System of Particles and Rotational Motion Class 11 Notes

System of Particles and Rotational Motion Class 11 Notes | NEET Physics
01

Introduction to System of Particles

The System of Particles and Rotational Motion class 11 notes begin with a foundational shift in perspective: instead of treating a body as a single point mass, we now consider an extended body as a collection of particles, each obeying Newton’s laws individually. Together, their collective behaviour determines the motion of the entire system. This chapter is one of the most concept-dense and formula-rich chapters in Class 11 Physics, and it carries consistent weight in NEET.

A system of particles is any group of two or more particles whose interactions and collective motion are analyzed as a whole. The particles may be bound together (rigid body) or free (like gas molecules). For NEET, the focus is on rigid bodies — bodies where the distance between any two particles remains constant regardless of the forces applied.

Rigid Body

Inter-particle distances are fixed. No deformation under applied forces.

Types of Motion

Pure translation, pure rotation, or combined rolling motion.

Why This Matters

Unifies force, momentum, energy concepts under one mechanical framework.

Key distinction: in translational motion, every point of the body has the same velocity and acceleration at any instant. In rotational motion, every point moves in a circular path about the axis of rotation, with angular velocity and angular acceleration defining the state of motion.

02

Centre of Mass (COM)

The centre of mass is a uniquely defined point in a system where the entire mass of the system can be assumed concentrated for the purpose of analyzing translational motion. It is not necessarily at the geometric centre; it depends entirely on the mass distribution.

COM for Discrete System
x_cm = (m₁x₁ + m₂x₂ + ... + mₙxₙ) / (m₁ + m₂ + ... + mₙ) r_cm = Σ(mᵢ rᵢ) / M where M = total mass
COM for Continuous Distribution
r_cm = (1/M) ∫ r dm x_cm = (1/M) ∫ x dm , y_cm = (1/M) ∫ y dm

For symmetric uniform bodies, the COM lies at the geometric centre. Key results to memorize:

Body COM Location Notes
Uniform Rod Midpoint (L/2 from either end) Symmetric body
Uniform Disc / Ring Geometric centre COM lies at centre even for hollow ring
Uniform Solid Sphere Geometric centre
Semicircular Ring (radius R) 2R/π from diameter Asymmetric; COM off centre
Semicircular Disc (radius R) 4R/(3π) from diameter Standard NEET result
Solid Hemisphere (radius R) 3R/8 from flat face High NEET frequency
Hollow Hemisphere (radius R) R/2 from flat face
Tip

For a system with a cavity (material removed), use the concept of negative mass. Treat the removed portion as a particle of negative mass at its original COM location and apply the COM formula for the remaining system.

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03

Motion of Centre of Mass

The most powerful result in the study of a system of particles: the centre of mass of a system moves as if all external forces act on a single particle of mass equal to the total mass of the system, located at the COM.

Equation of Motion for COM
F_ext = M × a_cm where a_cm = d²r_cm/dt² and M = total mass of system

Internal forces — forces between particles within the system — always appear in action-reaction pairs and cancel out when summed over the entire system (Newton’s Third Law). They do not affect the motion of the COM; only external forces determine how the COM accelerates.

Warning

In an explosion or collision, even if the object shatters into many pieces, the COM continues on the same parabolic or linear trajectory as before — because no external horizontal force acts. This is a classic NEET trap question.

Practical application: A bomb thrown as a projectile follows a parabolic path. When it explodes mid-air, the fragments scatter in all directions, but the COM of all fragments continues along the original parabola. If one fragment lands at a known position, the other fragment’s landing position can be located using COM principles.

04

Linear Momentum of a System

The total linear momentum of a system of particles is the vector sum of the momenta of all individual particles:

Total Linear Momentum
P = Σ pᵢ = Σ mᵢvᵢ = M × v_cm The total momentum equals total mass times velocity of COM.

Differentiating this with respect to time: dP/dt = F_ext. This is Newton’s second law for a system of particles. When no external force acts, dP/dt = 0, which leads directly to conservation of linear momentum.

Impulse–Momentum Theorem for System
J = F_ext × Δt = ΔP = M(v_cm,f − v_cm,i)
05

Conservation of Linear Momentum

One of the most fundamental principles in physics: if the net external force on a system is zero, the total linear momentum of the system remains constant.

Conservation Condition
F_ext = 0 ⟹ P_total = constant m₁u₁ + m₂u₂ = m₁v₁ + m₂v₂ (for two-particle system)

Critical applications for NEET:

  • Recoil of a gun: Before firing, total momentum = 0. After firing, bullet and gun have equal and opposite momenta. m_gun × v_gun = m_bullet × v_bullet.
  • Rocket propulsion: Exhaust gases ejected backward give the rocket forward momentum. No external force needed — conservation applies within the system.
  • Elastic collision: Both kinetic energy and momentum are conserved. For equal masses, velocities exchange.
  • Perfectly inelastic collision: Momentum conserved; maximum kinetic energy lost. Bodies stick together: (m₁ + m₂)v = m₁u₁ + m₂u₂.
Elastic Collision (1D) — Velocity Formulae
v₁ = [(m₁ − m₂)/(m₁ + m₂)]u₁ + [2m₂/(m₁ + m₂)]u₂ v₂ = [2m₁/(m₁ + m₂)]u₁ + [(m₂ − m₁)/(m₁ + m₂)]u₂
06

Introduction to Rotational Motion

When a rigid body rotates about a fixed axis, every particle moves in a circle. The axis of rotation may pass through the body (spin) or be external (revolution). Understanding rotational motion is central to mastering System of Particles and Rotational Motion class 11 notes for NEET.

Translational Quantity Rotational Analogue Symbol
Displacement (s) Angular displacement θ (radians)
Velocity (v) Angular velocity ω = dθ/dt (rad/s)
Acceleration (a) Angular acceleration α = dω/dt (rad/s²)
Mass (m) Moment of inertia I (kg·m²)
Force (F) Torque τ = r × F (N·m)
Linear momentum (p) Angular momentum L = Iω (kg·m²/s)
Kinetic energy (½mv²) Rotational KE ½Iω²
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07

Angular Variables and Kinematics

The kinematic equations for uniform angular acceleration are exact analogues of the linear kinematic equations. Mastering the parallel structure makes both sets trivially easy.

Linear Kinematics
v = u + at s = ut + ½at² v² = u² + 2as
Rotational Kinematics
ω = ω₀ + αt θ = ω₀t + ½αt² ω² = ω₀² + 2αθ

Relationship between linear and angular variables for a particle at radius r from axis:

Linear–Angular Relationships
v = rω (tangential speed) aₜ = rα (tangential acceleration) aᶜ = rω² = v²/r (centripetal acceleration)
Tip

Angular displacement θ must always be in radians (not degrees) when using these kinematic equations. Convert degrees to radians: θ(rad) = θ(°) × π/180.

08

Moment of Inertia

Moment of inertia (I) is the rotational analogue of mass. It measures a body’s resistance to angular acceleration. Unlike mass, I depends on both the total mass and its distribution relative to the axis of rotation.

Definition
I = Σ mᵢrᵢ² (discrete system) I = ∫ r² dm (continuous body) Unit: kg·m² Dimensional formula: [ML²]

Radius of gyration (K): An equivalent radius at which the entire mass can be concentrated to give the same moment of inertia: I = MK², so K = √(I/M).

Body Axis Moment of Inertia (I)
Thin Ring (mass M, radius R) Through centre, perpendicular to plane MR²
Thin Ring Diameter MR²/2
Solid Disc (mass M, radius R) Through centre, perpendicular MR²/2
Solid Disc Diameter MR²/4
Thin Rod (length L) Through centre, perpendicular to rod ML²/12
Thin Rod (length L) Through one end, perpendicular ML²/3
Solid Sphere (radius R) Through diameter 2MR²/5
Hollow Sphere (radius R) Through diameter 2MR²/3
Solid Cylinder (radius R) Geometric axis MR²/2
Hollow Cylinder (radius R) Geometric axis MR²
Warning

I is not invariant — it changes with the axis chosen. The same disc has I = MR²/2 about its central axis but I = MR²/4 about a diameter. Always specify the axis before quoting a value.

09

Theorems of Moment of Inertia

Two powerful theorems allow calculation of I about any axis if the I about a standard axis is known.

Parallel Axis Theorem
I = I_cm + Md² I_cm = MOI about axis through COM (parallel to new axis) d = perpendicular distance between the two axes
Perpendicular Axis Theorem (Planar Bodies Only)
I_z = I_x + I_y Applies only to laminar (2D) bodies. z-axis is perpendicular to the plane of the body.
Tip

The perpendicular axis theorem is restricted to flat (laminar) objects. Do not apply it to 3D bodies like spheres or cylinders. The parallel axis theorem, however, applies universally to all bodies — 2D or 3D.

Classic NEET application: For a disc, I about diameter = MR²/4. By perpendicular axis theorem, I about central perpendicular axis = I_x + I_y = MR²/4 + MR²/4 = MR²/2. This confirms the standard result.

10

Torque and Angular Momentum

Torque (τ) is the rotational analogue of force. It is the tendency of a force to produce rotation about an axis. Torque depends not just on the magnitude of the force but also on the point of application and direction.

Torque
τ = r × F (vector cross product) |τ| = rF sin θ where θ = angle between r and F τ = I × α (Newton's 2nd law for rotation)

Angular momentum (L) is the rotational analogue of linear momentum:

Angular Momentum
L = r × p = r × mv (for a particle) L = Iω (for a rigid body about fixed axis) τ = dL/dt (analogous to F = dp/dt)
Warning

Torque and angular momentum are both axial vectors (direction given by right-hand rule). In NEET numerical problems, always confirm that the axis of rotation is fixed before applying L = Iω. If the axis changes, the problem is significantly more complex.

11

Conservation of Angular Momentum

When no external torque acts on a system, the total angular momentum remains constant. This is one of the most beautiful and practically significant principles in classical mechanics.

Conservation of Angular Momentum
τ_ext = 0 ⟹ L = Iω = constant I₁ω₁ = I₂ω₂ (before and after any internal change)

Classic applications and NEET examples:

  • Ballet dancer / spinning skater: Pulls arms inward → I decreases → ω increases (spins faster). Extends arms → I increases → ω decreases.
  • Diver tucks in mid-air: Reduces I, increases ω to complete more rotations before hitting water.
  • Collapsing star (pulsar): As a dying star collapses, its radius decreases enormously → I decreases → ω increases dramatically, producing the characteristic rapid spin of neutron stars.
  • Planet in elliptical orbit: Closer to sun (perihelion) → moves faster; farther (aphelion) → moves slower. L = mvr = constant (Kepler’s second law).
12

Rotational Dynamics

Newton’s second law for rotation: The net external torque acting on a rigid body equals the product of its moment of inertia and angular acceleration.

Newton’s 2nd Law (Rotational Form)
τ_net = I × α This is the exact analogue of F_net = ma

When both translational and rotational motions occur simultaneously (e.g., a cylinder rolling down an incline), two equations are written:

Combined Dynamics (e.g., Rolling on Inclined Plane)
Translational: Mg sin θ − f = Ma_cm Rotational: f × R = I × α = I × (a_cm/R) Solving: a_cm = g sin θ / (1 + I/MR²)

This result shows that a solid sphere (I = 2MR²/5) accelerates faster down an incline than a hollow sphere (I = 2MR²/3), which in turn accelerates faster than a ring (I = MR²). The more the mass is concentrated at the rim, the slower the acceleration.

13

Work Done in Rotational Motion

The work–energy theorem extends naturally to rotational systems. Work done by a torque over an angular displacement is:

Work by Torque
W = ∫ τ dθ For constant torque: W = τ × θ Power: P = τ × ω (analogous to P = F × v)
Tip

For NEET problems involving work done against friction torque in rotational motion, apply work-energy theorem directly: Work done by all torques = Change in rotational KE = ½I(ω₂² − ω₁²).

14

Rotational Kinetic Energy

A rotating body possesses kinetic energy by virtue of its rotation, distinct from (and additive to) any translational kinetic energy it may have.

Rotational Kinetic Energy
KE_rot = ½ I ω² Compare with translational: KE_trans = ½ mv² Both have the same mathematical structure: ½ × (inertia) × (velocity)²
Work–Energy Theorem (Rotational)
W_net = ΔKE_rot = ½I(ω_f² − ω_i²)
15

Rolling Motion

Rolling motion is the superposition of pure translation of the COM and pure rotation about the COM. For pure rolling without slipping, there is a crucial constraint linking linear and angular quantities.

Pure Rolling Condition (No Slipping)
v_cm = R × ω (velocity constraint) a_cm = R × α (acceleration constraint) The contact point P has zero instantaneous velocity.

Velocity at different points on a rolling body:

Point on Body Velocity Magnitude
Contact point (bottom) v_cm − Rω Zero (pure rolling)
Centre of mass v_cm (horizontal) v_cm
Top point v_cm + Rω 2v_cm
Warning

The topmost point of a rolling body moves at twice the speed of the centre of mass. This frequently appears in NEET questions as a conceptual trap — students often forget the rotational contribution at the top point.

16

Energy in Rolling Motion

The total mechanical energy of a rolling body is the sum of its translational and rotational kinetic energies. This distinction is critical for inclined plane problems.

Total Kinetic Energy in Rolling
KE_total = KE_trans + KE_rot = ½mv_cm² + ½Iω² = ½mv_cm²(1 + I/mR²) [using v_cm = Rω] = ½mv_cm²(1 + K²/R²) [using I = mK²]
Rolling Body I/MR² KE_rot/KE_total v at bottom (from height h)
Ring / Hollow Cylinder 1 50% √(gh)
Solid Cylinder / Disc 1/2 33% √(4gh/3)
Hollow Sphere 2/3 40% √(6gh/5)
Solid Sphere 2/5 29% √(10gh/7)

The solid sphere reaches the bottom with the highest velocity because the least fraction of energy goes into rotation. The ring is slowest for the same reason in reverse.

17

Numerical Framework

NEET-level numericals in System of Particles and Rotational Motion class 11 notes fall into predictable categories. Here is the solution strategy for each type:

Problem Type Key Equation(s) Watch Out For
Finding COM of composite body r_cm = Σmᵢrᵢ / Σmᵢ Use negative mass for cavities
COM after explosion/collision COM trajectory unchanged (no ext. force) Internal forces do not shift COM
Moment of inertia problems I = Icm + Md² (parallel axis) Choose correct standard I first
Torque and angular acceleration τ = Iα Net torque only; check direction
Conservation of angular momentum I₁ω₁ = I₂ω₂ No external torque condition must hold
Rolling on incline a = g sinθ / (1 + I/MR²) Friction does no work in pure rolling
Rolling energy conservation mgh = ½mv²(1 + K²/R²) Use K²/R² for that specific body
Quick Reference — Inclined Plane Race
Order of reaching bottom (fastest first): Solid Sphere > Solid Cylinder > Hollow Sphere > Ring Smaller I/MR² ratio ⟹ higher bottom speed ⟹ wins the race
18

Conceptual Questions

Conceptual questions in System of Particles and Rotational Motion class 11 notes for NEET test the depth of understanding, not just formula recall. These types appear regularly in the NEET MCQ paper:

  • Can the COM of a body lie outside the body? Yes — hollow ring, horseshoe, donut-shaped body.
  • A body can have angular momentum even without rotating about its own axis — any particle moving in a straight line has angular momentum about a point not on that line (L = mvr).
  • Friction is essential for rolling — without friction, a body would slide, not roll. However, friction does no work during pure rolling.
  • A spinning top exhibits gyroscopic precession — the gravitational torque causes the angular momentum vector to precess, not fall.
  • If a person walks from the rim of a rotating platform toward the centre, the platform speeds up (L conserved, I decreases).
  • Two identical cylinders (solid and hollow) released simultaneously from the top of an identical incline — the solid cylinder always reaches the bottom first, regardless of mass or radius.
19

PYQ Trends

Analysis of previous year NEET questions reveals consistent high-frequency areas within this chapter:

Topic Frequency Type
Very HighMoment of Inertia (standard bodies + theorems) 3–4 questions/year Numerical + Conceptual
HighRolling Motion (energy, velocity at bottom) 2–3 questions/year Numerical
HighConservation of Angular Momentum 1–2 questions/year Conceptual + Numerical
HighTorque and Rotational Dynamics 1–2 questions/year Numerical
ModerateCentre of Mass (COM location, motion) 1 question/year Conceptual
ModerateConservation of Linear Momentum (collisions) 1 question/year Numerical
Tip

NEET PYQ pattern shows that rolling motion questions have appeared every single year since 2010 without exception. Master the I/MR² ratios for all standard bodies and the energy partition formula. This alone can secure 8–12 marks in NEET Physics.

20

Chapter Summary

This chapter builds a unified framework connecting translational and rotational mechanics. Every concept on the translational side has a precise rotational counterpart, and the chapter culminates in rolling motion — where both operate simultaneously.

Quick Revision — Must-Know Points

  • COM of a system: r_cm = Σmᵢrᵢ / M; lies at geometric centre for symmetric uniform bodies.
  • COM moves as if all external forces act on total mass M at that point.
  • Total linear momentum P = Mv_cm; conserved when F_ext = 0.
  • Angular velocity ω = dθ/dt; angular acceleration α = dω/dt; analogues of v and a.
  • Moment of inertia I = Σmᵢrᵢ²; depends on axis chosen. Key values: disc = MR²/2, ring = MR², solid sphere = 2MR²/5.
  • Parallel axis theorem: I = I_cm + Md²; perpendicular axis theorem: I_z = I_x + I_y (laminar bodies only).
  • Torque τ = r × F; Newton’s 2nd law for rotation: τ = Iα.
  • Angular momentum L = Iω; conserved when τ_ext = 0.
  • Rolling without slipping: v_cm = Rω; total KE = ½mv²(1 + K²/R²).
  • Inclined plane race order: solid sphere wins, ring is last.
  • Power in rotational motion: P = τω; work = τθ (constant torque).
21

Common Mistakes

  • Using Perpendicular Axis Theorem for 3D bodies: It applies only to flat (laminar) objects. Applying it to a sphere or cylinder is incorrect.
  • Forgetting the axis when quoting I: Moment of inertia of a disc is MR²/2 only about the central axis perpendicular to its plane. About a diameter, it is MR²/4.
  • Confusing rolling and sliding: Pure rolling means v_cm = Rω exactly. If there is slipping, this constraint does not hold and friction does work.
  • Applying angular momentum conservation incorrectly: External torque must be zero. Gravity can create torque; verify the condition before applying I₁ω₁ = I₂ω₂.
  • Sign errors in torque: Always define a positive direction of rotation. Torques in the positive direction are positive; opposing torques are negative. Sum them algebraically.
  • Using translational KE formula for rolling objects: Rolling objects have BOTH ½mv² AND ½Iω². Omitting the rotational term leads to incorrect energy calculations.
  • COM trajectory after explosion: Students often assume the COM shifts after a mid-air explosion. It does not — in the absence of external horizontal forces, the COM trajectory is unchanged.
  • Radius of gyration vs. radius of body: K (radius of gyration) is defined via I = MK² and is not the physical radius R unless I = MR² (ring/hollow cylinder case).

Frequently Asked Questions — Rotational Motion NEET

What is the difference between moment of inertia and mass in rotational motion? +
Mass is the measure of resistance to linear (translational) acceleration under a net force (F = ma). Moment of inertia (I) is the analogous quantity for rotational motion — it measures resistance to angular acceleration under a net torque (τ = Iα). The key distinction is that while mass is an intrinsic scalar property of a body, moment of inertia depends on both the mass and the distribution of that mass relative to a chosen axis of rotation. The same body has different values of I for different axes.
Why does a solid sphere reach the bottom of an incline before a hollow sphere? +
When rolling down an incline, a portion of the potential energy converts to translational KE and the rest to rotational KE. The fraction going to rotation is I/(I + MR²). A solid sphere has I = 2MR²/5, giving a ratio of 2/7 ≈ 29% to rotation. A hollow sphere has I = 2MR²/3, giving 2/5 = 40% to rotation. Since the solid sphere devotes less energy to spinning, more goes into translational speed — it reaches the bottom faster. This result is independent of mass and radius.
How can the centre of mass lie outside the body? +
The COM is a weighted average of mass positions and is not required to lie within the physical boundaries of the body. For a uniform ring or hollow cylinder, all mass lies at radius R from the centre — the centre itself is empty space, yet that is exactly where the COM is located. Similarly, a boomerang or horseshoe has its COM in the hollow interior region. Any body with a hole or concave shape where mass is absent near the geometric centre can have its COM in empty space.
Does friction do work in pure rolling motion? +
No. In pure rolling without slipping, the contact point between the rolling body and the surface has zero instantaneous velocity. Since the point of application of the static friction force has zero velocity, the work done by friction is zero (W = F × displacement of point of application = 0). However, friction is still essential — it provides the torque necessary to maintain the rolling constraint. Without friction, the body would slide rather than roll.
How is angular momentum conservation applied in the System of Particles and Rotational Motion class 11 notes? +
Angular momentum is conserved when the net external torque on the system is zero. The law states L = Iω = constant in such situations. A classic example is a dancer who spins with arms outstretched (large I, small ω) and then pulls arms in (smaller I). Since Iω must remain constant, ω increases — the dancer spins faster. For NEET, identify that no external torque acts, then write I₁ω₁ = I₂ω₂ and solve for the unknown angular velocity or moment of inertia.
What is the perpendicular axis theorem and when can it be used? +
The perpendicular axis theorem states that for a laminar (flat, 2D) body, the moment of inertia about an axis perpendicular to its plane equals the sum of moments of inertia about two mutually perpendicular axes lying in the plane: I_z = I_x + I_y. This theorem is strictly limited to planar (2D) objects such as discs, rings, rectangular sheets, and triangular plates. It cannot be applied to three-dimensional bodies like spheres, cylinders, or cones.

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Table of Contents — Physics Class 11

Table of Contents

Physics — Class 11

01Units and MeasurementsGo to page
02Motion in a Straight LineGo to page
03Motion in a PlaneGo to page
04Laws of MotionGo to page
05Work, Energy and PowerGo to page
06System of Particles and Rotational MotionGo to page
07GravitationGo to page
08Mechanical Properties of SolidsGo to page
09Mechanical Properties of FluidsGo to page
10Thermal Properties of MatterGo to page
11ThermodynamicsGo to page
12Kinetic TheoryGo to page
13OscillationsGo to page
14WavesGo to page

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