CBSE

Physics Formulas for Class 12 – All Chapters

Physics Formulas for Class 12

Physics can feel overwhelming when you’re staring at a stack of textbooks before your Class 12 exams. But here’s the secret weapon that can transform your preparation: mastering physics formulas for class 12! Whether you’re aiming for top marks in your board exams or preparing for competitive tests like JEE or NEET, having all formulas of physics class 12 at your fingertips is absolutely crucial. 

This comprehensive guide brings together every important physics formulas for class 12 from all chapters, making your revision systematic and stress-free. Students often search for physics formulas for class 12 pdf free download to have offline access, and this guide serves as your complete reference.

Chapter-Wise List of Physics Formulas for Class 12

Understanding Class 12 physics formulas becomes much easier when they’re organised chapter-wise. The all formulas of physics class 12 CBSE curriculum covers 14 essential chapters, each containing fundamental equations that form the backbone of physics concepts. These physics formulas for Class 12 CBSE board examinations are carefully selected to cover all important topics that frequently appear in board exams and competitive tests. Let’s explore each chapter’s key formulas with their symbols and SI units for better understanding of physics class 12 formulas.

Chapter 1: Electric Charges and Fields

Introduces the concept of electric charge, forces between charges (Coulomb’s law), and the electric field. Gauss’s Law is a key highlight for solving symmetrical charge distribution problems.

FormulaDescriptionSI Unit
F = k(q₁q₂)/r²Coulomb’s LawN (Newton)
E = F/qElectric FieldN/C or V/m
E = kQ/r²Electric Field due to Point ChargeN/C
E = kQ/4πε₀r²Electric Field (Alternative Form)N/C
φ = E⋅A cosθElectric FluxN⋅m²/C
φ = Q/ε₀Gauss’s LawN⋅m²/C
E = λ/2πε₀rElectric Field due to Line ChargeN/C
E = σ/2ε₀Electric Field due to Infinite SheetN/C
F = qEForce on Charge in Electric FieldN
p = qdElectric Dipole MomentC⋅m
E = 2kp/r³Electric Field on Axial Line of DipoleN/C
E = kp/r³Electric Field on Equatorial Line of DipoleN/C
τ = pE sinθTorque on Electric DipoleN⋅m
U = -pE cosθPotential Energy of DipoleJ
λ = Q/LLinear Charge DensityC/m
σ = Q/ASurface Charge DensityC/m²
ρ = Q/VVolume Charge DensityC/m³

Constants:

  • k = 9 × 10⁹ N⋅m²/C²
  • ε₀ = 8.85 × 10⁻¹² C²/N⋅m²

Diagrams:

physics class 12 formulas

Chapter 2: Electrostatic Potential and Capacitance

Covers electric potential, capacitors, and energy stored in electric fields. Focuses on how charge behaves in different capacitor systems.

FormulaDescriptionSI Unit
V = W/qElectric PotentialV (Volt)
V = kQ/rPotential due to Point ChargeV
V = kQ/4πε₀rPotential (Alternative Form)V
W = q(V₂ – V₁)Work Done in Moving ChargeJ
E = -dV/drElectric Field from PotentialN/C
V = kp cosθ/r²Potential due to DipoleV
C = Q/VCapacitanceF (Farad)
C = ε₀A/dParallel Plate CapacitorF
C = 4πε₀RCapacitance of Isolated SphereF
C = 2πε₀L/ln(b/a)Capacitance of Cylindrical CapacitorF
K = C/C₀Dielectric ConstantDimensionless
C = KC₀Capacitance with DielectricF
U = ½CV²Energy Stored in CapacitorJ
U = ½QVEnergy Stored (Alternative)J
U = Q²/2CEnergy Stored (Alternative)J
u = ½ε₀E²Energy DensityJ/m³
1/C = 1/C₁ + 1/C₂ + 1/C₃Capacitors in SeriesF
C = C₁ + C₂ + C₃Capacitors in ParallelF
F = ½ε₀E²AForce between Capacitor PlatesN

Diagrams:

class 12 physics formula all chapters pdf

Chapter 3: Current Electricity

Deals with electric current, Ohm’s Law, combination of resistors, EMF, and the heating effect of electric current (Joule’s Law).

FormulaDescriptionSI Unit
I = Q/tCurrentA (Ampere)
I = nAveCurrent (Microscopic Form)A
vd = I/nAeDrift Velocitym/s
V = IROhm’s LawV (Volt)
R = ρL/AResistanceΩ (Ohm)
G = 1/RConductanceS (Siemens)
σ = 1/ρConductivityS/m
ρ = ρ₀[1 + α(T – T₀)]Temperature Dependence of ResistivityΩ⋅m
J = I/ACurrent DensityA/m²
J = σECurrent Density (Ohm’s Law)A/m²
P = VIPowerW (Watt)
P = I²RPower (Alternative)W
P = V²/RPower (Alternative)W
H = I²RtHeat Produced (Joule’s Law)J
Rs = R₁ + R₂ + R₃Resistors in SeriesΩ
1/Rp = 1/R₁ + 1/R₂ + 1/R₃Resistors in ParallelΩ
ε = I(R + r)EMF of CellV
ε = V + IrEMF (Alternative Form)V
η = R/(R + r)Efficiency of CellDimensionless
I = ε/(R + r)Current from CellA
V = ε – IrTerminal VoltageV
Req = nr + R/nCells in SeriesΩ
Req = r/n + RCells in ParallelΩ
I₁R₁ = I₂R₂Current Division RuleA
V₁/V₂ = R₁/R₂Voltage Division RuleV

Diagrams:

Current Electricity Diagram

Chapter 4: Moving Charges and Magnetism

Discusses magnetic effects of electric current, Lorentz force, and the motion of charged particles in magnetic fields. Key for understanding cyclotrons and magnetic fields due to wires and loops.

FormulaDescriptionSI Unit
F = q(v × B)Lorentz Force (Vector Form)N (Newton)
F = qvB sinθLorentz Force (Scalar Form)N
F = q(E + v × B)Complete Lorentz ForceN
F = BIL sinθForce on Current-Carrying WireN
F = BI∫dlForce on Current ElementN
B = μ₀I/2πrMagnetic Field due to Straight WireT (Tesla)
B = μ₀I/4πr²Magnetic Field due to Current ElementT
B = μ₀IR²/2(R² + x²)^(3/2)Magnetic Field on Axis of Circular LoopT
B = μ₀I/2RMagnetic Field at Centre of Circular LoopT
B = μ₀nIMagnetic Field inside SolenoidT
B = μ₀nI/2Magnetic Field at End of SolenoidT
B = μ₀NI/LMagnetic Field inside ToroidT
r = mv/qBRadius of Circular Pathm
T = 2πm/qBTime Period of Circular Motions
f = qB/2πmCyclotron FrequencyHz
ω = qB/mAngular Frequencyrad/s
p = qBrMomentum of Charged Particlekg⋅m/s
KE = q²B²r²/2mKinetic EnergyJ
μ = IAMagnetic Dipole MomentA⋅m²
τ = μ × BTorque on Magnetic DipoleN⋅m
U = -μ⋅BPotential Energy of DipoleJ
F = μ(dB/dx)Force on Magnetic DipoleN
dB = μ₀I dl × r̂/4πr²Biot-Savart LawT

Constants:

  • μ₀ = 4π × 10⁻⁷ T⋅m/A

Diagrams:

Magnetic Field and Moving Charges

Chapter 5: Magnetism and Matter

Explores Earth’s magnetism and classification of magnetic materials. Introduces magnetic susceptibility, permeability, and behavior in external fields.

FormulaDescriptionSI Unit
M = mLMagnetic MomentA⋅m²
m = IAMagnetic Dipole MomentA⋅m²
B = μ₀(H + M)Magnetic Field in MaterialT
H = B/μ₀ – MMagnetic Field IntensityA/m
I = M/HMagnetic IntensityA/m
χ = M/HMagnetic SusceptibilityDimensionless
μ = B/HMagnetic PermeabilityH/m
μᵣ = μ/μ₀Relative PermeabilityDimensionless
μᵣ = 1 + χRelation between μᵣ and χDimensionless
B = μ₀H(1 + χ)Magnetic Field with SusceptibilityT
B = μ₀μᵣHMagnetic Field with Relative PermeabilityT
F = χVB(dB/dx)Force on Magnetic MaterialN
μB = eℏ/2mBohr MagnetonJ/T
μ = -gμB√(J(J+1))Magnetic Moment of AtomJ/T
χ = C/TCurie’s Law (Paramagnetic)K
χ = C/(T – TC)Curie-Weiss Law (Ferromagnetic)K
Hc = -M/χCoercive FieldA/m

Material Classifications:

  • Diamagnetic: χ < 0, μᵣ < 1
  • Paramagnetic: χ > 0, μᵣ > 1
  • Ferromagnetic: χ >> 1, μᵣ >> 1

Chapter 6: Electromagnetic Induction

Focuses on Faraday’s and Lenz’s Laws of induction, EMF generation, inductance, and LR circuits. Crucial for understanding transformers and electric generators.

FormulaDescriptionSI Unit
ε = -dφ/dtFaraday’s LawV (Volt)
ε = -N(dφ/dt)Faraday’s Law for N TurnsV
ε = BLvMotional EMFV
ε = ½BLv²Motional EMF (Rotating Rod)V
φ = BA cosθMagnetic FluxWb (Weber)
φ = ∫B⋅dAMagnetic Flux (General)Wb
ε = -L(dI/dt)Self-Induced EMFV
ε = -M(dI/dt)Mutually Induced EMFV
L = φ/ISelf-InductanceH (Henry)
L = μ₀n²AlSelf-Inductance of SolenoidH
L = μ₀N²A/lSelf-Inductance (Alternative)H
M = φ₂/I₁ = φ₁/I₂Mutual InductanceH
M = μ₀N₁N₂A/lMutual Inductance of SolenoidsH
k = M/√(L₁L₂)Coupling CoefficientDimensionless
U = ½LI²Energy Stored in InductorJ
u = B²/2μ₀Magnetic Energy DensityJ/m³
F = BILForce on ConductorN
P = BILvPower DissipatedW
I = I₀(1 – e^(-Rt/L))Current Growth in LR CircuitA
I = I₀e^(-Rt/L)Current Decay in LR CircuitA
τ = L/RTime Constant of LR Circuits
ε = BLv sinωtAC Motional EMFV

Diagrams:

Induction Heating

Chapter 7: Alternating Current

Covers AC circuits, reactance, impedance, power in AC, and resonance. Includes key quantities like RMS, average current, and power factor.

FormulaDescriptionSI Unit
I = I₀ sinωtInstantaneous AC CurrentA (Ampere)
V = V₀ sinωtInstantaneous AC VoltageV (Volt)
I = I₀ sin(ωt + φ)AC Current with PhaseA
V = V₀ sin(ωt + φ)AC Voltage with PhaseV
Iᵣₘₛ = I₀/√2RMS CurrentA
Vᵣₘₛ = V₀/√2RMS VoltageV
Iₐᵥₑ = 2I₀/πAverage CurrentA
Vₐᵥₑ = 2V₀/πAverage VoltageV
XL = ωL = 2πfLInductive ReactanceΩ
XC = 1/ωC = 1/2πfCCapacitive ReactanceΩ
Z = √(R² + (XL – XC)²)ImpedanceΩ
tanφ = (XL – XC)/RPhase AngleDimensionless
VL = IXLVoltage across InductorV
VC = IXCVoltage across CapacitorV
VR = IRVoltage across ResistorV
P = VᵣₘₛIᵣₘₛ cosφAverage PowerW
P = I²ᵣₘₛRPower DissipatedW
Q = VᵣₘₛIᵣₘₛ sinφReactive PowerVAr
S = VᵣₘₛIᵣₘₛApparent PowerVA
cosφ = R/ZPower FactorDimensionless
f₀ = 1/2π√(LC)Resonant FrequencyHz
ω₀ = 1/√(LC)Angular Resonant Frequencyrad/s
Q = ω₀L/R = 1/ω₀RCQuality FactorDimensionless
BW = f₀/QBandwidthHz
Z₀ = √(L/C)Characteristic ImpedanceΩ
Np/Ns = Vp/Vs = Is/IpTransformer EquationDimensionless
η = PsVsIs cosφs/PpVpIp cosφpTransformer EfficiencyDimensionless

Diagrams:

Alternate Current

Chapter 8: Electromagnetic Waves

Discusses the nature, propagation, and characteristics of EM waves including energy transport and the electromagnetic spectrum.

FormulaDescriptionSI Unit
c = 1/√(μ₀ε₀)Speed of Light in Vacuumm/s
c = fλWave Equationm/s
v = fλWave Speed in Mediumm/s
n = c/vRefractive IndexDimensionless
E = hf = hc/λEnergy of PhotonJ (Joule)
E = pcEnergy-Momentum RelationJ
p = E/c = h/λMomentum of Photonkg⋅m/s
I = P/AIntensity of WaveW/m²
I = ε₀cE₀²/2Intensity in terms of Electric FieldW/m²
I = B₀²/2μ₀cIntensity in terms of Magnetic FieldW/m²
E₀/B₀ = cRatio of Electric to Magnetic Fieldm/s
u = ε₀E²/2 + B²/2μ₀Energy DensityJ/m³
S = E × B/μ₀Poynting VectorW/m²
P = uAcPower Carried by WaveW
Pᵣₐd = I/cRadiation PressureN/m²
F = PARadiation ForceN
λ = c/fWavelength in Vacuumm
T = 1/fTime Periods
ω = 2πfAngular Frequencyrad/s
k = 2π/λWave Numberm⁻¹
E = E₀ sin(kx – ωt)Electric Field WaveV/m
B = B₀ sin(kx – ωt)Magnetic Field WaveT
ε = ε₀εᵣPermittivity of MediumF/m
μ = μ₀μᵣPermeability of MediumH/m
v = 1/√(εμ)Speed in Mediumm/s

Constants:

  • c = 3 × 10⁸ m/s
  • h = 6.63 × 10⁻³⁴ J⋅s

Electromagnetic Spectrum:

  • Radio waves: λ > 1 m
  • Microwaves: 1 mm < λ < 1 m
  • Infrared: 700 nm < λ < 1 mm
  • Visible: 400 nm < λ < 700 nm
  • Ultraviolet: 10 nm < λ < 400 nm
  • X-rays: 0.01 nm < λ < 10 nm
  • Gamma rays: λ < 0.01 nm

Diagrams:

all formulas of physics class 12 CBSE

Chapter 9: Ray Optics and Optical Instruments

Explores reflection, refraction, lens/mirror formulas, and optical instruments like microscopes and telescopes. Critical for image formation and power of lenses.

FormulaDescriptionSI Unit
1/f = 1/v + 1/uLens Formulam⁻¹
1/f = 1/v + 1/uMirror Formulam⁻¹
m = v/uLinear MagnificationDimensionless
m = h’/hMagnification (Height Ratio)Dimensionless
P = 1/fPower of LensD (Dioptre)
P = P₁ + P₂Power of Combined LensesD
n₁sinθ₁ = n₂sinθ₂Snell’s LawDimensionless
sinθc = n₂/n₁Critical AngleDimensionless
sinθc = 1/nCritical Angle (Denser to Rarer)Dimensionless
1/f = (n-1)(1/R₁ – 1/R₂)Lens Maker’s Formulam⁻¹
1/f = (n-1)/RLens Maker’s (Equiconvex)m⁻¹
n = sinθ₁/sinθ₂Refractive IndexDimensionless
n = c/vRefractive Index (Speed)Dimensionless
n = λ₀/λRefractive Index (Wavelength)Dimensionless
δ = θ₁ + θ₂ – ADeviation in PrismDegree
δₘ = 2i – AMinimum DeviationDegree
n = sin((A + δₘ)/2)/sin(A/2)Refractive Index of PrismDimensionless
r₁ + r₂ = ARelation in PrismDegree
A = r₁ + r₂Prism AngleDegree
fe = D/f₀Magnifying Power of TelescopeDimensionless
m = D/fMagnifying Power of MicroscopeDimensionless
m = (D/f₀)(1 + D/fe)Compound MicroscopeDimensionless
m = D/fSimple MicroscopeDimensionless
f = R/2Focal Length of Spherical Mirrorm
1/R = 1/fMirror Curvaturem⁻¹
h’ = -h(v/u)Image Heightm
M = m₀ × meTotal MagnificationDimensionless
Resolving Power = 1.22λ/DResolving Power of TelescopeDimensionless
dθ = 1.22λ/DAngular Resolutionrad

Diagrams:

physics formulas for class 12 CBSE board

Chapter 10: Wave Optics

Covers interference, diffraction, and polarization of light. Focuses on wave-based behavior of light and applications like Young’s double-slit experiment.

FormulaDescriptionSI Unit
λ = c/fWavelengthm (Metre)
v = fλWave Speedm/s
n = c/vRefractive IndexDimensionless
y = (nλD)/dFringe Position (Young’s Experiment)m
β = λD/dFringe Widthm
Δx = β = λD/dFringe Separationm
I = I₁ + I₂ + 2√(I₁I₂)cosφIntensity in InterferenceW/m²
I = I₀cos²(φ/2)Intensity (Two Source)W/m²
φ = (2π/λ)ΔPhase Differencerad
Δ = S₂P – S₁PPath Differencem
φ = (2π/λ)d sinθPhase Difference (General)rad
dsinθ = nλDiffraction Gratingm
N = 1/dGrating Elementm⁻¹
sinθ = nλ/aSingle Slit DiffractionDimensionless
I = I₀(sin²α/α²)Intensity in Single SlitW/m²
α = (πa sinθ)/λDiffraction Parameterrad
R = λ/ΔλResolving PowerDimensionless
R = mNResolving Power of GratingDimensionless
θ = λ/aAngular Width of Central Maximumrad
dθ = λ/DAngular Resolutionrad
μ = n₁/n₂Relative Refractive IndexDimensionless
sinθp = n₂/n₁Polarising AngleDimensionless
tanθp = nBrewster’s LawDimensionless
I = I₀cos²θMalus’ LawW/m²

Chapter 11: Dual Nature of Radiation and Matter

Discusses photoelectric effect, de Broglie wavelength, and quantum concepts of light and matter. Lays foundation for modern physics.

FormulaDescriptionSI Unit
E = hf = hc/λPlanck’s EquationJ (Joule)
KEmax = hf – φPhotoelectric EffectJ
KEmax = hf – hf₀Photoelectric Effect (Alternative)J
hf₀ = φWork FunctionJ
eV₀ = hf – φStopping PotentialeV
λ = h/pde Broglie Wavelengthm
λ = h/mvde Broglie Wavelength (Particles)m
λ = h/√(2mKE)de Broglie Wavelength (KE Form)m
λ = h/√(2meV)de Broglie Wavelength (Electrons)m
p = h/λMomentumkg⋅m/s
E = pcEnergy-Momentum Relation (Photons)J
E² = (pc)² + (mc²)²Energy-Momentum Relation (Particles)J
hf = KEmax + φEinstein’s Photoelectric EquationJ
ν₀ = φ/hThreshold FrequencyHz
λ₀ = hc/φThreshold Wavelengthm
I = nhfIntensity of LightW/m²
N = I/hfPhoton Fluxphotons/s/m²
p = E/c = hf/cPhoton Momentumkg⋅m/s
K = ½mv²Kinetic EnergyJ
λc = h/mcCompton Wavelengthm
Δλ = λc(1 – cosθ)Compton Scatteringm
E = hf = hc/λPhoton EnergyJ
Group velocity = dω/dkGroup Velocitym/s
Phase velocity = ω/kPhase Velocitym/s

Chapter 12: Atoms

Explains the structure of atoms, Bohr’s model, and energy transitions. Introduces energy levels, spectral lines, and atomic constants.

FormulaDescriptionSI Unit
rn = n²r₀Bohr’s Radiusm
r₀ = ε₀h²/πme²Bohr Radius Constantm
En = -13.6/n²Energy Levels (Hydrogen)eV
En = -me⁴/8ε₀²h²n²Energy Levels (Detailed)J
E∞ = 13.6 eVIonisation Energy of HydrogeneV
f = (E₂ – E₁)/hFrequency of Emitted PhotonHz
λ = hc/(E₂ – E₁)Wavelength of Emitted Photonm
1/λ = R(1/n₁² – 1/n₂²)Rydberg Formulam⁻¹
R = me⁴/8ε₀²h³cRydberg Constantm⁻¹
L = √(l(l+1))ℏOrbital Angular MomentumJ⋅s
Lz = mlℏz-component of Angular MomentumJ⋅s
μ = -μB√(j(j+1))Magnetic MomentJ/T
μB = eℏ/2mBohr MagnetonJ/T
vn = e²/2ε₀hnOrbital Velocitym/s
Tn = 8ε₀²h³n³/me⁴Time Periods
fn = me⁴/8ε₀²h³n³Orbital FrequencyHz
KE = 13.6/n²Kinetic EnergyeV
PE = -27.2/n²Potential EnergyeV
E = KE + PETotal EnergyeV
Z = 1 (for Hydrogen)Atomic NumberDimensionless
En = -13.6Z²/n²Energy for Hydrogen-like atomseV
a = me²c²/2ℏFine Structure ConstantDimensionless

Constants:

  • r₀ = 0.529 × 10⁻¹⁰ m
  • ℏ = h/2π = 1.055 × 10⁻³⁴ J⋅s
  • R = 1.097 × 10⁷ m⁻¹

Diagrams:

Atoms

Chapter 13: Nuclei

Covers nuclear structure, radioactivity, nuclear binding energy, and decay laws. Important for understanding energy release in nuclear reactions.

FormulaDescriptionSI Unit
N = N₀e⁻λtRadioactive Decay LawDimensionless
A = A₀e⁻λtActivity DecayBq
T₁/₂ = ln2/λ = 0.693/λHalf-Lifes
τ = 1/λMean Lifes
A = λNActivityBq (Becquerel)
A = dN/dtRate of DecayBq
λ = ln2/T₁/₂Decay Constants⁻¹
N = N₀/2ⁿDecay after n half-livesDimensionless
BE = (Δm)c²Binding EnergyJ
BE = (Zmp + Nmn – M)c²Binding Energy (Detailed)J
BE/A = Binding Energy per nucleonBinding Energy per NucleonJ
Q = (mi – mf)c²Q-Value of ReactionJ
R = R₀A^(1/3)Nuclear Radiusm
ρ = 3A/4πR³Nuclear Densitykg/m³
E = mc²Mass-Energy EquivalenceJ
1 u = 931.5 MeV/c²Atomic Mass UnitJ
r = 1.2 × 10⁻¹⁵ mNuclear Radius Constantm
α-decay: ᴬzX → ᴬ⁻⁴z₋₂Y + ⁴₂HeAlpha Decay
β⁻-decay: ᴬzX → ᴬz₊₁Y + e⁻ + ν̄Beta Minus Decay
β⁺-decay: ᴬzX → ᴬz₋₁Y + e⁺ + νBeta Plus Decay
γ-decay: X* → X + γGamma Decay
Kα = ½mv²Kinetic Energy of AlphaJ
Eα/Eproduct = mproduct/mαEnergy Sharing in Alpha DecayJ
Cross-section = σReaction Cross-section

Constants:

  • R₀ = 1.2 × 10⁻¹⁵ m
  • c = 3 × 10⁸ m/s
  • 1 u = 1.66 × 10⁻²⁷ kg = 931.5 MeV/c²

Chapter 14: Semiconductor Electronics

Introduces semiconductors, diodes, transistors, and logic gates. Key for understanding electronics and modern devices.

FormulaDescriptionSI Unit
I = I₀(e^(eV/kT) – 1)Diode Current EquationA
I = I₀(e^(qV/kT) – 1)Diode Current (Alternative)A
η = Pout/Pin × 100%EfficiencyPercentage
β = IC/IBCurrent Gain (BJT)Dimensionless
α = IC/IECurrent Gain (CB)Dimensionless
β = α/(1-α)Relation between α and βDimensionless
IE = IB + ICCurrent Relation in BJTA
Av = -βRL/riVoltage GainDimensionless
Av = -gmRLVoltage Gain (FET)Dimensionless
Ai = βCurrent GainDimensionless
Ap = Av × AiPower GainDimensionless
Ri = βreInput ResistanceΩ
R₀ = RCOutput ResistanceΩ
f₀ = 1/(2π√LC)Resonant FrequencyHz
fc = 1/(2πRC)Cut-off FrequencyHz
BW = f₂ – f₁BandwidthHz
Q = f₀/BWQuality FactorDimensionless
gm = ΔIC/ΔVBETransconductanceS
rd = 1/gmDynamic ResistanceΩ
VBE = 0.7 VBase-Emitter Voltage (Si)V
VBE = 0.3 VBase-Emitter Voltage (Ge)V
ni = √(NC NV)e^(-Eg/2kT)Intrinsic Carrier Concentrationm⁻³
σ = nμₑe + pμₕeConductivityS/m
VT = kT/qThermal VoltageV
G = 1/RConductanceS

Constants:

  • k = 1.38 × 10⁻²³ J/K (Boltzmann constant)
  • q = 1.6 × 10⁻¹⁹ C (Electronic charge)
  • T = 300 K (Room temperature)

Also Check: Toughest and Easiest Chapters in CBSE Class 12 Chemistry

Tips to Memorise Physics Formulas for Class 12 Students

Memorising physics formulas for class 12 doesn’t have to be a nightmare! Here are some proven strategies that actually work for mastering physics formulas:

Create flashcards – Write the formula on one side and its application on the other. Review them during breaks or whilst travelling to reinforce your memory of physics formulas for class 12.

Practice derivations – Understanding how formulas are derived helps you remember them better and builds deeper understanding of fundamental physics formulas for class 12.

Use mnemonics – Create memorable phrases or acronyms. For example, “V = IR” can be remembered as “Voltage Is Resistance times Current.”

Apply formulas immediately – Solve problems right after learning a formula. This reinforces memory through practice with physics formulas for class 12.

Group similar formulas – Study related formulas together (like all the lens formulas or all the AC formulas) to understand patterns in physics formulas for class 12.

Write them repeatedly – The old-fashioned method of writing formulas multiple times still works wonders for muscle memory.

Make formula sheets – Create concise summary sheets for each chapter and stick them where you’ll see them often.

Also Check: Toughest and Easiest Chapters in CBSE Class 12 Physics

Conclusion

Mastering physics formulas for class 12 is your gateway to exam success and a deeper understanding of the physical world around you. Remember that physics formulas for class 12 aren’t just equations to memorise, they’re the language physics uses to describe natural phenomena. Regular practice with these physics formulas for class 12 will not only help you score better marks but also develop logical thinking skills that benefit you beyond academics. Keep this comprehensive guide handy, practice consistently with these physics formulas for class 12, and watch your physics performance soar to new heights!

FAQs

How many formulas should I memorise for Class 12 Physics?

Focus on the essential formulas from each chapter—approximately 100-120 key formulas. Quality over quantity is important; understand the derivation and application of each formula.

What’s the best way to avoid mixing up similar formulas?

Create comparison charts, practice derivations, and solve plenty of problems. Understanding the physical meaning behind each formula helps prevent confusion.

Should I memorise the values of all physical constants?

Learn the most commonly used constants like c, h, k, μ₀, ε₀, and their approximate values. Most exams provide a formula sheet with constants.

How can I remember which formula to use in word problems?

Practice identifying keywords in problems, understand the physical situation described, and create a mental map linking problem types to relevant formulas.

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