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A.2 Forces and momentum

Syllabus
First assessment 2025
Topic
Level
SL

Objective notes

26 learning objectives
A.2.1—Newton’s three laws of motion

• Newton’s three laws of motion.

A.2.2—Forces as interactions between bodies

• Forces as interactions between bodies.

A.2.3—Free-body diagrams

• Forces acting on a body can be represented in a free-body diagram.

A.2.4—Resultant force from diagrams

• Free-body diagrams can be analysed to find the resultant force on a system.

A.2.5—Contact forces

• Contact forces include normal, friction, tension, elastic restoring force, viscous drag and buoyancy.

A.2.6—Normal force

• Normal force FN acts perpendicular to the contact surface.

A.2.7—Frictional force

• Friction acts parallel to contact.

• Static: Ff <= μsFN; dynamic: Ff = μdFN.

A.2.8—Tension

• Tension.

A.2.9—Hooke’s law restoring force

• Elastic restoring force follows Hooke’s law: FH = -kx.

A.2.10—Viscous drag

• Viscous drag on a small sphere: Fd = 6πηrv, opposite motion.

• η is fluid viscosity, r sphere radius, v speed through fluid.

A.2.11—Buoyancy

• Buoyancy from displaced fluid: Fb = ρVg.

A.2.12—Field forces

• Know field forces: gravitational, electric and magnetic.

A.2.13—Weight

• Weight is gravitational force: Fg = mg.

A.2.14—Electric force Fe

• Electric force Fe.

A.2.15—Magnetic force Fm

• Magnetic force Fm.

A.2.16—Linear momentum conservation

• Linear momentum p=mv is conserved unless a resultant external force acts.

A.2.17—Impulse

• Impulse from resultant external force: J = FΔt = Δp.

A.2.18—Impulse-momentum change

• The applied external impulse equals the change in momentum of the system.

A.2.19—Newton’s second law forms

• Use F=ma for constant mass; use F=Δp/Δt when mass changes.

A.2.20—Elastic and inelastic collisions

• Elastic and inelastic collisions of two bodies.

A.2.21—Explosions

• Explosions.

A.2.22—Collision energy

• Compare energy in elastic collisions, inelastic collisions and explosions.

A.2.23—Centripetal acceleration

• Centripetal acceleration is radial: a=v^2/r=ω^2r=4π^2r/T^2.

• Direction is radially toward the centre of the circle.

A.2.24—Centripetal force

• Circular motion is caused by a centripetal force acting perpendicular to the velocity.

A.2.25—Direction change in circular motion

• A centripetal force causes the body to change direction even if its magnitude of velocity may remain constant.

A.2.26—Angular and linear speed

• Circular motion relation: v=2πr/T=ωr.

• Use angular velocity ω and period T to link angular and linear descriptions.

ConceptIB Physics SL