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CBSE 14 min read23 October 2026

CBSE Class 11 Physics All Formulas Chapter Wise With SI Units 2027

Complete CBSE Class 11 Physics formulas for all 15 chapters: Units, Motion in Straight Line, Motion in Plane, Laws of Motion, Work-Energy-Power, System of Particles, Gravitation, Mechanical Properties, Thermal Properties, Thermodynamics, Kinetic Theory, Oscillations, Waves. Every formula with SI unit.

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

FormulaExpressionSI Unit
Dimensional formula[M^a L^b T^c]—
Percentage error(Δa/a) × 100%
Absolute errorΔa =a − a_mean
Relative errorΔa/aDimensionless
Addition/subtraction errorΔz = Δa + ΔbAbsolute errors add
Multiplication/division errorΔz/z = Δa/a + Δb/bRelative errors add
Power rule errorIf z = aᵐbⁿ, then Δz/z = m(Δa/a) + n(Δb/b)—

Chapter 2: Motion in a Straight Line

FormulaExpressionSI Unit
Average speedv_avg = total distance / total timem/s
Average velocityv⃗_avg = displacement / timem/s
Instantaneous velocityv = ds/dtm/s
Average accelerationa = (v − u)/tm/s²
1st equation of motionv = u + atm/s
2nd equation of motions = ut + ½at²m
3rd equation of motionv² = u² + 2asm²/s²
Distance in nth secondsₙ = u + a(2n−1)/2m
Free fallg = 9.8 m/s²; equations same with a = gm/s²
Relative velocityv_AB = v_A − v_Bm/s

Chapter 3: Motion in a Plane

FormulaExpressionSI Unit
Vector additionR⃗ = A⃗ + B⃗; R = √(A² + B² + 2AB cosθ)—
Direction of resultanttan α = B sinθ/(A + B cosθ)—
Projectile: time of flightT = 2u sinθ/gs
Projectile: maximum heightH = u² sin²θ/(2g)m
Projectile: rangeR = u² sin2θ/gm
Maximum rangeAt θ = 45°, R_max = u²/gm
Centripetal accelerationa_c = v²/r = ω²rm/s²
Centripetal forceF_c = mv²/r = mω²rN
Angular velocityω = 2π/T = 2πf = v/rrad/s
Period and frequencyT = 1/fs, Hz

Chapter 4: Laws of Motion

FormulaExpressionSI Unit
Newton's Second LawF⃗ = ma⃗N (kg·m/s²)
Momentump⃗ = mv⃗kg·m/s
ImpulseJ = FΔt = ΔpN·s
Newton's Third LawF₁₂ = −F₂₁N
Friction (static max)f_s = μ_s NN
Friction (kinetic)f_k = μ_k NN
Angle of reposetan 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 roadstan 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

FormulaExpressionSI Unit
WorkW = F⃗·d⃗ = Fd cosθJ (joule)
Kinetic energyKE = ½mv²J
Potential energy (gravitational)PE = mghJ
Work-energy theoremW_net = ΔKE = ½mv² − ½mu²J
Spring PEPE = ½kx²J
PowerP = W/t = F⃗·v⃗W (watt)
Conservative forceWork done in closed path = 0; PE definable—
Elastic collision (1D)v₁ = [(m₁−m₂)u₁ + 2m₂u₂]/(m₁+m₂)m/s
Coefficient of restitutione = (v₂−v₁)/(u₁−u₂)Dimensionless
Inelastic collisionm₁u₁ + m₂u₂ = (m₁+m₂)vConservation of momentum

Chapter 6: System of Particles and Rotational Motion

FormulaExpressionSI Unit
Centre of massx_cm = Σmᵢxᵢ / Σmᵢm
Torqueτ⃗ = r⃗ × F⃗; τ = rF sinθN·m
Angular momentumL⃗ = r⃗ × p⃗ = Iωkg·m²/s
Moment of inertiaI = Σmᵢrᵢ²kg·m²
Parallel axis theoremI = I_cm + Md²kg·m²
Perpendicular axis theoremI_z = I_x + I_y (for planar body)kg·m²
Newton's 2nd law (rotation)τ = IαN·m
Rotational KEKE = ½Iω²J
Rolling (without slipping)KE = ½mv² + ½Iω²; v = RωJ

Common MI values:

BodyAxisI
RingThrough centre, ⊥ to planeMR²
DiscThrough centre, ⊥ to plane½MR²
Solid sphereThrough centre⅖MR²
Hollow sphereThrough centre⅔MR²
RodThrough centre, ⊥ to rodML²/12
RodThrough end, ⊥ to rodML²/3

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Chapter 7: Gravitation

FormulaExpressionSI Unit
Newton's law of gravitationF = Gm₁m₂/r²N
Gravitational constantG = 6.674 × 10⁻¹¹ N·m²/kg²N·m²/kg²
Acceleration due to gravityg = GM/R²m/s²
g at height hg_h = g(1 − 2h/R) for h << R; g_h = g R²/(R+h)² exactm/s²
g at depth dg_d = g(1 − d/R)m/s²
Gravitational PEU = −GMm/rJ
Escape velocityv_e = √(2gR) = √(2GM/R)m/s
Orbital velocityv_o = √(gR) = √(GM/r)m/s
Relationv_e = √2 × v_o—
Time period of satelliteT = 2π√(r³/GM)s
Kepler's 3rd lawT² ∝ r³—
Geostationary satelliteT = 24 hrs, r ≈ 42,000 km from Earth's centre—

Chapter 8: Mechanical Properties of Solids

FormulaExpressionSI Unit
Stressσ = F/APa (N/m²)
Strainε = ΔL/L (longitudinal), ΔV/V (volumetric), tanφ (shear)Dimensionless
Hooke's LawStress = E × Strain (within elastic limit)—
Young's modulusY = (F/A)/(ΔL/L) = FL/(AΔL)Pa
Bulk modulusB = −PV/ΔVPa
Shear modulusG = (F/A)/tanφPa
Poisson's ratioσ = lateral strain / longitudinal strainDimensionless
Elastic PE per unit volumeu = ½ × stress × strainJ/m³

Chapter 9: Mechanical Properties of Fluids

FormulaExpressionSI Unit
PressureP = F/APa
Pressure at depthP = P₀ + ρghPa
Pascal's lawPressure applied at one point is transmitted undiminished—
Hydraulic liftF₁/A₁ = F₂/A₂—
Buoyant force (Archimedes)F_b = ρ_fluid × V_submerged × gN
Equation of continuityA₁v₁ = A₂v₂m³/s
Bernoulli's equationP + ½ρv² + ρgh = constantPa
Torricelli's theoremv = √(2gh) (speed of efflux)m/s
Viscous force (Stokes)F = 6πηrvN
Terminal velocityv_t = 2r²(ρ − σ)g/(9η)m/s
Surface tensionS = F/lN/m
Excess pressure (bubble in liquid)ΔP = 2S/rPa
Excess pressure (soap bubble)ΔP = 4S/r (two surfaces)Pa
Capillary riseh = 2S cosθ/(ρgr)m

Chapter 10: Thermal Properties of Matter

FormulaExpressionSI Unit
Linear expansionΔL = αLΔTm
Area expansionΔA = 2αAΔT = βAΔTm²
Volume expansionΔV = 3αVΔT = γVΔTm³
Heat transferQ = mcΔT (specific heat)J
Latent heatQ = mLJ
ConductionQ/t = KA(T₁−T₂)/dW
Stefan's lawE = σT⁴ (σ = 5.67 × 10⁻⁸ W/m²K⁴)W/m²
Wien's displacement lawλ_max × T = b (b = 2.898 × 10⁻³ m·K)m·K
Newton's law of coolingdT/dt = −k(T − T₀)K/s

Chapter 11: Thermodynamics

FormulaExpressionSI Unit
First lawΔU = Q − W (IUPAC: Q = heat added, W = work done by system)J
Work done by gasW = ∫PdV; for isobaric: W = PΔVJ
Isothermal processW = nRT ln(V₂/V₁); ΔU = 0J
Adiabatic processQ = 0; PV^γ = constant; W = (P₁V₁ − P₂V₂)/(γ−1)J
Isochoric processW = 0; Q = nCvΔTJ
Isobaric processW = PΔV = nRΔT; Q = nCpΔTJ
Relation Cp − CvCp − Cv = RJ/(mol·K)
Ratio γγ = Cp/CvDimensionless
Carnot efficiencyη = 1 − T₂/T₁Dimensionless
Refrigerator COPβ = T₂/(T₁ − T₂)Dimensionless

Chapter 12: Kinetic Theory of Gases

FormulaExpressionSI Unit
Pressure from kinetic theoryP = ⅓ρv²_rms = ⅓(mn/V)v²_rmsPa
KE per moleculeKE = ½mv²_rms = (3/2)kTJ
KE per moleKE = (3/2)RTJ/mol
RMS speedv_rms = √(3RT/M) = √(3kT/m)m/s
Degrees of freedomf = 3 (monoatomic), 5 (diatomic at room T), 6 (polyatomic non-linear)—
Energy per degree of freedom½kT per molecule, ½RT per moleJ
Total energyU = (f/2)nRTJ
Cvf R/2J/(mol·K)
Cp(f/2 + 1)RJ/(mol·K)
γ valuesMonoatomic: 5/3; Diatomic: 7/5; Polyatomic: 4/3—
Mean free pathλ = 1/(√2 πd²n)m

Chapter 13: Oscillations

FormulaExpressionSI Unit
SHM displacementx = A sin(ωt + φ)m
Velocity in SHMv = Aω cos(ωt + φ) = ω√(A²−x²)m/s
Acceleration in SHMa = −ω²xm/s²
Time period (general)T = 2π/ωs
Spring-mass systemT = 2π√(m/k)s
Simple pendulumT = 2π√(l/g)s
KE in SHM½mω²(A²−x²)J
PE in SHM½mω²x²J
Total energyE = ½mω²A² = ½kA²J
Springs in series1/k_eff = 1/k₁ + 1/k₂N/m
Springs in parallelk_eff = k₁ + k₂N/m
Damped oscillationx = Ae^(−bt/2m) sin(ω't + φ)m

Chapter 14: Waves

FormulaExpressionSI Unit
Wave equationy = A sin(kx − ωt)m
Wave speedv = fλ = ω/km/s
Wave numberk = 2π/λrad/m
Angular frequencyω = 2πf = 2π/Trad/s
Speed on stringv = √(T/μ) (T = tension, μ = mass per unit length)m/s
Speed of soundv = √(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 frequencyf_beat =f₁ − f₂
Doppler effectf' = f × (v ± v₀)/(v ∓ vₛ)Hz

Doppler convention: upper signs when source and observer approach each other; lower signs when they recede.


Revision Schedule

DayChaptersFormula Count
1Ch 1–2: Units + Straight Line Motion~17
2Ch 3–4: Plane Motion + Laws of Motion~21
3Ch 5–6: Work/Energy + Rotational Motion~19
4Ch 7–8: Gravitation + Solids~20
5Ch 9–10: Fluids + Thermal~24
6Ch 11–12: Thermodynamics + Kinetic Theory~21
7Ch 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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