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.
Inter-particle distances are fixed. No deformation under applied forces.
Pure translation, pure rotation, or combined rolling motion.
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.
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.
x_cm = (m₁x₁ + m₂x₂ + ... + mₙxₙ) / (m₁ + m₂ + ... + mₙ)
r_cm = Σ(mᵢ rᵢ) / M where M = total mass
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 | — |
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.
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.
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.
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.
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:
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.
J = F_ext × Δt = ΔP = M(v_cm,f − v_cm,i)
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.
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.
v₁ = [(m₁ − m₂)/(m₁ + m₂)]u₁ + [2m₂/(m₁ + m₂)]u₂
v₂ = [2m₁/(m₁ + m₂)]u₁ + [(m₂ − m₁)/(m₁ + m₂)]u₂
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 |
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.
v = u + at
s = ut + ½at²
v² = u² + 2as
ω = ω₀ + αt
θ = ω₀t + ½αt²
ω² = ω₀² + 2αθ
Relationship between linear and angular variables for a particle at radius r from axis:
v = rω (tangential speed)
aₜ = rα (tangential acceleration)
aᶜ = rω² = v²/r (centripetal acceleration)
Angular displacement θ must always be in radians (not degrees) when using these kinematic equations. Convert degrees to radians: θ(rad) = θ(°) × π/180.
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.
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 |
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.
Theorems of Moment of Inertia
Two powerful theorems allow calculation of I about any axis if the I about a standard axis is known.
I = I_cm + Md²
I_cm = MOI about axis through COM (parallel to new axis)
d = perpendicular distance between the two axes
I_z = I_x + I_y
Applies only to laminar (2D) bodies.
z-axis is perpendicular to the plane of the body.
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.
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.
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:
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)
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.
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.
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).
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.
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:
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.
Work Done in Rotational Motion
The work–energy theorem extends naturally to rotational systems. Work done by a torque over an angular displacement is:
W = ∫ τ dθ
For constant torque: W = τ × θ
Power: P = τ × ω (analogous to P = F × v)
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).
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.
KE_rot = ½ I ω²
Compare with translational: KE_trans = ½ mv²
Both have the same mathematical structure: ½ × (inertia) × (velocity)²
W_net = ΔKE_rot = ½I(ω_f² − ω_i²)
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.
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 |
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.
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.
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.
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 |
Order of reaching bottom (fastest first):
Solid Sphere > Solid Cylinder > Hollow Sphere > Ring
Smaller I/MR² ratio ⟹ higher bottom speed ⟹ wins the race
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.
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 |
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.
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).
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?
Why does a solid sphere reach the bottom of an incline before a hollow sphere?
How can the centre of mass lie outside the body?
Does friction do work in pure rolling motion?
How is angular momentum conservation applied in the System of Particles and Rotational Motion class 11 notes?
What is the perpendicular axis theorem and when can it be used?
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Table of Contents
Physics — Class 11
| 01 | Units and Measurements | Go to page |
| 02 | Motion in a Straight Line | Go to page |
| 03 | Motion in a Plane | Go to page |
| 04 | Laws of Motion | Go to page |
| 05 | Work, Energy and Power | Go to page |
| 06 | System of Particles and Rotational Motion | Go to page |
| 07 | Gravitation | Go to page |
| 08 | Mechanical Properties of Solids | Go to page |
| 09 | Mechanical Properties of Fluids | Go to page |
| 10 | Thermal Properties of Matter | Go to page |
| 11 | Thermodynamics | Go to page |
| 12 | Kinetic Theory | Go to page |
| 13 | Oscillations | Go to page |
| 14 | Waves | Go to page |
