📚 Class 11 Physics — Complete Notes

Class 11 Physics Revision Notes

All chapters · Keypoints · Important Formulas · Exam Important Questions
Clean, no-animation format — perfect for last-minute revision

10
Chapters
150+
Key Formulas
80+
Exam Questions
🖨️
Printable
Ch1: Units Ch2: Motion 1D Ch3: Motion Plane Ch4: Laws of Motion Ch5: Work & Energy Ch6: System of Particles Ch7: Gravitation Ch8: Mechanical Properties Ch9: Thermodynamics Ch10: Waves
📏

Chapter 1: Units & Measurements

Physical quantities · SI units · Dimensional analysis · Errors · Significant figures

Chapter 1
🔑 Key Points
  • Physical quantity = something that can be measured. Two types: Fundamental (7) and Derived.
  • 7 Fundamental quantities: Length (m), Mass (kg), Time (s), Temperature (K), Electric current (A), Luminous intensity (cd), Amount of substance (mol).
  • Dimensional formula — expressed in terms of M, L, T, I, θ, J, N. Used to check equation correctness.
  • Principle of homogeneity: Both sides of any valid physical equation must have the same dimensions.
  • Absolute error = |true value − measured value|. Relative error = absolute error / true value. Percentage error = relative error × 100.
  • When quantities are added or subtracted — add absolute errors. When multiplied or divided — add relative errors.
  • Significant figures — all certain digits plus one uncertain. Rules: all non-zero digits significant, zeros between non-zero significant, trailing zeros after decimal significant.
  • Order of magnitude — power of 10 nearest to the number.
📐 Important Dimensional Formulas

Force

[MLT⁻²]

Energy / Work

[ML²T⁻²]

Power

[ML²T⁻³]

Pressure / Stress

[ML⁻¹T⁻²]

Velocity

[LT⁻¹]

Acceleration

[LT⁻²]

Momentum

[MLT⁻¹]

Angular momentum

[ML²T⁻¹]

Torque

[ML²T⁻²]

Surface tension

[MT⁻²]

Viscosity

[ML⁻¹T⁻¹]

Gravitational const G

[M⁻¹L³T⁻²]

🎯 Exam Important Questions — Ch 1
  1. State the principle of homogeneity of dimensions. Using dimensional analysis, derive the formula for time period of a simple pendulum. 3 marks
  2. Check by dimensional method whether the equation v² = u² + 2as is dimensionally correct. 2 marks
  3. The period of oscillation of a simple pendulum depends on length L, mass m and acceleration due to gravity g. Derive an expression for time period using dimensional analysis. 4 marks
  4. Define absolute error, relative error and percentage error with examples. 3 marks
  5. Add 1.234 m and 2.3 m and express result with correct significant figures. 1 mark
  6. Name any 4 pairs of physical quantities that have the same dimensional formula. 2 marks
  7. The resistance R = V/I where V = (100 ± 2)V, I = (10 ± 0.2)A. Find percentage error in R. 3 marks
  8. Convert 1 joule into ergs using dimensional analysis. 2 marks
🚀

Chapter 2: Motion in a Straight Line

Distance · Displacement · Velocity · Acceleration · Equations of motion · Graphs

Chapter 2
🔑 Key Points
  • Distance — total path length. Scalar. Always positive. Displacement — shortest distance from start to end. Vector. Can be negative or zero.
  • Average velocity = total displacement / total time. Average speed = total distance / total time. Average speed ≥ |average velocity|.
  • Instantaneous velocity = dx/dt = slope of position-time (x-t) graph at that instant.
  • Instantaneous acceleration = dv/dt = d²x/dt² = slope of v-t graph.
  • Area under v-t graph = displacement. Area under a-t graph = change in velocity.
  • Equations of motion are valid only for uniform acceleration in a straight line.
  • For free fall: u = 0 (dropped from rest), a = g = 9.8 m/s² (downward). Time to reach ground from height h: t = √(2h/g). Velocity at ground: v = √(2gh).
  • If object thrown upward with velocity u: max height H = u²/2g, time to top = u/g, total time of flight = 2u/g.
  • Distance in nth second: s_n = u + a(2n−1)/2
📐 Equations of Motion

1st Equation

v = u + at

No displacement

2nd Equation

s = ut + ½at²

No final velocity

3rd Equation

v² = u² + 2as

No time

nth Second

sₙ = u + a(2n−1)/2

Distance in nth sec
⭐ Free Fall: Replace a = g, u = 0 (if dropped). Taking downward as +ve: v = gt, h = ½gt², v² = 2gh, t = √(2h/g)
📊 Graph Summary
GraphUniform MotionUniform AccelerationKey Relation
x-t graphStraight line (slope = const v)Parabola (increasing slope)Slope = velocity
v-t graphHorizontal line (a = 0)Straight line (slope = a)Area = displacement
a-t graphLine on x-axis (a = 0)Horizontal line (const a)Area = Δv
🎯 Exam Important Questions — Ch 2
  1. Distinguish between distance and displacement with examples. When is displacement equal to distance? 2 marks
  2. A car starts from rest and accelerates uniformly at 4 m/s². Find (i) velocity after 5s (ii) distance covered in 5s (iii) distance covered in 3rd second. 3 marks
  3. Draw velocity-time graphs for (i) uniform motion (ii) uniform acceleration (iii) uniformly retarded motion. 3 marks
  4. A ball is thrown vertically upward with velocity 20 m/s. Find (i) maximum height (ii) time to reach top (iii) total time of flight. (g = 10 m/s²) 3 marks
  5. Derive the third equation of motion v² = u² + 2as graphically. 4 marks
  6. A stone is dropped from a height of 80 m. Find time to reach the ground and velocity just before hitting the ground. (g = 10 m/s²) 2 marks
  7. Show that distance travelled in nth second by uniformly accelerated body is sₙ = u + a(2n−1)/2. 3 marks
  8. Two cars A and B are at the same point. A moves with constant velocity 30 m/s and B starts from rest with acceleration 3 m/s². When and where will B catch A? 4 marks
✈️

Chapter 3: Motion in a Plane

Scalars & Vectors · Vector Operations · Projectile Motion · Relative Velocity · Circular Motion

Chapter 3
📌 3.1 Scalars and Vectors
Definition Scalar quantity — has only magnitude. e.g. mass, speed, time, temperature, energy, distance.
Vector quantity — has both magnitude and direction. e.g. displacement, velocity, acceleration, force, momentum.
  • Vectors are represented by bold letters or letters with arrow on top: A⃗ or A
  • Equal vectors — same magnitude and same direction.
  • Negative vector — same magnitude, opposite direction. −A⃗
  • Zero (null) vector — magnitude = 0, no specific direction.
  • Unit vector — magnitude = 1, used to indicate direction. â = A⃗/|A⃗|
  • Unit vectors along x, y, z axes: î, ĵ, k̂. |î| = |ĵ| = |k̂| = 1.
  • Position vector r⃗ = xî + yĵ + zk̂ — specifies position of a point from origin.
  • Vectors can be added geometrically (Triangle/Parallelogram law) or analytically (component method).
➕ 3.2 Addition of Vectors
Triangle Law of Vector Addition If two vectors A⃗ and B⃗ are represented by two sides of a triangle taken in order (head to tail), then the third side (closing side, taken in opposite order) represents their resultant R⃗ = A⃗ + B⃗.
Parallelogram Law of Vector Addition If two vectors A⃗ and B⃗ are represented by two adjacent sides of a parallelogram drawn from a common point, then the diagonal of the parallelogram drawn from that point represents their resultant.
Magnitude of Resultant R = √(A² + B² + 2AB cosθ)
where θ = angle between A⃗ and B⃗
Direction of Resultant tan α = B sinθ / (A + B cosθ)
α = angle of R⃗ with A⃗
Angle θ between A⃗ & B⃗Resultant RSpecial Case
θ = 0° (same direction)R = A + BMaximum resultant
θ = 180° (opposite direction)R = |A − B|Minimum resultant
θ = 90° (perpendicular)R = √(A² + B²)Pythagoras case
A = B, θ = 60°R = A√3Equilateral triangle case
A = B, θ = 120°R = AR equals each vector
⭐ Properties of Vector Addition: Commutative — A⃗ + B⃗ = B⃗ + A⃗. Associative — (A⃗ + B⃗) + C⃗ = A⃗ + (B⃗ + C⃗).
🔀 3.3 Resolution of Vectors (Components)
Resolution Breaking a vector into two or more component vectors along chosen directions. The components are its projections along the axes.
Components of a vector A⃗ making angle θ with x-axis Aₓ = A cosθ (x-component)    Aᵧ = A sinθ (y-component)
A⃗ = Aₓî + Aᵧĵ    |A⃗| = √(Aₓ² + Aᵧ²)    θ = tan⁻¹(Aᵧ/Aₓ)
  • To add vectors analytically: Add x-components separately, y-components separately.
  • R⃗ = A⃗ + B⃗ → Rₓ = Aₓ + Bₓ, Rᵧ = Aᵧ + Bᵧ
  • R = √(Rₓ² + Rᵧ²), direction: θ = tan⁻¹(Rᵧ/Rₓ)
  • In 3D: A⃗ = Aₓî + Aᵧĵ + Aᵤk̂, |A⃗| = √(Aₓ² + Aᵧ² + Aᵤ²)
✖️ 3.4 Dot Product & Cross Product

Dot Product (Scalar Product)

A⃗ · B⃗ = AB cosθ

Result is a SCALAR. θ = angle between them.

Cross Product (Vector Product)

|A⃗ × B⃗| = AB sinθ

Result is a VECTOR. Direction by right-hand rule.

Dot Product in components

A⃗·B⃗ = AₓBₓ + AᵧBᵧ + AᵤBᵤ

î·î = ĵ·ĵ = k̂·k̂ = 1, î·ĵ = 0

Cross Product — unit vectors

î×ĵ = k̂, ĵ×k̂ = î, k̂×î = ĵ

î×î = ĵ×ĵ = k̂×k̂ = 0
PropertyDot Product A⃗·B⃗Cross Product A⃗×B⃗
ResultScalarVector
FormulaAB cosθAB sinθ (magnitude)
CommutativeA⃗·B⃗ = B⃗·A⃗ ✓A⃗×B⃗ = −B⃗×A⃗ ✗
If A⃗ ⊥ B⃗ (θ=90°)A⃗·B⃗ = 0|A⃗×B⃗| = AB (max)
If A⃗ ∥ B⃗ (θ=0°)A⃗·B⃗ = AB (max)|A⃗×B⃗| = 0
Physical useWork = F⃗·d⃗, Power = F⃗·v⃗Torque τ⃗ = r⃗×F⃗, L⃗ = r⃗×p⃗
🗺️ 3.5 Motion in a Plane — 2D Kinematics
Key Principle Motion in 2D can be resolved into two independent 1D motions along x and y axes. x and y motions are completely independent of each other.

Position vector

r⃗ = xî + yĵ

Velocity vector

v⃗ = vₓî + vᵧĵ = dr⃗/dt

Acceleration vector

a⃗ = aₓî + aᵧĵ = dv⃗/dt

Average velocity

v⃗_av = Δr⃗/Δt

Equations of Motion in 2D (vector form) v⃗ = u⃗ + a⃗t     s⃗ = u⃗t + ½a⃗t²
x-direction: vₓ = uₓ + aₓt    sₓ = uₓt + ½aₓt²
y-direction: vᵧ = uᵧ + aᵧt    sᵧ = uᵧt + ½aᵧt²
🎯 3.6 Projectile Motion — Complete Notes
Definition A projectile is any object thrown (projected) with an initial velocity and then moving under the influence of gravity alone (no air resistance). Its path is called trajectory — always a PARABOLA.
  • Initial velocity u at angle θ with horizontal → uₓ = u cosθ (horizontal), uᵧ = u sinθ (vertical)
  • Horizontal: No force acts → aₓ = 0 → vₓ = u cosθ = constant throughout
  • Vertical: Gravity acts downward → aᵧ = −g → vᵧ changes with time
  • At highest point: vᵧ = 0, only vₓ remains → velocity = u cosθ (horizontal only)
  • Trajectory equation: y = x tanθ − gx²/(2u²cos²θ) — form y = Ax + Bx² → parabola
🌟 All Projectile Formulas — Must Memorise Time of Flight: T = 2u sinθ / g
Maximum Height: H = u² sin²θ / 2g
Horizontal Range: R = u² sin2θ / g = u² × 2sinθcosθ / g
Maximum Range: R_max = u²/g   (at θ = 45°)
Velocity at time t: vₓ = u cosθ, vᵧ = u sinθ − gt, |v| = √(vₓ² + vᵧ²)
Angle θTime of Flight TMax Height HRange R
30°u/gu²/8gu²√3/2g
45°u√2/gu²/4gu²/g (maximum)
60°u√3/g3u²/8gu²√3/2g
90°2u/gu²/2g0 (straight up)
⭐ Same range for complementary angles: θ and (90°−θ) give the same range. e.g. 30° and 60° → same R. This is because sin2θ = sin2(90°−θ).
⭐ Relation between H and R: R = 4H/tanθ → at θ=45°, R = 4H. Also H_max = R_max/4 (at 45°).
📝 Proof: Trajectory is a Parabola
Derivation Horizontal: x = uₓt = u cosθ · t → t = x/(u cosθ)
Vertical: y = uᵧt − ½gt² = u sinθ · t − ½gt²
Substitute t: y = u sinθ · [x/(u cosθ)] − ½g · [x/(u cosθ)]²
y = x tanθ − gx²/(2u²cos²θ)
This is of the form y = Ax + Bx² → equation of a parabola ✓
🚂 3.7 Relative Velocity in 2D
Definition The velocity of object A as observed from object B is called the velocity of A relative to B.
Relative Velocity Formula v⃗_AB = v⃗_A − v⃗_B   (velocity of A w.r.t. B)
v⃗_BA = v⃗_B − v⃗_A   (velocity of B w.r.t. A)
|v⃗_AB| = |v⃗_BA| but directions are opposite
SituationRelative Speed
Both moving in same direction with speeds v₁, v₂|v₁ − v₂|
Moving in opposite directions with speeds v₁, v₂v₁ + v₂
Moving at angle θ to each other√(v₁² + v₂² − 2v₁v₂cosθ)
⭐ Rain-Man Problem: To protect from rain, umbrella must be tilted at angle α = tan⁻¹(v_man/v_rain) in the direction of walking. The effective relative velocity of rain w.r.t. man determines the angle.
⭐ River-Boat Problem: To cross river of width d, boat speed v_b, river current v_r. Time to cross = d/v_b (independent of current). To cross in minimum time, point boat perpendicular to river bank.
🔵 3.8 Uniform Circular Motion (UCM)
Definition Motion of an object along a circular path with constant speed is called Uniform Circular Motion. Speed is constant but velocity direction changes continuously → acceleration exists.

Angular displacement θ

θ = arc/radius = s/r

Unit: radian

Angular velocity ω

ω = dθ/dt = v/r = 2π/T = 2πn

Unit: rad/s

Linear velocity v

v = rω = 2πr/T = 2πrn

Tangential direction

Time period T

T = 2πr/v = 2π/ω

Time for 1 revolution

Centripetal acceleration

a_c = v²/r = ω²r = vω

Towards centre

Centripetal force

F_c = mv²/r = mω²r

Towards centre
  • In UCM: speed is constant but velocity direction changes → NOT in equilibrium → net force acts (centripetal).
  • Centripetal acceleration is always directed towards the centre, perpendicular to velocity.
  • Centripetal force is not a new type of force — it is provided by existing forces (tension, gravity, friction, normal reaction depending on situation).
  • Centrifugal force — pseudo force in rotating (non-inertial) frame. Equal in magnitude, opposite in direction to centripetal force. It is NOT a real force.
SituationCentripetal Force provided by
Stone on a string (horizontal circle)Tension T in string
Planet orbiting SunGravitational force F = GMm/r²
Car on circular road (flat)Friction between tyre and road
Car on banked roadComponent of Normal force N sinθ
Electron orbiting nucleusElectrostatic attraction (Coulomb force)
📐 Conical Pendulum & Banking of Roads

Conical Pendulum

T = 2π√(L cosθ/g)

L = string length, θ = half-angle with vertical

Banking of Road (no friction)

tan θ = v²/rg
v = √(rg tanθ)

θ = banking angle, v = optimum speed

Max speed on flat road

v_max = √(μrg)

μ = coefficient of friction

Max speed on banked road

v_max = √[rg(tanθ+μ)/(1−μtanθ)]

With friction on banked road
📋 Chapter 3 — Complete Formula Quick Reference
QuantityFormulaUnit
Resultant of two vectorsR = √(A²+B²+2AB cosθ)same as A, B
Direction of resultanttan α = B sinθ/(A+B cosθ)degree/radian
Dot productA⃗·B⃗ = AB cosθscalar
Cross product|A⃗×B⃗| = AB sinθvector
Time of flightT = 2u sinθ/gsecond (s)
Maximum heightH = u²sin²θ/2gmetre (m)
Horizontal rangeR = u²sin2θ/gmetre (m)
Maximum rangeR_max = u²/g at θ=45°metre (m)
Trajectory equationy = x tanθ − gx²/2u²cos²θ—
Angular velocityω = v/r = 2π/T = 2πnrad/s
Centripetal accelerationa = v²/r = ω²rm/s²
Centripetal forceF = mv²/r = mω²rNewton (N)
Relative velocityv⃗_AB = v⃗_A − v⃗_Bm/s
Banking angletan θ = v²/rgdegree
🎯 Exam Important Questions — Chapter 3: Motion in a Plane
  1. State and prove the parallelogram law of vector addition. Derive expression for magnitude and direction of resultant vector. 5 marks
  2. Define scalar and vector quantities. Give 4 examples of each. What are unit vectors? 2 marks
  3. Distinguish between dot product and cross product of two vectors with two examples each. 3 marks
  4. What is a projectile? Prove that the trajectory of a projectile is a parabola. 4 marks
  5. Derive expressions for (i) Time of flight (ii) Maximum height (iii) Horizontal range of a projectile thrown at angle θ with horizontal. 5 marks
  6. Show that the horizontal range is maximum at 45°. Also show that two angles of projection θ and (90°−θ) give the same range. 3 marks
  7. A ball is projected with 40 m/s at 30° above horizontal. Find: (i) time of flight (ii) maximum height (iii) horizontal range. (g = 10 m/s²) 4 marks
  8. Define uniform circular motion. Show that a body in UCM has centripetal acceleration directed towards the centre. Derive a = v²/r. 4 marks
  9. What is centripetal force? Give 3 examples of circular motion and identify the force providing centripetal force in each. 3 marks
  10. Derive the expression for maximum safe speed of a car on a flat circular road. What is the effect of increasing the radius of the road? 3 marks
  11. Explain banking of roads. Derive expression for optimum speed on a banked road (without friction). 4 marks
  12. Define relative velocity. Two trains A and B move at 60 km/h and 80 km/h in the same direction. Find velocity of B relative to A and A relative to B. 2 marks
  13. A particle moves in a circle of radius 2 m with speed 4 m/s. Find (i) angular velocity (ii) time period (iii) centripetal acceleration. 3 marks
  14. A stone is tied to a string of length 1 m and whirled in a horizontal circle at 2 rev/s. Find linear speed, angular velocity and centripetal force if mass = 0.5 kg. 3 marks
  15. Distinguish between centripetal force and centrifugal force. Why is centrifugal force called a pseudo force? 2 marks
⚖️

Chapter 4: Laws of Motion

Newton's 3 Laws · Friction · Tension · Free body diagrams · Conservation of momentum

Chapter 4
🔑 Key Points
  • Newton's 1st Law (Inertia): A body at rest stays at rest; a body in motion stays in uniform motion, unless an external unbalanced force acts. Defines inertia and force.
  • Newton's 2nd Law: F⃗ = dp⃗/dt = ma⃗ (for constant mass). Force ∝ rate of change of momentum. 1 Newton = force that gives 1 kg mass an acceleration of 1 m/s².
  • Newton's 3rd Law: Every action has equal and opposite reaction. Forces act on DIFFERENT bodies — they don't cancel.
  • Inertia ∝ mass. More mass = more inertia = harder to accelerate or stop.
  • Friction: Force opposing relative motion. Static friction ≤ μₛN. Kinetic friction = μₖN. μₛ > μₖ always. Rolling friction < kinetic friction.
  • Limiting friction = maximum static friction = μₛN. Once in motion, kinetic friction applies.
  • Free body diagram (FBD) — shows all forces on a single body. Newton's 2nd law applied to each body separately.
  • Conservation of momentum: If net external force = 0, total momentum = constant. Collision, explosion — use this principle.
📐 Important Formulas

Newton's 2nd Law

F = ma, F = Δp/Δt

Impulse

J = F·Δt = Δp = m(v−u)

Static friction

f_s ≤ μₛN

Kinetic friction

f_k = μₖN

Angle of friction (λ)

tan λ = μ

Atwood machine

a = (m₂−m₁)g/(m₁+m₂)
T = 2m₁m₂g/(m₁+m₂)

Body on incline

a = g(sinθ − μcosθ)
N = mg cosθ

Momentum conservation

m₁u₁ + m₂u₂ = m₁v₁ + m₂v₂

⭐ Pseudo force: In a non-inertial (accelerating) frame, a pseudo force = −ma acts on every object. E.g. lift accelerating upward — apparent weight = m(g+a). Lift falling freely — apparent weight = 0 (weightlessness).
🎯 Exam Important Questions — Ch 4
  1. State and explain Newton's three laws of motion with one example each. 5 marks
  2. Define impulse. Show that impulse = change in momentum. A bat exerts 500 N force on a cricket ball for 0.01 s. Find impulse and change in momentum. 3 marks
  3. Explain the concept of friction. Distinguish between static, kinetic and rolling friction. 3 marks
  4. Two masses 3 kg and 5 kg are connected by a string over a frictionless pulley (Atwood machine). Find acceleration and tension. 4 marks
  5. A 10 kg block is placed on a surface with μ = 0.3. Find force needed to move it and acceleration when 40 N is applied. (g = 10 m/s²) 3 marks
  6. Why does a gun recoil when fired? Explain using conservation of momentum. 2 marks
  7. A person stands on a weighing machine in a lift. What will the scale read when lift (i) moves up with uniform velocity (ii) accelerates up at 2 m/s² (iii) is in free fall? (m = 50 kg, g = 10 m/s²) 3 marks
  8. Derive the expression for acceleration of masses on a smooth inclined plane. 4 marks
⚡

Chapter 5: Work, Energy & Power

Work · Kinetic & Potential energy · Conservation of energy · Collisions · Power

Chapter 5
🔑 Key Points
  • Work = F·s·cosθ. Work is zero if F⊥s (θ=90°). Work can be negative (opposing force). Unit: Joule = N·m.
  • Work-Energy Theorem: Net work done on body = change in KE. W_net = ½mv² − ½mu².
  • Conservative force — work done is path independent (gravity, spring force). Non-conservative — path dependent (friction) — energy lost as heat.
  • Potential energy — stored energy due to position. Gravitational PE = mgh. Spring PE = ½kx².
  • Conservation of energy: Total mechanical energy (KE + PE) is conserved in the absence of non-conservative forces.
  • Power = Work/time = F·v·cosθ. Unit: Watt (W) = J/s. 1 hp = 746 W.
  • Elastic collision: Both momentum AND KE conserved. Inelastic: Only momentum conserved. Perfectly inelastic: Bodies stick together (max KE loss).
  • For elastic collision (equal masses, one at rest): striking ball stops, struck ball moves with striking ball's original velocity.
📐 Key Formulas

Work done

W = F·s·cosθ = F⃗·s⃗

Kinetic Energy

KE = ½mv²

Gravitational PE

PE = mgh

Spring PE

PE = ½kx²

Work-Energy Theorem

W = ΔKE = ½mv² − ½mu²

Power

P = W/t = Fv cosθ

Elastic collision v₁

v₁ = (m₁−m₂)u₁/(m₁+m₂)

Elastic collision v₂

v₂ = 2m₁u₁/(m₁+m₂)

⭐ Variable force: W = ∫F·ds = area under F-x graph. For spring: W = ½kx² (work done in stretching spring by x from natural length).
⭐ Coefficient of Restitution e: e = relative speed of separation / relative speed of approach. Elastic: e=1. Perfectly inelastic: e=0. Any collision: 0 ≤ e ≤ 1.
🎯 Exam Important Questions — Ch 5
  1. State and prove the work-energy theorem. 4 marks
  2. Distinguish between conservative and non-conservative forces with two examples each. 2 marks
  3. A 2 kg body falls freely from height 20 m. Find KE and PE at h = 10 m and h = 0. Verify conservation of energy. (g = 10 m/s²) 4 marks
  4. Derive expressions for final velocities after a head-on elastic collision between two balls. State the special cases. 5 marks
  5. Define power. A machine does 6000 J of work in 2 minutes. Find power in watts and horsepower. 2 marks
  6. A spring of spring constant 200 N/m is compressed by 10 cm. Find elastic PE stored. How much KE does a 0.5 kg mass acquire if released? 3 marks
  7. Show that in a perfectly inelastic collision between two equal masses, KE loss = half the initial KE. 3 marks
  8. What is work done by a porter carrying a load on his head while walking on a horizontal floor? Explain. 2 marks
🔄

Chapter 6: System of Particles & Rotational Motion

Centre of mass · Torque · MI · Angular momentum · Rolling motion

Chapter 6
🔑 Key Points
  • Centre of mass (CM) — the point where entire mass of system can be assumed concentrated. For uniform bodies, CM = geometric centre.
  • CM of two-body system: x_cm = (m₁x₁ + m₂x₂)/(m₁+m₂). CM of system moves as if all external force acts on it.
  • Torque τ = r × F = rF sinθ. Rotational equivalent of force. τ = Iα.
  • Moment of Inertia I = Σmᵢrᵢ² — resistance to rotational motion. Depends on axis and mass distribution.
  • Parallel axis theorem: I = I_cm + Md²
  • Perpendicular axis theorem (lamina only): I_z = I_x + I_y
  • Angular momentum L = Iω = r × p. τ = dL/dt. If τ = 0, L = constant (conservation).
  • Rolling (no slip): v_cm = Rω. Total KE = ½mv² + ½Iω² = ½mv²(1 + I/mR²)
📐 MI Table — Most Important
BodyAxisI
Thin rod (L)Centre ⊥ lengthML²/12
Thin rod (L)End ⊥ lengthML²/3
Disc / Solid cylinder (R)Central axisMR²/2
Disc (R)DiameterMR²/4
Ring / Hoop (R)Central axis ⊥ planeMR²
Ring (R)DiameterMR²/2
Solid sphere (R)Diameter2MR²/5
Hollow sphere (R)Diameter2MR²/3
⭐ Rolling race on incline: Body with smallest I/MR² reaches bottom first. Order: Solid sphere (2/5) → Solid cylinder (1/2) → Hollow sphere (2/3) → Ring (1)
🎯 Exam Important Questions — Ch 6
  1. Define moment of inertia. State its physical significance and write its SI unit and dimensional formula. 2 marks
  2. State and prove the theorem of parallel axes. 4 marks
  3. State and prove the theorem of perpendicular axes. Where is it applicable? 3 marks
  4. Derive an expression for KE of a body rolling without slipping. Show that for a solid sphere KE = 7/10 mv². 4 marks
  5. An ice skater pulls her arms in during a spin. Using conservation of angular momentum, explain why her rotation speeds up. 3 marks
  6. Define centre of mass. Derive its position for a two-particle system. 3 marks
  7. Find the MI of a disc about an axis passing through its diameter using the perpendicular axis theorem. 3 marks
  8. A disc of mass 2 kg and radius 0.5 m rotates at 10 rad/s. Find angular momentum and KE of rotation. 3 marks
🌍

Chapter 7: Gravitation

Newton's law · g · Orbital velocity · Escape velocity · Kepler's laws · Satellites

Chapter 7
🔑 Key Points
  • Newton's Law of Gravitation: F = Gm₁m₂/r². G = 6.67×10⁻¹¹ N·m²/kg². Always attractive. Obeys inverse square law.
  • g at surface: g = GM/R² = 9.8 m/s². g at height h: g' = g(1 − 2h/R) for h << R. Exact: g' = gR²/(R+h)².
  • g decreases with height above surface AND with depth below surface. At centre, g = 0.
  • g at depth d: g' = g(1 − d/R). At centre (d=R): g = 0.
  • Orbital velocity of satellite at height h: v_o = √[GM/(R+h)] = √[g'(R+h)]. For close orbit (h≈0): v_o = √(gR) ≈ 7.9 km/s.
  • Escape velocity: v_e = √(2GM/R) = √(2gR) = √2 × v_o ≈ 11.2 km/s. Does not depend on mass of object.
  • Time period of satellite: T = 2π(R+h)/v_o = 2π√[(R+h)³/GM].
  • Geostationary satellite: T = 24 h, altitude ≈ 36,000 km, moves in equatorial plane from west to east.
📐 Kepler's Laws + Formulas
Kepler's 3 Laws:
1. Law of Orbits: All planets move in elliptical orbits with Sun at one focus.
2. Law of Areas: The line joining planet to Sun sweeps equal areas in equal time intervals (areal velocity = constant → L = constant).
3. Law of Periods: T² ∝ a³ (a = semi-major axis). T²/a³ = constant for all planets around Sun.

Gravitational force

F = Gm₁m₂/r²

g at surface

g = GM/R²

Orbital velocity

v_o = √(GM/r)

Escape velocity

v_e = √(2gR) = √2 v_o

Satellite period

T = 2π√(r³/GM)

Gravitational PE

U = −GMm/r

Binding energy

BE = GMm/2r

Kepler's 3rd Law

T² = (4π²/GM) × r³

🎯 Exam Important Questions — Ch 7
  1. State Newton's law of universal gravitation. Derive expression for acceleration due to gravity g on the surface of Earth. 4 marks
  2. Show that g decreases with altitude. Derive g' = g(1 − 2h/R) for h << R. 3 marks
  3. Show that g decreases with depth. What is g at the centre of Earth? 3 marks
  4. Derive expression for orbital velocity and time period of a satellite. 4 marks
  5. Derive expression for escape velocity from Earth. Why does it not depend on the mass of the projected body? 3 marks
  6. State Kepler's three laws of planetary motion. Derive the third law from Newton's law of gravitation. 5 marks
  7. What is a geostationary satellite? State its four characteristics. Give two applications. 3 marks
  8. The mass of Earth is 6×10²⁴ kg, radius 6400 km. Find (i) g at surface (ii) orbital speed of close satellite (iii) escape speed. (G = 6.67×10⁻¹¹) 4 marks
⚙️

Chapter 8: Mechanical Properties of Solids & Fluids

Stress · Strain · Elastic moduli · Pressure · Bernoulli · Viscosity · Surface tension

Chapter 8
🔑 Key Points — Solids
  • Stress = Restoring force / Area = F/A. Unit: N/m² (Pa). Strain = Change in dimension / Original dimension. Dimensionless.
  • Hooke's Law: Within elastic limit, stress ∝ strain. Stress/Strain = elastic modulus (constant).
  • Young's modulus Y = (F/A)/(ΔL/L) = FL/AΔL. For wires under tension/compression.
  • Bulk modulus K = −P/(ΔV/V). For fluids and all states. Compressibility = 1/K.
  • Rigidity modulus η = (F/A)/(Δx/L). For shear — changes shape not volume.
  • Elastic PE stored in wire = ½ × stress × strain × volume = ½ × Y × (strain)² × volume.
🔑 Key Points — Fluids
  • Pressure = F/A. Fluid pressure at depth h: P = P₀ + ρgh. SI unit: Pascal (Pa).
  • Pascal's Law: Pressure applied to enclosed fluid transmits equally in all directions → Hydraulic press: F₂/F₁ = A₂/A₁.
  • Archimedes' Principle: Buoyant force = weight of fluid displaced = ρ_fluid × V_submerged × g.
  • Bernoulli's Theorem: P + ½ρv² + ρgh = constant. Applies to ideal (non-viscous, incompressible) steady flow.
  • Equation of continuity: A₁v₁ = A₂v₂ (for incompressible fluid). Narrower pipe → faster flow.
  • Torricelli's theorem: Speed of efflux from hole at depth h: v = √(2gh).
  • Viscosity η: F = ηA(dv/dy). Viscosity of liquid decreases with temp. Viscosity of gas increases with temp.
  • Stokes' Law: F = 6πηrv. Terminal velocity: v_t = 2r²(ρ−ρ₀)g/9η.
  • Surface Tension T: T = F/l. Excess pressure in soap bubble = 4T/R. In liquid drop = 2T/R. Capillary rise h = 2T cosθ/ρgr.
🎯 Exam Important Questions — Ch 8
  1. Define stress and strain. State Hooke's Law. Draw and explain the stress-strain curve for a metallic wire. 5 marks
  2. Define Young's modulus, Bulk modulus, and Modulus of Rigidity with formulae and SI units. 3 marks
  3. State and prove Bernoulli's theorem. Mention any two applications. 5 marks
  4. Explain Torricelli's theorem. Derive expression for velocity of efflux. 3 marks
  5. Define terminal velocity. Derive its expression using Stokes' Law. 4 marks
  6. What is surface tension? Derive expression for excess pressure inside a soap bubble and a liquid drop. 4 marks
  7. Derive expression for capillary rise. Why does mercury show capillary depression? 3 marks
  8. A wire of length 2 m and cross-section area 10⁻⁶ m² is stretched by 1 mm. If Y = 2×10¹¹ Pa, find force applied and elastic PE stored. 3 marks
🌡️

Chapter 9: Thermodynamics

Laws of thermodynamics · Heat engines · Specific heat · Thermodynamic processes

Chapter 9
🔑 Key Points
  • Zeroth Law: If A is in thermal equilibrium with B, and B with C, then A is in equilibrium with C. Defines temperature.
  • First Law (Energy conservation): ΔU = Q − W. Q = heat absorbed, W = work done BY system, ΔU = change in internal energy.
  • Isothermal: T = const → ΔU = 0 → Q = W. PV = const. W = nRT ln(V₂/V₁).
  • Isochoric (Isovolumic): V = const → W = 0 → Q = ΔU = nCvΔT.
  • Isobaric: P = const → W = PΔV = nRΔT → Q = nCpΔT.
  • Adiabatic: Q = 0 → ΔU = −W. PV^γ = const. TV^(γ−1) = const.
  • Second Law: Heat cannot flow spontaneously from cold to hot. No engine can be 100% efficient. Entropy of universe always increases.
  • Carnot efficiency: η = 1 − T₂/T₁ (in Kelvin). This is the maximum possible efficiency.
  • Cp − Cv = R (Mayer's relation). γ = Cp/Cv. Monatomic γ = 5/3, Diatomic γ = 7/5.
📐 Process Summary Table
ProcessConditionWQΔU
IsothermalΔT = 0nRT ln(V₂/V₁)= W0
IsochoricΔV = 00nCvΔT= Q
IsobaricΔP = 0nRΔTnCpΔTnCvΔT
AdiabaticQ = 0−nCvΔT0nCvΔT
🎯 Exam Important Questions — Ch 9
  1. State the first law of thermodynamics. Apply it to (i) isothermal (ii) adiabatic processes. 4 marks
  2. State the second law of thermodynamics (both statements). Explain why no heat engine can be 100% efficient. 3 marks
  3. Describe the Carnot cycle with a PV diagram. Derive expression for efficiency of Carnot engine. 5 marks
  4. Derive Mayer's relation Cp − Cv = R. 3 marks
  5. A Carnot engine works between 500 K and 300 K. Find (i) efficiency (ii) heat rejected if heat absorbed is 1000 J. 3 marks
  6. Explain isothermal and adiabatic processes. Compare their PV curves. Which is steeper and why? 3 marks
  7. What is heat engine? Define its efficiency. What does it mean if efficiency = 40%? 2 marks
  8. Calculate work done by 2 moles of ideal gas at 300 K expanding isothermally to double its volume. (R = 8.3 J/mol·K) 3 marks
🌊

Chapter 10: Oscillations & Waves

SHM · Simple pendulum · Speed of sound · Standing waves · Beats · Doppler effect

Chapter 10
🔑 Key Points — SHM & Waves
  • SHM: Motion where restoring force ∝ displacement and directed towards equilibrium. F = −kx. a = −ω²x.
  • Displacement in SHM: x = A sin(ωt + φ). Velocity: v = Aω cos(ωt + φ). Max velocity = Aω at x = 0.
  • Max acceleration = Aω² at extreme positions (x = ±A). Acceleration = 0 at x = 0.
  • Energy in SHM: KE = ½mω²(A²−x²). PE = ½mω²x². Total E = ½mω²A² = constant.
  • Simple pendulum: T = 2π√(L/g). Does not depend on mass or amplitude (for small angles).
  • Spring-mass system: T = 2π√(m/k). ω = √(k/m).
  • Wave equation: y = A sin(kx − ωt). Wave speed v = ω/k = λ/T = λf. k = 2π/λ (wave number).
  • Speed of sound: v = √(B/ρ) (Newton). Laplace correction: v = √(γP/ρ). In air at 0°C: v = 332 m/s. v_t = v₀ + 0.6t.
  • Standing waves: y = 2A cos(kx) sin(ωt). Nodes at kx = nπ (spacing λ/2). Antinodes at kx = (2n+1)π/2.
  • Beats: n_beats = |n₁ − n₂|. Heard when two close frequencies superpose.
  • Doppler effect: Apparent frequency changes when source or observer moves.
📐 Key Formulas

SHM period

T = 2π/ω = 2π√(m/k)

Pendulum period

T = 2π√(L/g)

Max velocity

v_max = Aω

Total energy SHM

E = ½mω²A² = ½kA²

Wave speed

v = fλ = ω/k

Speed of sound

v = √(γP/ρ) = √(γRT/M)

Beats

n_b = |n₁ − n₂|

Doppler (source moving)

n' = n(v ± v_o)/(v ∓ v_s)

⭐ Organ pipe: Open pipe — L = nλ/2, harmonics n = 1,2,3... Closed pipe — L = (2n−1)λ/4, only ODD harmonics.
⭐ Doppler sign convention: Numerator: + if observer moves towards source, − if away. Denominator: − if source moves towards observer, + if away.
🎯 Exam Important Questions — Ch 10
  1. Define SHM. Show that the motion of a particle attached to a spring is SHM. Derive expression for time period. 5 marks
  2. Derive expression for time period of a simple pendulum. Why does it not depend on mass or amplitude? 4 marks
  3. Show that total energy in SHM is constant. Draw graphs of KE, PE and total energy vs displacement. 4 marks
  4. Explain the formation of standing waves. Differentiate between nodes and antinodes. 3 marks
  5. Derive an expression for speed of sound in a gas. What is Laplace's correction and why is it needed? 4 marks
  6. What are beats? How are they produced? Give one practical application. 2 marks
  7. State and explain Doppler effect. Derive expression for apparent frequency when source moves towards stationary observer. 4 marks
  8. A tuning fork of 256 Hz produces 4 beats/s with a wire. The wire is tightened and beats drop to 2/s. Find original frequency of wire. 3 marks
📋

Master Formula Sheet — Class 11 Physics

All important formulas at a glance — for last-minute revision

⭐ Must-Know Formulas (Exam Focused)
TopicFormulaSymbol meaning
Equations of Motionv=u+at, s=ut+½at², v²=u²+2as, sₙ=u+a(2n−1)/2u=initial, v=final, a=acceleration
Projectile RangeR = u²sin2θ/g, H = u²sin²θ/2g, T = 2usinθ/gu=speed, θ=angle, g=gravity
Newton's 2nd LawF = ma = Δp/Δtp = momentum = mv
Frictionf_s ≤ μₛN, f_k = μₖNN = normal force
Work-EnergyW = Fscosθ, W = ΔKE = ½mv² − ½mu²—
PowerP = W/t = Fvcosθ—
Torque & MIτ = rFsinθ = Iα, L = Iω, τ = dL/dtI = moment of inertia
GravitationF = Gm₁m₂/r², g = GM/R², v_e = √(2gR)G = 6.67×10⁻¹¹
Orbital velocityv_o = √(GM/r), T = 2π√(r³/GM)r = orbital radius
Young's ModulusY = FL/AΔLΔL = elongation
Bernoulli'sP + ½ρv² + ρgh = constρ = density
Carnot Efficiencyη = 1 − T₂/T₁T in Kelvin
First Law ThermoΔU = Q − WQ absorbed, W by system
SHMT = 2π√(m/k), T = 2π√(L/g), E = ½kA²k = spring constant
Wave speedv = fλ = √(γP/ρ)λ = wavelength
Surface TensionΔP_bubble = 4T/R, ΔP_drop = 2T/R, h = 2Tcosθ/ρgrT = surface tension
⚠️ Common Mistakes to Avoid
  • Equations of motion — Valid ONLY for uniform acceleration. Don't apply if acceleration changes.
  • Projectile — Horizontal velocity is CONSTANT. Only vertical component changes. At top, vy = 0 but vx ≠ 0.
  • Newton's 3rd Law — Action and reaction act on DIFFERENT bodies. They CANNOT cancel each other.
  • Carnot efficiency — Use KELVIN temperature, NOT Celsius.
  • Isothermal vs Adiabatic — Isothermal: ΔU = 0 (NOT Q = 0). Adiabatic: Q = 0 (NOT ΔU = 0).
  • Soap bubble vs drop — Bubble has 2 surfaces: 4T/R. Drop has 1 surface: 2T/R.
  • MI — Parallel axis theorem: I = I_cm + Md² (d from CM, NOT from any axis). Perpendicular axis theorem only for FLAT LAMINA.
  • Escape velocity — Does NOT depend on mass of the projected object. v_e = √2 × v_o.
  • Work done by friction — Always negative (opposes motion). Not zero on horizontal surface.
  • g at depth d — g' = g(1 − d/R). At centre g = 0. Don't use g' = gR²/(R+d) for depth.