Comprehensive Study Guide & Exam Revision Overview: Work Energy Power - AHC RO/ARO Study Guide

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Work, Energy & Power

Understand the definitions and calculations of work, mechanical energy (kinetic and potential), the work-energy theorem, conservative vs. non-conservative forces, power, and collisions.

Chronological Evolution of Work Energy Power

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Work, Energy & Power Core Study Notes

Thoroughly review the fundamental concepts, calculations, conservation laws, power, and collisions.

1. Work: Scientific Definition & Types

Work is defined as the product of the component of the force in the direction of the displacement and the magnitude of this displacement. Mathematically:

W = F · s · cos(θ)

Where θ is the angle between the Force vector (F) and the Displacement vector (s).

Mass (m) Force (F) Displacement (s) Positive Work (θ < 90°) Mass (m) Normal Force (N) Displacement (s) Zero Work (θ = 90°)
Type of Work Condition (Angle θ) Physical Meaning Example
Positive Work 0° ≤ θ < 90° (cos θ is positive) Force assists the displacement A horse pulling a cart, stretching a spring
Negative Work 90° < θ ≤ 180° (cos θ is negative) Force opposes the displacement Frictional force on a sliding object, brakes stopping a car
Zero Work θ = 90° (cos θ = 0) Force is perpendicular to displacement A coolie walking horizontally with a load on his head

2. Kinetic and Potential Energy

Energy is the quantitative property that must be transferred to a body to perform work on it. Mechanical energy consists of two main types:

Energy Type Definition Formula Key Exam Characteristics
Kinetic Energy (KE) Energy possessed by an object due to its motion. KE = ½mv² = p² / 2m Always positive; depends on frame of reference; related to momentum (p).
Potential Energy (PE) Energy stored in an object due to its position or configuration. PE = mgh (gravitational)
PE = ½kx² (spring)
Can be positive, negative, or zero; defined only for conservative forces.

Relation between Kinetic Energy and Momentum:

If momentum (p) of a body is doubled, its kinetic energy increases by 4 times (since KE ∝ p² for constant mass).

3. Work-Energy Theorem & Conservation of Energy

Work-Energy Theorem: The work done by the net force acting on a particle is equal to the change in its kinetic energy.

Wnet = KEf - KEi = ΔKE

This holds true for both constant and variable forces, as well as conservative and non-conservative forces.

Law of Conservation of Energy: Energy can neither be created nor destroyed; it can only be transformed from one form to another. The total energy of an isolated system remains constant.

For a conservative system (like a free-falling body under gravity):

Total Mechanical Energy (E) = KE + PE = Constant

Height (h) Top: PE = mgh | KE = 0 | Total = mgh Middle (h/2): PE = ½mgh | KE = ½mgh | Total = mgh Bottom: PE = 0 | KE = mgh | Total = mgh

4. Power & Commercial Units of Energy

Power: The rate at which work is done or energy is transferred. Mathematically:

P = W / t = F · v

Where F is the applied force and v is the instantaneous velocity.

  • SI Unit: Watt (W) = 1 Joule/second.
  • Dimensional Formula: [ML²T⁻³]
  • 1 Horsepower (HP) = 746 Watts.

Commercial Unit of Energy:

The standard commercial unit of electrical energy is the Kilowatt-hour (kWh), commonly called a 'Unit'.

1 kWh = 1000 W × 3600 s = 3.6 × 106 J = 3.6 MJ

5. Collisions & Restitution

A collision is a short-duration interaction between two bodies or particles, altering their momentum and energy. Collisions are broadly classified as:

  • Elastic Collision: Both total linear momentum and total kinetic energy are conserved. The colliding bodies separate after impact (e.g., collisions between gas molecules).
  • Inelastic Collision: Linear momentum is conserved, but kinetic energy is not conserved (it converts into heat, sound, etc.).
  • Perfectly Inelastic Collision: The colliding bodies stick together and move with a common velocity after impact (maximum kinetic energy loss).

Coefficient of Restitution (e):

It is the ratio of relative velocity of separation to relative velocity of approach.

e = (v₂ - v₁) / (u₁ - u₂)

  • For perfectly elastic collision: e = 1
  • For perfectly inelastic collision: e = 0
  • For real-world inelastic collision: 0 < e < 1

Practice Zone: 50 Questions

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