum at the bottom (mv2/r + mg) and minimum at the top (mv2/r − mg).

Key terms

TermMeaning
Resultant forceVector sum of all forces acting on a body.
ImpulseForce multiplied by time, equal to change in momentum.
MomentumProduct of mass and velocity.
Elastic collisionCollision in which kinetic energy is conserved.
Centripetal forceResultant force towards the centre keeping a body in circular motion.
BuoyancyUpward force from displaced fluid, ρVg.
Viscous dragFrictional force between an object and a fluid.

Avoid these mistakes

1
Treating weight and the normal force as a third-law pair — they act on the same object.
2
Calling centripetal force a separate force rather than the resultant of real forces.
3
Forgetting the sign change of velocity, momentum and impulse on rebound.
4
Using ρ of the object instead of the fluid density in the buoyancy force.
5
Using angles in degrees for angular speed — use radians.

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