A What you learned in 123 “Normal incidence” We have complete picture in 471: All angles Polarization (refers to E direction, not to polarized atoms) Complex index (next time)
Break linear polarization into two components Plane of incidence vs interface plane
Equations we must write: Unknowns we want to solve for: Any one of these gives us: Frequency cons. Reflection law Snell’s law Amazing!
n=2 n=1 Huygen’s principle and Snell’s law: Each point of space or matter can be imagined as a point source of forward semicircular waves. The sum of the circular wavefronts gives a wavefront of the real wave. Points farther down the interface are ahead in phase. They emit waves with different wavelength. wave turns
Photon picture of Snell’s law Photon energy Photon momentum From our findings for k and across the interface, which is not conserved? Photon energy Photon momentum perpendicular to interface Photon momentum parallel to interface All are conserved None are conserved
The B field that must accompany E t p is_______. a)Parallel to E t p b)antiparallel to E t p c)Into the page d)Out of the page e)Along k
The B field that must accompany E t p has magnitude _____ a)nE t p /c b)ncE t p c)cE t p /n d)E t p /(cn) e)E t p /c
Fresnel Coefficients
Suppose we have a laser beam entering a piece of glass under special conditions so R = 0. What is the same for both beams? Beam intensity Beam power both neither
R and T from r and t
References Wave amplitude, energy and N-photons The beam is focused to an area A. What is the average amplitude of the E-field? A laser puts out power P (watts): How many photons per second leave it? What is the photon density photons/m 3 in this case?
Suppose we have a laser beam entering a piece of glass at normal incidence. Assume it’s anti-reflection coated so we can ignore reflection. In the glass the photons move slower. The energy density u is ____ than in air. larger smaller the same Photon picture