NEET Physics · NCERT Class 11

Work, Energy and Power notes

Work & Work-Energy Theorem, Kinetic & Potential Energy, Variable Force & Conservative Forces, Conservation of Mechanical Energy, Spring Potential Energy & Power and Collisions — explained topic by topic with key points, formulas, memory tricks and common mistakes.

  • 7 topics
  • 66 min read
  • 34 formulas
  • 26 PYQs
1

Chapter Overview

7 min

Work, Energy and Power connects force with motion using energy methods. Work is done when a force causes displacement, and it depends on the component of force along displacement. Energy is the capacity to do work and appears as kinetic energy, potential energy, spring energy, heat and other forms. The work-energy theorem states that net work done on a body equals change in kinetic energy. Conservation laws help solve problems quickly when forces are conservative and mechanical energy remains constant. Power measures the rate of doing work, while efficiency compares useful output to input. For NEET, this chapter is very important because it simplifies motion, spring, collision and conservation problems.

Key points6

  • Work is a scalar, but it may be positive, negative or zero.
  • Energy and work have the same SI unit: joule.
  • Work-energy theorem is valid for both conservative and non-conservative forces.
  • Mechanical energy is conserved only when non-conservative work is zero.
  • Area under force-displacement graph gives work done.
  • In collisions, momentum is conserved if external impulse is negligible, but kinetic energy is conserved only in elastic collisions.

Memory tricks2

Work Sign: Force with motion is positive work; force against motion is negative work; force perpendicular to motion is zero work.

Energy Method: When forces vary or path is curved, think energy before equations of motion.

Examples2

Daily Life Example

A motor lifts water by doing work against gravity, converting electrical energy into gravitational potential energy.

NEET Quick Check

If a force of 10 N acts perpendicular to displacement 5 m, work done is 10 × 5 × cos90° = 0.

Common mistakes3

Confusing Work and Force

A force can act without doing work if displacement is zero or perpendicular to force.

Assuming Mechanical Energy Always Conserved

Mechanical energy is conserved only when non-conservative work, such as frictional work, is zero.

Ignoring Units

Work and energy are in joule; power is in watt.

Reference tables2

Quick revision8

Formulas4

Work Done by Constant Force
W= Fs cosθW =\text{ Fs cos}θ

Work done is the product of force, displacement and cosine of the angle between them.

W
Work done
F
Magnitude of force
s
Displacement
θ
Angle between force and displacement
Work-Energy Theorem
Wnet=ΔK=Kf−KiW_{net} = ΔK = K_f - K_i

Net work done by all forces equals change in kinetic energy.

W_net
Net work done
K_f
Final kinetic energy
K_i
Initial kinetic energy
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2

Work & Work-Energy Theorem

9 min

Work is done when a force produces displacement of its point of application. For a constant force, work is W = Fs cosθ, where θ is the angle between force and displacement. Work is positive when force helps motion, negative when force opposes motion and zero when force is perpendicular to displacement or displacement is zero. For variable force, work is found by adding small works and equals area under the force-displacement graph. When multiple forces act, net work is the sum of work done by all forces or work done by the resultant force. The work-energy theorem states that net work done on a particle equals change in kinetic energy.

Key points6

  • Normal reaction does zero work on a block moving horizontally on a fixed surface.
  • Friction usually does negative work during sliding.
  • Centripetal force does zero work in uniform circular motion because it is perpendicular to displacement.
  • Work done by multiple forces can be calculated separately and added.
  • Work-energy theorem uses net work, not work by only one force unless specified.
  • The theorem is valid even when forces are variable.

Memory tricks2

Work Sign Shortcut: Along = plus, against = minus, perpendicular = zero.

Work-Energy Theorem: Net work is the energy bill: it tells exactly how kinetic energy changes.

Examples3

Solved NEET Example

A 2 kg body speeds up from 3 m/s to 5 m/s. Net work = 1/2×2×(25 - 9) = 16 J.

Constant Force Example

A 20 N force pulls a block through 4 m at 60 degrees. Work = 20×4×cos60 = 40 J.

Stopping Example

If friction does -100 J work on a moving object, its kinetic energy decreases by 100 J.

Common mistakes3

Using Distance Instead of Displacement Direction

Work depends on displacement direction and the angle between force and displacement.

Taking Normal Work as Non-Zero

For a block moving on a fixed horizontal surface, normal is perpendicular to displacement, so its work is zero.

Using One Force Instead of Net Work

Work-energy theorem requires total work done by all forces.

Reference tables2

Quick revision8

Formulas4

Work by Constant Force
W=F⋅s= Fs cosθW = F · s =\text{ Fs cos}θ

Work is the dot product of force and displacement.

W
Work done
F
Force magnitude
s
Displacement magnitude
θ
Angle between force and displacement
Work by Variable Force
W=∫F(x)dxW = ∫ F(x) dx

Work done by a variable force along x-direction is the area under F-x curve.

F(x)
Force as a function of position
dx
Small displacement
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3

Kinetic & Potential Energy

10 min

Kinetic energy is the energy possessed by a body due to motion. For translational motion, K = 1/2 mv², so it depends on mass and square of speed. It is also related to momentum by K = p²/2m. Work done by net force changes kinetic energy. Potential energy is energy stored because of position or configuration. Near Earth’s surface, gravitational potential energy is U = mgh relative to a chosen reference level. More generally, gravitational potential energy is negative and depends on separation from Earth or another mass. Mechanical energy is the sum of kinetic and potential energies. Many problems involve conversion between kinetic and potential energy.

Key points6

  • Doubling speed makes kinetic energy four times.
  • Potential energy depends on the selected zero level, but change in potential energy is physically meaningful.
  • General gravitational potential energy is U = -GMm/r.
  • Near Earth approximation mgh is valid when height is small compared to Earth’s radius.
  • Mechanical energy may remain constant even though kinetic and potential energy individually change.
  • Energy is scalar, so signs come from reference choices and work relations, not direction like vectors.

Memory tricks2

Kinetic Energy Speed Rule: Speed double means kinetic energy four times.

Potential Energy Reference: PE is like altitude on a map: zero level is chosen, but height difference matters.

Examples3

Kinetic Energy Example

A 2 kg body moving at 5 m/s has K = 1/2×2×25 = 25 J.

Momentum Relation Example

A body with momentum 10 kg m/s and mass 2 kg has K = p²/2m = 100/4 = 25 J.

Potential Energy Example

A 3 kg mass raised by 4 m gains U = mgh = 3×10×4 = 120 J.

Common mistakes3

Forgetting Square in Kinetic Energy

Kinetic energy depends on v², so small speed changes strongly affect energy.

Treating Potential Energy as Absolute

Only change in potential energy is physically important in most mechanics problems.

Using Velocity Direction in Kinetic Energy

Kinetic energy depends on speed, not direction, so it is never negative.

Reference tables2

Quick revision8

Formulas6

Translational Kinetic Energy
K=(1/2)mv2K = (1/2)mv²

Energy possessed by a body due to translational motion.

K
Kinetic energy
m
Mass
v
Speed
Kinetic Energy and Momentum
K=p2/(2m)K = p²/(2m)

Relates kinetic energy to linear momentum.

p
Linear momentum
m
Mass
Work-Kinetic Energy Relation
Wnet=ΔKW_{net} = ΔK

Net work done on a body changes its kinetic energy.

W_net
Net work
ΔK
Change in kinetic energy
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4

Variable Force & Conservative Forces

9 min

A variable force changes in magnitude or direction during motion. Its work cannot generally be calculated by simple W = Fs cosθ; instead, the displacement is divided into small parts and work is integrated. Graphically, work done by a force along a line is the area under the force-displacement graph. Conservative forces are special forces for which work depends only on initial and final positions, not on path. Gravity and spring force are common examples. For conservative forces, work done equals negative change in potential energy. Non-conservative forces, such as friction and air resistance, depend on path and usually convert mechanical energy into heat.

Key points6

  • Constant force work is a special case of variable force work.
  • If F-x graph is below the x-axis, work contribution is negative.
  • Potential energy can be defined only for conservative forces.
  • Gravity does the same work between two heights regardless of path.
  • Friction does more negative work for longer path length.
  • Spring force is variable and conservative.

Memory tricks2

Conservative Force: Conservative cares about endpoints, not route.

F-x Graph: Work is the area story under the force-displacement curve.

Examples2

Graph Work Example

If force increases linearly from 0 to 10 N over 4 m, work = area of triangle = 1/2×4×10 = 20 J.

Conservative Work Example

A 2 kg body falls 5 m. Work by gravity = mgh = 2×10×5 = 100 J, independent of path.

Common mistakes3

Using W = Fs for Every Force

W = Fs applies directly only for constant force parallel to displacement.

Ignoring Negative Area

Area below the displacement axis represents negative work.

Calling Friction Conservative

Frictional work depends on path length, so friction is non-conservative.

Reference tables2

Quick revision8

Formulas4

Variable Force Work
W=∫ from x1tox2F(x)dxW = ∫\text{ from }x1 to x2 F(x) dx

Work done by a one-dimensional variable force equals area under the F-x curve.

W
Work done
F(x)
Force as a function of position
x1, x2
Initial and final positions
Work and Potential Energy
Wconservative=−ΔUW_{\text{conservative}} = -ΔU

Work done by a conservative force equals decrease in potential energy.

W_conservative
Work done by conservative force
ΔU
Change in potential energy
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5

Conservation of Mechanical Energy

10 min

The law of conservation of energy states that energy can neither be created nor destroyed; it only transforms from one form to another. In mechanics, if only conservative forces such as gravity or spring force do work, total mechanical energy remains constant. Thus K + U at one point equals K + U at another point. This principle solves free fall, smooth inclined plane, pendulum and roller coaster problems without directly using acceleration equations. In free fall, gravitational potential energy converts into kinetic energy. On a smooth incline, loss of height decides speed, not the path length. In a pendulum, energy exchanges between kinetic and potential forms during swing.

Key points6

  • Mechanical energy conservation is easier than Newton’s laws when normal force does no work.
  • Mass cancels in many gravitational energy problems.
  • The reference level of potential energy can be chosen conveniently.
  • At the highest point of a pendulum, speed is minimum; at the lowest point, speed is maximum.
  • For smooth tracks, final speed depends only on change in height.
  • If non-conservative work is present, use K_i + U_i + W_nc = K_f + U_f.

Memory tricks2

Smooth Track Rule: No friction means height decides speed.

Energy Conservation Setup: Write initial K + U on left, final K + U on right, then cancel common terms.

Examples3

Free Fall Example

A body falls from rest through 20 m. v = √(2×10×20) = 20 m/s.

Inclined Plane Example

A block slides down a smooth incline losing height 5 m. Speed at bottom = √(2×10×5) = 10 m/s.

Pendulum Example

If a pendulum bob drops vertically by 0.2 m, its speed at lowest point is √(2×10×0.2) = 2 m/s.

Common mistakes3

Using Path Length Instead of Height

For gravitational potential energy, use vertical height change, not distance along path.

Forgetting Friction Work

If friction acts, mechanical energy is not conserved; include W_nc.

Assuming Normal Does Work on Smooth Track

On a fixed smooth track, normal is perpendicular to instantaneous displacement, so it does no work.

Reference tables2

Quick revision8

Formulas4

Conservation of Mechanical Energy
Ki+Ui=Kf+UfK_i + U_i = K_f + U_f

Valid when only conservative forces do work.

K_i, K_f
Initial and final kinetic energies
U_i, U_f
Initial and final potential energies
Mechanical Energy with Non-Conservative Work
Ki+Ui+Wnc=Kf+UfK_i + U_i + W_{nc} = K_f + U_f

Use when friction, air resistance or other non-conservative forces do work.

W_nc
Work done by non-conservative forces
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6

Spring Potential Energy & Power

11 min

A spring stores energy when stretched or compressed. For an ideal spring, Hooke’s law gives F = -kx, where k is the spring constant and x is displacement from natural length. The elastic potential energy stored is U = 1/2 kx². This energy can convert into kinetic energy when the spring is released. Springs connected in series become softer, while springs in parallel become stiffer. Power measures how fast work is done or energy is transferred. Average power is total work divided by total time, while instantaneous power is the rate at a particular instant and can be written as P = F · v. Efficiency measures useful output compared with input.

Key points7

  • The negative sign in Hooke’s law shows restoring direction.
  • Spring energy depends on x², so compression and extension store positive energy.
  • A stiffer spring has larger spring constant k.
  • In series, extension is shared and equivalent spring constant decreases.
  • In parallel, forces add and equivalent spring constant increases.
  • One horsepower is approximately 746 W.
  • Efficiency is always less than or equal to 100% for real machines.

Memory tricks3

Spring Energy: Spring energy is half k x-square: half, stiffness, deformation squared.

Power: Power tells how fast energy is spent or work is done.

Efficiency: Efficiency asks: useful out of total in.

Examples3

Spring Energy Example

A spring of k = 200 N/m compressed by 0.1 m stores U = 1/2×200×0.01 = 1 J.

Power Example

A machine does 500 J work in 10 s. Average power = 500/10 = 50 W.

Efficiency Example

If a motor takes 1000 W input and gives 750 W useful output, efficiency = 75%.

Common mistakes3

Forgetting Half in Spring Energy

Spring energy is 1/2 kx², not kx².

Confusing Spring Force and Spring Energy

Force is proportional to x, but energy is proportional to x².

Using Average Power as Instantaneous Power

Average power is total work over total time; instantaneous power is F · v at that instant.

Reference tables2

Quick revision8

Formulas7

Hooke’s Law
F=−kxF = -kx

Restoring force of an ideal spring is proportional and opposite to displacement.

F
Spring force
k
Spring constant
x
Extension or compression
Elastic Potential Energy
U=(1/2)kx2U = (1/2)kx²

Energy stored in a spring stretched or compressed by x.

U
Spring potential energy
k
Spring constant
x
Deformation from natural length
Springs in Series
1/keq=1/k1+1/k21/k_{eq} = 1/k1 + 1/k2

Equivalent spring constant for two springs connected end-to-end.

k_eq
Equivalent spring constant
k1, k2
Individual spring constants
Springs in Parallel
keq=k1+k2k_{eq} = k1 + k2

Equivalent spring constant for two springs supporting the same displacement.

k_eq
Equivalent spring constant
k1, k2
Individual spring constants
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7

Collisions

10 min

A collision is a short-duration interaction between bodies during which internal forces are very large compared with external forces. Therefore, total linear momentum of the system is conserved if external impulse is negligible. Kinetic energy may or may not be conserved. In an elastic collision, both momentum and kinetic energy are conserved. In an inelastic collision, momentum is conserved but kinetic energy decreases, usually converting into heat, sound or deformation. In a perfectly inelastic collision, bodies stick together. The coefficient of restitution measures how elastic a collision is and is the ratio of relative speed of separation to relative speed of approach. One-dimensional collisions are common NEET problems.

Key points6

  • Momentum conservation is vector conservation; direction matters.
  • Kinetic energy lost in inelastic collision becomes heat, sound or deformation.
  • For a system of colliding bodies, internal collision forces cancel in total momentum equation.
  • External impulse must be negligible for momentum conservation during collision.
  • In one dimension, assign positive direction before writing equations.
  • NEET often combines conservation of momentum with coefficient of restitution.

Memory tricks3

Collision Conservation: Momentum is mandatory; kinetic energy is special.

Coefficient of Restitution: e compares separation after to approach before.

Perfectly Inelastic: Inelastic plus stick together means one common final velocity.

Examples3

Perfectly Inelastic Example

A 2 kg mass moving at 6 m/s sticks to a 4 kg mass at rest. Final velocity = (2×6)/(2+4) = 2 m/s.

Elastic Equal Mass Shortcut

In a head-on elastic collision of equal masses where one is initially at rest, the first mass stops and the second moves with the first mass’s initial velocity.

Coefficient of Restitution Example

If approach speed is 10 m/s and separation speed is 6 m/s, e = 6/10 = 0.6.

Common mistakes4

Conserving Kinetic Energy in Every Collision

Kinetic energy is conserved only in elastic collisions, not in all collisions.

Ignoring Velocity Signs

In one-dimensional collisions, velocities in opposite directions must have opposite signs.

Using Momentum Conservation with Large External Impulse

Momentum conservation requires external impulse to be zero or negligible during collision.

Wrong Restitution Order

Use relative speed of separation divided by relative speed of approach, with correct signs.

Reference tables3

Quick revision8

Formulas5

Momentum Conservation in 1D
m1u1+m2u2=m1v1+m2v2m1u1 + m2u2 = m1v1 + m2v2

Total momentum before collision equals total momentum after collision.

m1, m2
Masses of colliding bodies
u1, u2
Initial velocities
v1, v2
Final velocities
Kinetic Energy Conservation in Elastic Collision
1/2m1u12+1/2m2u22=1/2m1v12+1/2m2v221/2 m1u1² + 1/2 m2u2² = 1/2 m1v1² + 1/2 m2v2²

In an elastic collision, total kinetic energy remains constant.

u1, u2
Velocities before collision
v1, v2
Velocities after collision
Coefficient of Restitution
e=(v2−v1)/(u1−u2)e = (v2 - v1)/(u1 - u2)

For 1D collision with body 1 approaching body 2, e is relative speed of separation divided by relative speed of approach.

e
Coefficient of restitution
u1 - u2
Relative speed of approach
v2 - v1
Relative speed of separation
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NEET PYQs from Work, Energy and Power

The latest 3 of 26 previous-year questions from this chapter.

  1. NEET 2026Set 50MediumQ1

    A particle of mass $M$ moves along a horizontal $x$ axis from $x = 0$ to $x = L$. The coefficient of kinetic friction varies as a function of $x$ as $\mu_k(x) = \mu_0 - \alpha x$, where $\mu_0$, $\alpha$ are constants of appropriate dimensions, so that $\mu_k(L) = 0$. The total work done by the frictional force during the motion is $n\mu_0 MgL$, where $g$ is the acceleration due to gravity. The value of $n$ is:

    • A$3$
    • B$1$
    • C$\frac{1}{3}$
    • D$\frac{1}{2}$
  2. NEET 2026Set 11EasyQ2

    The power of a crane, which lifts a mass of 1000 kg to a height of 20 m in 10 s is: (g = 9.8 m/s²)

    • A19.6 W
    • B39.2 W
    • C19.6 kW
    • D39.2 kW
  3. NEET 2026Set 50EasyQ3

    Bob $B$ of mass $m$ at rest is hanging vertically from the ceiling via a massless string of length $10\ \mathrm{m}$, as shown in the figure. Point mass $A$ of mass $m$ travelling horizontally with speed $10\ \mathrm{ms^{-1}}$ hits bob $B$ elastically. The bob $B$ rises $h$ meter after the collision. Taking the acceleration due to gravity $g = 10\ \mathrm{ms^{-2}}$ and neglecting the size of the bob, the value of $h$ is:

    • A$8$
    • B$7$
    • C$5$
    • D$2.5$

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