| 1 | Mirror Formula | v1+u1=f1 | Sign convention: New Cartesian |
| 2 | Magnification (Mirror) | m=−uv=hohi | Lateral magnification |
| 3 | Lens Formula | v1−u1=f1 | Thin lens |
| 4 | Lens Maker’s Formula | f1=(n−1)(R11−R21) | For thin lens in air |
| 5 | Magnification (Lens) | m=uv=hohi | - |
| 6 | Power of Lens | P=f1 (f in metre) | Unit: Dioptre (D) |
| 7 | Equivalent Focal Length (Two thin lenses) | F1=f11+f21−f1f2d | d = separation |
| 8 | Refraction at Single Surface | vn2−un1=Rn2−n1 | - |
| 9 | Snell’s Law | n1sini=n2sinr | - |
| 10 | Critical Angle | sinC=μ1 | For denser to rarer |
| 11 | Total Internal Reflection (TIR) | Occurs when i>C | Optical fibre principle |
| 12 | Lateral Shift in Glass Slab | d=tsini(1−μ1) | t = thickness |
| 13 | Prism Deviation | δ=i+e−A | Minimum deviation δm=2i−A |
| 14 | Prism Refractive Index (Minimum Deviation) | μ=sin(A/2)sin(2A+δm) | - |
| 15 | Apparent Depth | d′=μd | For small angles |
| 16 | Combination of Prism (Dispersion without Deviation) | δ1+δ2=0 | Crown + Flint glass |
| 17 | Young’s Double Slit – Path Difference | Δx=dsinθ | - |
| 18 | Condition for Bright Fringe | dsinθ=mλ (m = 0,1,2…) | Constructive interference |
| 19 | Condition for Dark Fringe | dsinθ=(2m+1)2λ | Destructive interference |
| 20 | Fringe Width | β=dλD | D = distance to screen |
| 21 | Intensity in Interference | I=4I0cos2(ϕ/2) | ϕ = phase difference |
| 22 | Single Slit Diffraction – Minima | asinθ=mλ (m=1,2,3…) | Central maxima width = a2λD |
| 23 | Resolving Power of Microscope | RP=dmin1=λ2μsinθ | - |
| 24 | Resolving Power of Telescope | RP=1.22λD | D = diameter of objective |
| 25 | Polarisation by Reflection (Brewster’s Law) | taniB=μ | iB = polarizing angle |
| 26 | Malus Law | I=I0cos2θ | Intensity after polarizer |
| 27 | Optical Path Length | OPL=μ×geometrical path | - |
| 28 | Condition for Constructive Reflection (Thin Film) | 2μtcosr=(m+21)λ (reflection) | Phase change consideration |
| 29 | Doppler Shift in Light | λΔλ=cv | For v << c |
| 30 | Rayleigh Criterion for Resolution | θ=1.22Dλ | Limit of resolution |