Properties of Light. 1. The Speed of Light 2. The Propagation of Light 3. Reflection and Refraction 4. Polarization

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Chapter 33 - Light

Properties of Light 1. The Speed of Light 2. The Propagation of Light 3. Reflection and Refraction 4. Polarization MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 2

Electromagnetic Spectrum of Radiation The visible spectrum runs from about 4000 Å to 8000 Å or 400nm to 800nm. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 3

Electromagnetic Spectrum of Radiation Ultraviolet 400nm λ 700nm Infrared Short wavelength Long wavelength Violet Red High Energy λf = c E = hf Low Energy Planck s constant h = 6.626x10-34 Js = 4.136x10-15 ev-s MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 4

The Propagation of Light MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 5

Electromagnetic Waves In Optics we treat light (EM radiation) as a wave. We ignore the B vector and treat the E vector only when it comes to polarization. The orientation of the E vector can be manipulated. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 6

Propagation Vectors are Light Rays Wave fronts of plane waves MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 7

Fermat s Principle The path taken by light traveling from one point to another is such that the time of travel is a minimum. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 8

http://hyperphysics.phy-astr.gsu.edu/hbase/phyopt/fermat.html MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 9

Spherical Wave Front MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 10

Wave Fronts and Rays A light wave can be represented by a wave front which is useful for discussing certain aspects of wave propagation. A vector that is normal to the wave front is called a light ray. For tracing light through a transparent material the light ray formalism is more useful MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 11

Huygens Principle Each point on a primary wavefront serves as the source of spherical secondary wavelets that advance at the wave speed for the propagating medium. The primary wavefront at some later time is the envelope of these wavelets. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 12

Transformation of the Wave Front MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 13

Transformation by Elastic Scattering Scattering of electromagnetic radiation (light) is described physically as elastic absorbtion and re-radiation (emission). The word elastic means that no energy is lost in the scattering process. This absorbtion and emission process takes time. It makes the light appear to be traveling slower when passing through a transparent material such as glass. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 14

Transformation by Elastic Scattering λf = c E = hf In free space the speed of light is a constant. EM radiation travels at the speed of light or it doesn t exist at all. Between the absorption and emission processes the EM wave doesn t exist. Its energy is in the absorbing atom or molecule. It is convenient to describe the passage of light through a transparent material as traveling slower rather than describing the details of the absorbtion and emission. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 15

Transformation of the Wave Front λf = c E = hf = h c λ Notice that the portion of the wave front that went through the thickest piece of glass is the farthest behind. This is because the speed of the wave slows down in glass. Remember this is elastic scattering - energy is conserved. The wavelength and speed must both decrease to maintain constant E. Planck s constant h = 6.626x10-34 Js = 4.136x10-15 ev-s MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 16

Wavelength in a Medium For all waves λf = v In a medium λ and v change ' λ has a velocity v in the medium ' λ f = v λ c ' = or λ = = ' λ v c ' Since n > 1 λ <λ λ λ n v Therefore λ decreases in a transparent material MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 17

Reflection and Refraction MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 18

Incident ray Reflection and Refraction Angle of incidence: θ 1 Angle of reflection: θ 1 Reflected ray Refracted ray Angle of refraction MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 19

Reflection and Refraction Incident waves Reflected waves Semicircular glass disk Refracted waves Ultrasonic waves in water reflecting off a steel plate. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 20

Multiple Reflection and Refraction Incident Light MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 21

Mirror Reflection MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 22

Reflection From a Rough Surface Smooth and rough are relative terms. Variations are large or small relative to the wavelength of the light. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 23

Snell s Law n sinθ = n sinθ All angles are measured 1 1 2 2 from the surface normal. sinθ = 1 2 1 n2-1 n1 θ = sin sinθ 2 1 n2-1 1.00 0 θ = sin 2 sin45 1.33-1 θ = sin 0.751 x 0.707 2 2 n θ = 32.1 0 sinθ ( ) MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 24

Snell s Law n1sinθ 1 = n2sinθ2 All angles are measured from the surface normal. More dense to less dense - bend away from the normal. Less dense to more dense - bend toward the normal. The reverse pathway of the light beam also satisfies Snell s Law. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 25

Index of Refraction c v f = = = constant frequency λ λ n v λ λ c λ = = = ; where n = n c c n v λ v The constant n is the index of refraction and is material and frequency dependent. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 26

Total Internal Reflection Total internal reflection requires light going from a more dense material to a less dense material. θ = 90 2 0 n sinθ = n sinθ 1 1 2 2 sinθ = c n n n 2 1 2 sinθ c = n 1 sin90 0 MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 27

Total Internal Reflection MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 28

The Geometry of Internal Reflection How do you get the light source inside the glass? MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 29

Typical Internal Reflection Problem Total internal reflection condition Two types of questions: n 2 (1) How big is the circle? (2) How deep are you? R tanθ c = sinθ = y n 2 ; c n1 n 2 = 1.00; n 1 = 1.33 n 1 R = 2.0m -1 1.00 0 θ = sin c = 48.8 1.33 R 2.00 y = = = 1.75m tanθ tan 48.8 c ( ) MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 30

Reflection via Wave Front Generation MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 31

Special Case - Normal Incidence I 0 = Incident intensity I = Reflected intensity n - n 1 2 I = n + n 1 2 2 I 0 For a typical case n 1 = 1.0, n 2 = 1.5 I 0 I = 25 Reflected intensity ~ 4% Transmitted intensity ~ 96% MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 32

Index of Refraction versus Frequency The dependence of the index of refraction with frequency is referred to as dispersion MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 33

Dispersion of Light n sinθ = n sinθ 1 1 2 2 By measuring the prism and deflection angles, a very precise determination of the index of refraction to 6 decimals places. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 34

Rainbow Formation MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 35

Viewing the Primary Rainbow A rainbow is the result of light scattering from many water droplets viewed from a particular angle. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 36

Viewing the Primary Rainbow The light source needs to be behind the observer. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 37

A Rainbow is the Result of Internal Scattering of Light within Water Drops Secondary - Double Scattering Primary - Single Scattering MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 38

Primary Rainbow Geometry Refraction Reflection Scattering angle Refraction Water droplet MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 39

Descartes s Construction of Parallel Rays Entering a Spherical Water Drop Rays exit at increasing angles up until ray #7. This maximum angle is about 42 0. The concentration of the exiting rays around this maximum angle gives rise to the rainbow effect. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 40

From Atmospheric Optics http://www.atoptics.co.uk/rainbows/primary.htm MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 41

Polarization MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 42

Optical Scattering Scattering of electromagnetic radiation (light) is described physically as elastic absorbtion and reradiation (emission). The elastic description means that no energy is lost in the scattering process. The process can be visualized be treating the scattering atoms as little dipole antennas. These little antennas have maximum radiation in the direction perpendicular to the antenna and no radiation along the axis of the antenna.. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 43

Polarization by Scattering Incident light polarized along the x-direction cannot produce radiation polarized in the x-direction. Incident light polarized along the y-direction cannot produce radiation polarized in the y-direction. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 44

Microwave Polarization Example The electric field vector of the microwave radition is oriented in the vertical direction. The wires in the grating on the left are oriented parallel to the electric vector and absorb energy and hence the microammeter gives a low reading. The grating wires on the right are perpendicular to the microwave electric vectors. Therefore they do not absorb any energy and hence the high reading on the microammeter. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 45

Polarization by Scattering Ordinary light incident from the left At the polarizing angle, known as Brewster s angle, the angle between the reflected ray and the refracted ray is 90 0 MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 46

Polarization by Scattering Plane polarized light incident from the left n sinθ = n sinθ 1 p 2 2 θ = 90 -θ 0 2 p n sinθ = n cosθ ( 0 ) n sinθ = n sin 90 -θ 1 p 2 p 1 p 2 p n 2 tanθ p = n 1 The separation of the electric vectors indicate the wavelength. The vectors are closer inside the glass because the wavelength is shorter in the glass. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 47

Polarization by Scattering MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 48

Polarization by Scattering MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 49

Crossed Polarizers MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 50

Birefringence MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 51

Crystals vs Glass Glass is described as an amorphous, homogenous and isotropic material Amorphous = It has no preferred directions such as found in a crystal. Homogenous = Every part of the material is exactly like every other part of the material. Isotropic = All directions in the material are the same. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 52

Crystal Structure MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 53

Crystals vs Glass Crystals are defined by their symmetry under rotation. A cubic crystal such as NaCl is not amorphous but it can still be described as isotropic because its properties are the same in all three directions. If a crystal is described by two different indices of refraction then we say the crystal exhibits axial symmetry. This symmetry axis is referred to as the optic axis Ordinary ray - electric vector perpendicular to optic axis. Extraordinary ray electric vector is parallel to the optic axis. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 54

Crystal Symmetries The Index of Refraction Ellipsoid 1. Type I: These include Si, GaAs and CdTe. They have cubic symmetry; 3 equivalent directions; n 1 = n 2 = n 3 ; the ellipsoid is a sphere; the material is isotropic. 2. Type II: These include calcium carbonate, quartz, LiNb, calcium sulfide. They have trigonal, tetragonal or hexagonal structure. There is one axis of symmetry, which is one of the principal axes. Thus, n 1 = n 2 n 3. The ellipsoid is an ellipse with one axis along the 3-direction, rotated around the 3-axis. That is, the ellipsoid exhibits the same symmetry as the crystal. Such crystals are called uniaxial. 3. Type III: These crystals have two axes of symmetry n 1 n 2 n 3 and so are called biaxial. The structure is orthorhombic, monoclinic or triclinic. All three principal axes of the ellipsoid are different. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 55

Uniaxial Crystal An uniaxial crystal is isotropic within the plane orthogonal to the optical axis of the crystal. This demonstrates that the optic axis a symmetry axis of the crystal under rotations. The refractive index of the ordinary ray (electric vector perpendicular to optic axis) is constant for any direction in the crystal. The refractive index of the extraordinary ray (electric vector parallel to the optic axis) is variable and depends on the direction. Non-crystalline materials have no double refraction and thus, no optic axis. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 56

Polarization By Birefringence Light propagation in the material is at an arbitrary angle relative to the optic axis. The ordinary ray has its electric vector perpendicular to the optic axis. The extraordinary ray s electric vector makes an angle with the optic axis. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 57

Birefringence MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 58

Optic Axis Prepares the light with the desired polarization The next slide shows the light exiting the Crystal plate. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 59

Ordinary and Extraordinary Light Rays The e ray experiences a different n e than the o ray n o The e ray will get out of phase with the o ray. In effect the optic material acts to rotate the direction of the electric field vector. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 60

Birefringence Spherical and ellipsoidal waves diverge from point S in a birefringent crystal Old name An example of Huygen's wavelets. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 61

Birefringence (b) Light traveling in the direction of the optic axis, (c) perpendicular to the optic axis, and (d) at an arbitrary angle to the optic axis. In case (c) there is no separation or shifting of the two polarization states but they are traveling at different speeds inside the material. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 62

Birefringence The optic axis determines the orientation of the propagation ellipsoid. Wavefront for the two rays. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 63

Ordinary and Extraordinary Light Rays Polarization in the plane of O.A. Rays separated for ease of viewing Polarization perpendicular to the plane of O.A. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 64

Ordinary and Extraordinary Light Rays Rays separated for ease of viewing MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 65

Crossed Polarizing Sheets MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 66

Crossed Polarizing Sheets for Analysis A polarizing sheet transmits light polarized parallel to the optic axis. The first sheet prepares the polarization in the vertical direction. The second sheet only allows light through that is polarized in the horizontal direction. As a result no light is transmitted. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 67

Crossed Polarizing Sheets for Analysis We are interested in the physical properties and phenomena taking place in the object between the polarizers. An object placed between the crossed polarizers can affect the light passing through it. By changing the plane of the polarization some of the light will now be transmitted through the final sheet. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 68

Shocked and Unshocked Quartz Crystals Quartz crystal grain from meteorite site Quartz crystal grain from volcanic rocks The shock of the impact is evident in the parallel lines in the crystal on the left. The crystal on the right exhibits no such shocked features. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 69

CO 2 Trapped in Antarctic Ice Cores 194 m deep - 1600 years old 56 m deep - 450 years old The trapped CO 2 in the thin slices of ice core appear as amber colored bubbles. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 70

Stressed Plastic Increased stress at point of tight curves. Uniform color of light at points of low stress. A portion of a stressed French Curve between crossed polarizers. MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 71

Stressed Plastic MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 72

Chartres Cathedral Chartres France MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 73

Chartres Cathedral thru Crossed Polarizers MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 74