Introduction to Force and Dynamics
Dynamics explores the underlying causes of changes in motion, extending beyond pure kinematics (horizontal straight-line, vertical straight-line, and circular motion) to analyze why objects start moving, stop, accelerate, or maintain constant velocity.
The study of dynamics integrates key kinematic quantities—displacement, velocity, and acceleration—with the foundational physical properties of force and mass.
Core objectives of force dynamics:
- Define force in terms of the acceleration imparted to a standard body.
- Assign mass to objects to explain why different bodies experience different accelerations when subjected to identical environmental conditions.
- Calculate net forces acting on a body based on object properties and environmental interactions.
Concepts of Force and Mass
A force is defined in everyday terms as a push or a pull.
Force is a vector quantity, possessing both magnitude and direction.
A spring balance is a standard instrument used for measuring the magnitude of a force.
Vector resolution of forces allows any angled force to be split into perpendicular horizontal (x) and vertical (y) components:

- Example of force component calculation:
- For a block of mass m=50.0kg pulled by an applied force FA=400N at an angle of 57∘ above the horizontal:
- Horizontal component (FAx):
FAx=FAcos(57∘)=400N×cos(57∘)=218N
- Vertical component (FAy):
FAy=FAsin(57∘)=400N×sin(57∘)=335N
Newton's Laws of Motion
- Newton's First Law of Motion (Law of Inertia):
- A body remains in a state of rest or continues in uniform motion in a straight line at a constant velocity unless acted upon by a net external force.
- Inertia is the inherent property of a body to resist changes in its state of rest or motion.
- When the vector sum of all forces acting on a body is zero, the body is in translational equilibrium:
∑F=0
∑Fx=0
∑Fy=0
In equilibrium, an object's acceleration is zero (a=0m/s2), meaning it is either permanently at rest or moving with constant velocity.
- Newton's Second Law of Motion:
If a net external force acts on a body, the body accelerates in the direction of that net force. The net force vector equals the product of the mass and the acceleration of the body:
∑F=ma
∑Fx=max
∑Fy=may
- The SI unit of force is the Newton (N):
1N=1kg⋅m/s2
- One Newton is defined as the force required to impart an acceleration of 1m/s2 to a mass of 1kg.
- Worked Example (Car Deceleration):
- Problem: Calculate the net force required to bring a 1500kg car to rest from an initial velocity of 30.6m/s within a stopping distance of 55m.
- Kinematic equation with constant acceleration:
vf2=vi2+2aΔx
- Solving for acceleration (a):
a=2Δxvf2−vi2=2(55m)02−(30.6m/s)2=110m−936.36=−8.5127m/s2
- Calculating required force (F):
F=ma=(1500kg)×(−8.5127m/s2)=−12769N≈−12800N
- The negative sign indicates that the net force opposes the initial velocity vector.
- Newton's Third Law of Motion:
- For every action, there is an equal and opposite reaction.
- If body A exerts a force FAB on body B, body B simultaneously exerts an equal and opposite force FBA on body A:
FAB=−FBA
- Action and reaction forces act on two entirely different objects, meaning they never directly cancel each other out on a single free body diagram.
Fundamental Types of Forces
- Weight (w):
- The gravitational pull exerted on a body by Earth (or another astronomical body).
- From Newton's second law, for a freely falling body, a=g:
w=mg
Weight acts vertically downward toward the center of the gravitational source.
- Normal Force (N or FN):
A contact force exerted by a surface on an object touching it.
It always acts perpendicular to the surface of contact.
The pulling force exerted by each end of a stretched rope, cord, string, or cable.
Tension pulls away from the attached object along the string line. In a continuous string connecting two objects, tension acts towards opposite directions at the respective endpoints.
A contact force exerted parallel to the interface between an object and a surface, opposing sliding or intended motion.

- Static Friction (fs): Prevents an object at rest from starting to move. Its maximum possible value is:
fs,max=μsN
- Motion does not begin until the applied force exceeds fs,max.
- Kinetic Friction (fk): Retards motion for an object actively sliding across a surface:
fk=μkN
- μs is the coefficient of static friction and μk is the coefficient of kinetic friction.
- Worked Example (Box of Bananas on Horizontal Surface):
- Given: Box weight w=40.0N, μs=0.40, μk=0.20.
- Normal force: N=w=40.0N.
- Maximum static friction limit: fs,max=μsN=0.40×40.0N=16.0N.
- Kinetic friction force: fk=μkN=0.20×40.0N=8.00N.
- Scenario Analyses:
- a) If no horizontal force is applied at rest, the friction force is 16.0N static limit threshold.
- b) If a monkey applies a horizontal force of 6.0N to the box while static, the recorded friction threshold is 16.0N.
- c) Minimum horizontal force needed to sustain constant velocity once moving equals the kinetic friction force fk=8.00N.
- d) If a horizontal force of 18.0N is applied:
- Net horizontal force: ∑Fx=Fapplied−fk=18.0N−8.00N=10.0N.
- Mass of box: m=gw=9.8m/s240.0N=4.0816kg.
- Acceleration calculation:
a=m∑Fx=4.0816kg10.0N=2.45m/s2
Applications of Newton's First Law

- Given: Block weight w=600N. Three cords meet at origin point O. Cord 1 makes 60∘ north of east with the ceiling, Cord 2 is horizontal to the left (west), and Cord 3 hangs vertically supporting the block.
- Step 1: Equilibrium of the suspended block:
∑Fy=T3−w=0⟹T3=w=600N
- Step 2: Equilibrium at junction O:
∑Fy=T1y−T3=0⟹T1sin(60∘)−T3=0
T1=sin(60∘)T3=sin(60∘)600N=693N
- Horizontal equilibrium:
∑Fx=T1x−T2=0⟹T1cos(60∘)−T2=0
T2=T1cos(60∘)=693N×cos(60∘)=347N
- Example 2: Asymmetric Hanging Sphere Equilibrium:

- Given: Mass m=5.0kg. Cord 1 makes an angle of 40∘ with the ceiling (40∘ north of west). Cord 2 makes an angle of 50∘ with the ceiling (50∘ north of east). Cord 3 hangs vertically attached to the mass.
- Step 1: Force on suspended block:
T3=w=mg=5.0kg×9.8m/s2=49N
- Step 2: Forces acting on the junction point:
∑Fx=T2x−T1x=0⟹T2cos(50∘)=T1cos(40∘)
T2=T1cos(50∘)cos(40∘)
- Vertical components:
∑Fy=T1y+T2y−T3=0⟹T1sin(40∘)+T2sin(50∘)−T3=0
- Substituting T2 expression into vertical equation:
T1sin(40∘)+T1(cos(50∘)cos(40∘))sin(50∘)=T3
T1(cos(50∘)sin(40∘)cos(50∘)+cos(40∘)sin(50∘))=T3
- Utilizing trigonometric angle addition identity sin(A+B)=sinAcosB+cosAsinB:
sin(40∘+50∘)=sin(90∘)=1
T1(cos(50∘)sin(90∘))=T3⟹T1=T3cos(50∘)
T1=49N×cos(50∘)=31.5N
- Calculating T2:
T2=31.5N×cos(50∘)cos(40∘)=37.5N
Applications of Newton's Second Law
- Example 1: Single Block Pulled at an Angle with Surface Friction:

- Given: Box mass m=10.0kg, cord tension T=40.0N at θ=30∘ north of east, coefficient of kinetic friction μk=0.20.
- Weight of box: w=mg=10.0kg×9.8m/s2=98.0N.
- Tension components:
Tx=Tcos(30∘)=40.0N×cos(30∘)=34.64N
Ty=Tsin(30∘)=40.0N×sin(30∘)=20.0N
∑Fy=N+Ty−w=may=0
N=w−Ty=98.0N−20.0N=78.0N
- (b) Acceleration (a):
- Friction force: fk=μkN=0.20×78.0N=15.6N.
- Horizontal dynamics:
∑Fx=Tx−fk=max
a=mTx−fk=10.0kg34.64N−15.6N=10.0kg19.04N=1.90m/s2
- Example 2: Two Connected Blocks over a Pulley:

- Given: Sliding block mass m1=4.0kg on table with μk=0.15, connected via string over pulley to hanging block m2=2.0kg.
- Forces on sliding block (m1):
- Vertical forces: N=m1g=4.0kg×9.8m/s2=39.2N.
- Kinetic friction: fk=μkN=0.15×39.2N=5.88N.
- Horizontal force equation: T−fk=m1a⟹T−5.88=4.0a
- Forces on hanging block (m2):
- Weight: w2=m2g=2.0kg×9.8m/s2=19.6N.
- Vertical force equation: w2−T=m2a⟹19.6−T=2.0a
- (a) Acceleration of the two blocks:
- Summing system equations:
(T−5.88)+(19.6−T)=4.0a+2.0a
13.72=6.0a⟹a=6.013.72=2.29m/s2
- (b) Tension in the cord (T):
T=19.6−2.0(2.2867)=15.0N
Applications of Newton's Third Law
- Example: Three Contact Blocks Pushed by External Force:

- Given: Three blocks each of mass m1=m2=m3=12.0kg placed side-by-side on a frictionless surface. External horizontal force F=96.0N is applied directly to block 1.
- (a) Acceleration of the system:
- Combined mass: Mtotal=m1+m2+m3=12.0kg+12.0kg+12.0kg=36.0kg.
a=MtotalF=36.0kg96.0N=2.67m/s2
- (b) Contact forces on each block:
- Free body diagram for block 1 (m1):
∑Fx=F−F12=m1a⟹96.0N−F12=(12.0kg)(2.67m/s2)=32.0N
F12=96.0N−32.0N=64.0N
- Free body diagram for block 3 (m3):
∑Fx=F23=m3a=(12.0kg)(2.67m/s2)=32.0N
- Verification on block 2 (m2):
∑Fx=F12−F23=64.0N−32.0N=32.0N=m2a
Newton's Law of Universal Gravitation
- Statement: Every particle in the universe attracts every other particle with a force directly proportional to the product of their masses and inversely proportional to the square of the distance separating their centers.

F=Gr2m1m2
- m1,m2 are the particle masses.
- r is the separation distance between centers.
- G is the universal gravitational constant:
G=6.674×10−11N⋅m2/kg2
- Example Calculation:
- Given: m1=12.0kg, m2=25.0kg, r=1.20m.
- Gravitational force calculation:
F=(6.674×10−11N⋅m2/kg2)×(1.20m)2(12.0kg)(25.0kg)
F=6.674×10−11×1.44300=6.674×10−11×208.333=1.39×10−8N
Centripetal Force
Fc=rmv2=mac
Where ac=rv2 is the centripetal acceleration.
Direction: Always points radially inward toward the center of the circular path, continuously changing direction as the body moves.
Worked Example (Ball Twirled on String):
Given: Ball mass m=12.0g=0.0120kg, radius r=10.0cm=0.100m, period T=0.500s.
Linear speed (v):
v=T2πr=0.500s2π(0.100m)=0.400πm/s=1.2566m/s
- (a) Tension in string (Tstring=Fc):
Tstring=rmv2=0.100m(0.0120kg)(1.2566m/s)2=0.190N
- (b) Effect of doubling speed:
- Because Fc∝v2, doubling the speed (v′=2v) results in:
Fc′=rm(2v)2=4(rmv2)=4Fc
- Thus, tension does not merely double; it increases by a factor of 4.