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Chapter 02 · Part IV · Optics
Revised on ____________________
Chapter 02 · Wave Optics

Add the amplitudes, and mind the half wavelength

2 sheets
2 diagrams
28 results

Formulas and conditions only — no derivations, no solved numbers. The diagrams are the reader's own.

I

Interference, in general

AMPLITUDES ADD, NOT INTENSITIES
I.Resultant intensity  I = I1 + I2 + 2√(I1I2) cos φ
II.Phase from path  φ = λ Δ
III.Maxima and minima  Imax = (a1 + a2 , Imin = (a1 − a2
IV.Equal sources  I = 4I0 cos² ( φ2 )
V.Contrast  ImaxImin = ( a1 + a2a1 − a2
VI.Coherence  a locked phase relation — not merely one colour
Two independent lamps of the same wavelength produce no fringes: their relative phase scrambles billions of times a second. This is why Young split one beam instead of using two sources.
II

Young's double slit

THE MEDIUM SHRINKS EVERYTHING
I.Path difference  Δ = d sin θ ≈ d yD
II.Bright fringes  Δ = n λ
III.Dark fringes  Δ = (n − 12) λ
IV.Fringe width  β = λ Dd
V.In a medium n  β → βn every wavelength becomes λ/n
VI.Slab over one slit  shift = (n − 1) t Dd toward the covered slit
VII.Missing orders  da = an integer
VIII.White light  the centre is white, then violet inward
S₁S₂dscreenPΔ = d sinθDθ
III

Thin films

ONE REFLECTION FLIPS, THE OTHER DOES NOT
I.Extra path on reflection  λ2 at the denser-medium face only
II.Bright in reflection  2 n t cos r = (m + 12) λ
III.Dark in reflection  2 n t cos r = m λ
IV.Transmission  the two conditions swap
V.Anti-reflection coat  t = λ4 n n between air and glass
VI.A very thin film  dark in reflection t → 0 leaves only the λ/2
airfilm (index n)airtr₁ (π flip · +λ/2)r₂ (extra 2nt·cos r)rbright: 2nt·cos r = (m + ½) λ
IV

Diffraction and resolution

a sinθ = nλ IS A MINIMUM
I.Single-slit minima  a sin θ = n λ n = 1, 2, 3 … never 0
II.Central maximum  width = 2 λ Da twice every other fringe
III.Circular aperture  θmin = 1.22 λD resolution — set by aperture, not magnification
IV.Grating  d sin θ = n λ here it is a maximum
V

Polarisation, and where the marks go

TRANSVERSE ONLY
I.Through a polariser  I = I02 unpolarised light, any orientation
II.Malus's law  I = I0 cos² θ already-polarised light
III.Brewster's angle  tan θB = n reflected ray fully polarised
IV.Then  the reflected and refracted rays are perpendicular
Where marks are lost in this chapter
1Dropping the λ/2 at a denser-medium reflection. Every bright and dark condition inverts with it.
2Reading a sin θ = nλ as a maximum. For one slit it locates the minima; for two slits d sin θ = nλ is a maximum.
3Adding intensities for coherent beams. Add amplitudes and square, or the dark fringe never reaches zero.
4Quoting the vacuum wavelength inside a liquid. In a medium λ → λ/n, and β shrinks with it.