4.1 Applied Mechanics
4.1 Applied Mechanics
1. Particles, Rigid and Deformable Bodies
Particle:
Mass concentrated at a point.
No dimensions (idealization).
Only translational motion considered.
Rigid Body:
Collection of particles with fixed distances.
No deformation under applied loads.
Both translational and rotational motion.
Deformable Body:
Particles can move relative to each other.
Changes shape under load.
Studied in Strength of Materials/Solid Mechanics.
2. Statics and Equilibrium
Statics: Study of bodies at rest or moving with constant velocity.
Equilibrium Conditions:
For a particle: Sum of all forces = zero. ∑F=0
For a rigid body:
Sum of forces = zero: ∑F=0
Sum of moments about any point = zero: ∑M=0
Free Body Diagram (FBD):
Essential tool showing all external forces acting on a body.
Isolate the body from its surroundings.
Support Reactions:
Roller: Single reaction force perpendicular to surface.
Pin/Hinge: Two reaction forces (horizontal and vertical).
Fixed Support: Two forces + one moment reaction.
3. Friction
Dry Friction (Coulomb Friction):
Occurs between dry surfaces in contact.
Opposes impending or actual relative motion.
Friction Forces:
Static Friction (fs): Acts before motion starts.
fs≤μsN where μs = coefficient of static friction.
Kinetic Friction (fk): Acts during motion.
fk=μkN where μk = coefficient of kinetic friction.
Characteristics:
μs>μk (static > kinetic).
Friction force depends on normal force, not contact area.
Angle of Friction (ϕ): tanϕ=μ.
Applications:
Wedges, belts, screws, brakes.
Limiting friction condition used in equilibrium analysis.
4. Newton's Laws
First Law (Inertia):
Body remains at rest or uniform motion unless acted upon by external force.
Defines inertial reference frames.
Second Law (Force-Acceleration):
∑F=ma
Force produces acceleration proportional to mass.
Valid in inertial frames.
Third Law (Action-Reaction):
For every action, equal and opposite reaction.
Forces always occur in pairs between interacting bodies.
5. Work–Energy Theorem
Work Done by a Force:
W=F⋅s=Fscosθ
Scalar quantity (Joules).
Kinetic Energy (KE):
Energy due to motion: KE=21mv2
Work–Energy Theorem:
Net work done = change in kinetic energy.
Wnet=ΔKE=21mv22−21mv12
Conservative Forces:
Work independent of path (gravity, spring).
Potential energy (PE) can be defined.
Conservation of Mechanical Energy:
With only conservative forces: KE1+PE1=KE2+PE2
6. Impulse–Momentum Principle
Linear Momentum:
p=mv
Vector quantity in direction of velocity.
Impulse:
J=∫Fdt
Also: J=FavgΔt
Impulse–Momentum Principle:
Impulse = change in momentum.
J=Δp=mv2−mv1
Conservation of Linear Momentum:
If net external force = 0, total momentum is constant.
∑mvinitial=∑mvfinal
Applications:
Impact/collision problems.
Variable force analysis.
Rocket propulsion.
Coefficient of Restitution (e):
e=u1−u2v2−v1 (relative velocities).
e=1: Perfectly elastic (KE conserved).
e=0: Perfectly plastic (maximum KE loss).
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