Mechanics

Kinematics, Newton's laws, work–energy, momentum, collisions, circular motion, SHM, and rigid body rotation.

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Kinematics

  • Position, velocity, and acceleration are related by derivatives: v = dx/dt, a = dv/dt.
  • For constant acceleration: v = u + at, s = ut + ½at², v² = u² + 2as.
  • Projectile motion separates into independent x (uniform) and y (accelerated) components.

v = u + at

s = ut + ½at²

R = v₀² sin(2θ) / g

Newton's Laws & Forces

  • 1st law: inertia — net force zero ⇒ constant velocity.
  • 2nd law: ΣF = ma (vector form).
  • 3rd law: action–reaction pairs act on different bodies.
  • Friction: f ≤ μN (static), f = μₖN (kinetic).

ΣF = ma

f_s ≤ μ_s N

f_k = μ_k N

Work, Energy, Momentum

  • Work by a constant force: W = F·s = Fs cosθ.
  • Kinetic energy KE = ½mv²; work–energy theorem: W_net = ΔKE.
  • Conservative forces → potential energy; mechanical energy conserved if only conservative forces do work.
  • Momentum p = mv is conserved in isolated systems; collisions may be elastic or inelastic.

W = F s cosθ

KE = ½mv²

p = mv

m₁u₁ + m₂u₂ = m₁v₁ + m₂v₂

Circular Motion & SHM

  • Centripetal acceleration a_c = v²/r = ω²r toward center.
  • SHM: restoring force F = −kx; ω = √(k/m); T = 2π√(m/k).
  • Pendulum (small angle): T = 2π√(L/g).

a_c = v²/r

T = 2π√(m/k)

T = 2π√(L/g)

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Quick practice (sample):

Quick quiz

1. A projectile is launched with speed v at angle θ. Max range on flat ground occurs at:

2. In an isolated system, which quantity is always conserved in collisions?

3. Period of a mass-spring SHM system is:

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