Quick Recap — Wave Optics in Action

  • YDSE: fringe width β=λDd\beta=\dfrac{\lambda D}{d}; nn-th bright at yn=nβy_n=n\beta; in a medium ββ/n\beta\to\beta/n.
  • Thin sheet over one slit: shift =(n1)tDd=\dfrac{(n-1)tD}{d}, i.e. N=(n1)tλN=\dfrac{(n-1)t}{\lambda} fringes.
  • Single slit: first minimum asinθ=λa\sin\theta=\lambda; central maximum width =2λDa=\dfrac{2\lambda D}{a}, angular width 2λa\dfrac{2\lambda}{a}.
  • Polarisation: Malus I=I0cos2θI=I_0\cos^2\theta; unpolarised loses half at the first Polaroid; Brewster tanθB=n\tan\theta_B=n.
  • Two sources: ImaxImin=(I1+I2I1I2)2\dfrac{I_{max}}{I_{min}}=\left(\dfrac{\sqrt{I_1}+\sqrt{I_2}}{\sqrt{I_1}-\sqrt{I_2}}\right)^2; and I=Imaxcos2 ⁣ϕ2I=I_{max}\cos^2\!\dfrac{\phi}{2} with ϕ=2πλΔx\phi=\dfrac{2\pi}{\lambda}\Delta x.

Worked mini-example. λ=600\lambda=600 nm, D=1.5D=1.5 m, d=0.5d=0.5 mm: β=(600×109)(1.5)0.5×103=1.8\beta=\dfrac{(600\times10^{-9})(1.5)}{0.5\times10^{-3}}=1.8 mm; the 3rd bright fringe sits at 3β=5.43\beta=5.4 mm from the centre.