In short: CBSE Class 11 Physics has 15 chapters with roughly 150+ formulas. This is the complete chapter-wise list with SI units for every quantity. Class 11 Physics is the foundation for Class 12 boards, JEE Main, and NEET. Every formula here will be used directly or indirectly in your board exam year. Bookmark, print, and revise one chapter per day.
Chapter 1: Units and Measurements
| Formula | Expression | SI Unit |
|---|---|---|
| Dimensional formula | [M^a L^b T^c] | — |
| Percentage error | (Δa/a) × 100 | % |
| Absolute error | Δa = | a − a_mean |
| Relative error | Δa/a | Dimensionless |
| Addition/subtraction error | Δz = Δa + Δb | Absolute errors add |
| Multiplication/division error | Δz/z = Δa/a + Δb/b | Relative errors add |
| Power rule error | If z = aᵐbⁿ, then Δz/z = m(Δa/a) + n(Δb/b) | — |
Chapter 2: Motion in a Straight Line
| Formula | Expression | SI Unit |
|---|---|---|
| Average speed | v_avg = total distance / total time | m/s |
| Average velocity | v⃗_avg = displacement / time | m/s |
| Instantaneous velocity | v = ds/dt | m/s |
| Average acceleration | a = (v − u)/t | m/s² |
| 1st equation of motion | v = u + at | m/s |
| 2nd equation of motion | s = ut + ½at² | m |
| 3rd equation of motion | v² = u² + 2as | m²/s² |
| Distance in nth second | sₙ = u + a(2n−1)/2 | m |
| Free fall | g = 9.8 m/s²; equations same with a = g | m/s² |
| Relative velocity | v_AB = v_A − v_B | m/s |
Chapter 3: Motion in a Plane
| Formula | Expression | SI Unit |
|---|---|---|
| Vector addition | R⃗ = A⃗ + B⃗; R = √(A² + B² + 2AB cosθ) | — |
| Direction of resultant | tan α = B sinθ/(A + B cosθ) | — |
| Projectile: time of flight | T = 2u sinθ/g | s |
| Projectile: maximum height | H = u² sin²θ/(2g) | m |
| Projectile: range | R = u² sin2θ/g | m |
| Maximum range | At θ = 45°, R_max = u²/g | m |
| Centripetal acceleration | a_c = v²/r = ω²r | m/s² |
| Centripetal force | F_c = mv²/r = mω²r | N |
| Angular velocity | ω = 2π/T = 2πf = v/r | rad/s |
| Period and frequency | T = 1/f | s, Hz |
Chapter 4: Laws of Motion
| Formula | Expression | SI Unit |
|---|---|---|
| Newton's Second Law | F⃗ = ma⃗ | N (kg·m/s²) |
| Momentum | p⃗ = mv⃗ | kg·m/s |
| Impulse | J = FΔt = Δp | N·s |
| Newton's Third Law | F₁₂ = −F₂₁ | N |
| Friction (static max) | f_s = μ_s N | N |
| Friction (kinetic) | f_k = μ_k N | N |
| Angle of repose | tan θ = μ_s | — |
| Apparent weight in lift (up) | W' = m(g + a) | N |
| Apparent weight in lift (down) | W' = m(g − a) | N |
| Banking of roads | tan θ = v²/(rg) | — |
| Connected bodies (Atwood machine) | a = (m₁ − m₂)g/(m₁ + m₂); T = 2m₁m₂g/(m₁ + m₂) | m/s², N |
Chapter 5: Work, Energy and Power
| Formula | Expression | SI Unit |
|---|---|---|
| Work | W = F⃗·d⃗ = Fd cosθ | J (joule) |
| Kinetic energy | KE = ½mv² | J |
| Potential energy (gravitational) | PE = mgh | J |
| Work-energy theorem | W_net = ΔKE = ½mv² − ½mu² | J |
| Spring PE | PE = ½kx² | J |
| Power | P = W/t = F⃗·v⃗ | W (watt) |
| Conservative force | Work done in closed path = 0; PE definable | — |
| Elastic collision (1D) | v₁ = [(m₁−m₂)u₁ + 2m₂u₂]/(m₁+m₂) | m/s |
| Coefficient of restitution | e = (v₂−v₁)/(u₁−u₂) | Dimensionless |
| Inelastic collision | m₁u₁ + m₂u₂ = (m₁+m₂)v | Conservation of momentum |
Chapter 6: System of Particles and Rotational Motion
| Formula | Expression | SI Unit |
|---|---|---|
| Centre of mass | x_cm = Σmᵢxᵢ / Σmᵢ | m |
| Torque | τ⃗ = r⃗ × F⃗; τ = rF sinθ | N·m |
| Angular momentum | L⃗ = r⃗ × p⃗ = Iω | kg·m²/s |
| Moment of inertia | I = Σmᵢrᵢ² | kg·m² |
| Parallel axis theorem | I = I_cm + Md² | kg·m² |
| Perpendicular axis theorem | I_z = I_x + I_y (for planar body) | kg·m² |
| Newton's 2nd law (rotation) | τ = Iα | N·m |
| Rotational KE | KE = ½Iω² | J |
| Rolling (without slipping) | KE = ½mv² + ½Iω²; v = Rω | J |
Common MI values:
| Body | Axis | I |
|---|---|---|
| Ring | Through centre, ⊥ to plane | MR² |
| Disc | Through centre, ⊥ to plane | ½MR² |
| Solid sphere | Through centre | ⅖MR² |
| Hollow sphere | Through centre | ⅔MR² |
| Rod | Through centre, ⊥ to rod | ML²/12 |
| Rod | Through end, ⊥ to rod | ML²/3 |
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Chapter 7: Gravitation
| Formula | Expression | SI Unit |
|---|---|---|
| Newton's law of gravitation | F = Gm₁m₂/r² | N |
| Gravitational constant | G = 6.674 × 10⁻¹¹ N·m²/kg² | N·m²/kg² |
| Acceleration due to gravity | g = GM/R² | m/s² |
| g at height h | g_h = g(1 − 2h/R) for h << R; g_h = g R²/(R+h)² exact | m/s² |
| g at depth d | g_d = g(1 − d/R) | m/s² |
| Gravitational PE | U = −GMm/r | J |
| Escape velocity | v_e = √(2gR) = √(2GM/R) | m/s |
| Orbital velocity | v_o = √(gR) = √(GM/r) | m/s |
| Relation | v_e = √2 × v_o | — |
| Time period of satellite | T = 2π√(r³/GM) | s |
| Kepler's 3rd law | T² ∝ r³ | — |
| Geostationary satellite | T = 24 hrs, r ≈ 42,000 km from Earth's centre | — |
Chapter 8: Mechanical Properties of Solids
| Formula | Expression | SI Unit |
|---|---|---|
| Stress | σ = F/A | Pa (N/m²) |
| Strain | ε = ΔL/L (longitudinal), ΔV/V (volumetric), tanφ (shear) | Dimensionless |
| Hooke's Law | Stress = E × Strain (within elastic limit) | — |
| Young's modulus | Y = (F/A)/(ΔL/L) = FL/(AΔL) | Pa |
| Bulk modulus | B = −PV/ΔV | Pa |
| Shear modulus | G = (F/A)/tanφ | Pa |
| Poisson's ratio | σ = lateral strain / longitudinal strain | Dimensionless |
| Elastic PE per unit volume | u = ½ × stress × strain | J/m³ |
Chapter 9: Mechanical Properties of Fluids
| Formula | Expression | SI Unit |
|---|---|---|
| Pressure | P = F/A | Pa |
| Pressure at depth | P = P₀ + ρgh | Pa |
| Pascal's law | Pressure applied at one point is transmitted undiminished | — |
| Hydraulic lift | F₁/A₁ = F₂/A₂ | — |
| Buoyant force (Archimedes) | F_b = ρ_fluid × V_submerged × g | N |
| Equation of continuity | A₁v₁ = A₂v₂ | m³/s |
| Bernoulli's equation | P + ½ρv² + ρgh = constant | Pa |
| Torricelli's theorem | v = √(2gh) (speed of efflux) | m/s |
| Viscous force (Stokes) | F = 6πηrv | N |
| Terminal velocity | v_t = 2r²(ρ − σ)g/(9η) | m/s |
| Surface tension | S = F/l | N/m |
| Excess pressure (bubble in liquid) | ΔP = 2S/r | Pa |
| Excess pressure (soap bubble) | ΔP = 4S/r (two surfaces) | Pa |
| Capillary rise | h = 2S cosθ/(ρgr) | m |
Chapter 10: Thermal Properties of Matter
| Formula | Expression | SI Unit |
|---|---|---|
| Linear expansion | ΔL = αLΔT | m |
| Area expansion | ΔA = 2αAΔT = βAΔT | m² |
| Volume expansion | ΔV = 3αVΔT = γVΔT | m³ |
| Heat transfer | Q = mcΔT (specific heat) | J |
| Latent heat | Q = mL | J |
| Conduction | Q/t = KA(T₁−T₂)/d | W |
| Stefan's law | E = σT⁴ (σ = 5.67 × 10⁻⁸ W/m²K⁴) | W/m² |
| Wien's displacement law | λ_max × T = b (b = 2.898 × 10⁻³ m·K) | m·K |
| Newton's law of cooling | dT/dt = −k(T − T₀) | K/s |
Chapter 11: Thermodynamics
| Formula | Expression | SI Unit |
|---|---|---|
| First law | ΔU = Q − W (IUPAC: Q = heat added, W = work done by system) | J |
| Work done by gas | W = ∫PdV; for isobaric: W = PΔV | J |
| Isothermal process | W = nRT ln(V₂/V₁); ΔU = 0 | J |
| Adiabatic process | Q = 0; PV^γ = constant; W = (P₁V₁ − P₂V₂)/(γ−1) | J |
| Isochoric process | W = 0; Q = nCvΔT | J |
| Isobaric process | W = PΔV = nRΔT; Q = nCpΔT | J |
| Relation Cp − Cv | Cp − Cv = R | J/(mol·K) |
| Ratio γ | γ = Cp/Cv | Dimensionless |
| Carnot efficiency | η = 1 − T₂/T₁ | Dimensionless |
| Refrigerator COP | β = T₂/(T₁ − T₂) | Dimensionless |
Chapter 12: Kinetic Theory of Gases
| Formula | Expression | SI Unit |
|---|---|---|
| Pressure from kinetic theory | P = ⅓ρv²_rms = ⅓(mn/V)v²_rms | Pa |
| KE per molecule | KE = ½mv²_rms = (3/2)kT | J |
| KE per mole | KE = (3/2)RT | J/mol |
| RMS speed | v_rms = √(3RT/M) = √(3kT/m) | m/s |
| Degrees of freedom | f = 3 (monoatomic), 5 (diatomic at room T), 6 (polyatomic non-linear) | — |
| Energy per degree of freedom | ½kT per molecule, ½RT per mole | J |
| Total energy | U = (f/2)nRT | J |
| Cv | f R/2 | J/(mol·K) |
| Cp | (f/2 + 1)R | J/(mol·K) |
| γ values | Monoatomic: 5/3; Diatomic: 7/5; Polyatomic: 4/3 | — |
| Mean free path | λ = 1/(√2 πd²n) | m |
Chapter 13: Oscillations
| Formula | Expression | SI Unit |
|---|---|---|
| SHM displacement | x = A sin(ωt + φ) | m |
| Velocity in SHM | v = Aω cos(ωt + φ) = ω√(A²−x²) | m/s |
| Acceleration in SHM | a = −ω²x | m/s² |
| Time period (general) | T = 2π/ω | s |
| Spring-mass system | T = 2π√(m/k) | s |
| Simple pendulum | T = 2π√(l/g) | s |
| KE in SHM | ½mω²(A²−x²) | J |
| PE in SHM | ½mω²x² | J |
| Total energy | E = ½mω²A² = ½kA² | J |
| Springs in series | 1/k_eff = 1/k₁ + 1/k₂ | N/m |
| Springs in parallel | k_eff = k₁ + k₂ | N/m |
| Damped oscillation | x = Ae^(−bt/2m) sin(ω't + φ) | m |
Chapter 14: Waves
| Formula | Expression | SI Unit |
|---|---|---|
| Wave equation | y = A sin(kx − ωt) | m |
| Wave speed | v = fλ = ω/k | m/s |
| Wave number | k = 2π/λ | rad/m |
| Angular frequency | ω = 2πf = 2π/T | rad/s |
| Speed on string | v = √(T/μ) (T = tension, μ = mass per unit length) | m/s |
| Speed of sound | v = √(γP/ρ) = √(γRT/M) | m/s |
| Standing wave (both ends fixed) | fₙ = nv/(2L); n = 1, 2, 3... | Hz |
| Standing wave (one end open) | fₙ = nv/(4L); n = 1, 3, 5... (odd harmonics only) | Hz |
| Beat frequency | f_beat = | f₁ − f₂ |
| Doppler effect | f' = f × (v ± v₀)/(v ∓ vₛ) | Hz |
Doppler convention: upper signs when source and observer approach each other; lower signs when they recede.
Revision Schedule
| Day | Chapters | Formula Count |
|---|---|---|
| 1 | Ch 1–2: Units + Straight Line Motion | ~17 |
| 2 | Ch 3–4: Plane Motion + Laws of Motion | ~21 |
| 3 | Ch 5–6: Work/Energy + Rotational Motion | ~19 |
| 4 | Ch 7–8: Gravitation + Solids | ~20 |
| 5 | Ch 9–10: Fluids + Thermal | ~24 |
| 6 | Ch 11–12: Thermodynamics + Kinetic Theory | ~21 |
| 7 | Ch 13–14: Oscillations + Waves | ~22 |
For study techniques, see how to study physics numericals without fear.
Frequently Asked Questions
How many formulas are in CBSE Class 11 Physics?
There are approximately 150 important formulas across all 15 chapters. The most formula-dense chapters are Mechanical Properties of Fluids (~14), Motion in a Plane (~10), Gravitation (~12), and Oscillations (~12). Not every formula is equally important — focus on the ones marked in bold above.
Which Class 11 Physics chapters are most important for Class 12 boards?
Laws of Motion, Work-Energy-Power, and Gravitation concepts are directly used in Class 12 Electrostatics and Magnetism. Oscillations and Waves form the base for Class 12 Wave Optics and AC circuits. Thermodynamics carries over to Chemistry as well.
Do I need to know SI units for every formula?
Yes, for board exams and competitive exams. CBSE sometimes asks dimensional analysis questions (1–2 marks). JEE frequently tests dimensional consistency. Writing the correct unit in numerical answers also earns marks.
Is Class 11 Physics harder than Class 12?
Most students find Class 11 harder because it introduces foundational concepts like vectors, rotational motion, and thermodynamics from scratch. Class 12 Physics uses these foundations and feels more structured. Building strong Class 11 fundamentals makes Class 12 significantly easier.
How should I practice these formulas?
Do not just read them. For each formula: (1) write it from memory, (2) solve 3 numericals using it, (3) check what happens when variables change (proportionality analysis). This takes about 10 minutes per formula but locks it in permanently.
Can I use these formulas for JEE Main and NEET?
Yes. Every formula listed here is directly relevant to JEE Main and NEET. JEE may require additional formulas for advanced topics, but the Class 11 NCERT formula set covers 80% of what appears in JEE Main Physics.
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