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Ch 35 Interference The colors in many of a hummingbird’s feathers are not due to pigment. The iridescence (虹彩) that makes the brilliant colors that often appear on the throat and belly (腹部) is due to an interference effect caused by structures in the feathers. The colors will vary with the viewing angle. Examples of Interference The bright colors of peacock feathers are also due to interference. In both types of birds, structures in the feathers split and recombine visible light so that interference occurs for certain colors. The blue of the top surface of a Morpho butterfly wing is due to optical interference and shifts in color as your viewing perspective changes. Examples of Interference Governments worldwide scurry to stay ahead of counterfeiters (偽造者) who are quick to use the latest technology to duplicate paper currencies. Some of the security measures now used to thwart counterfeiters are security threads and special watermarks (both of which can be seen if the currency is held up against a light) and microprinting (which consists of dots too small to be picked up by a scanner). The feature that is probably the most difficult for a counterfeiter to duplicate is the variable tint that results from color-shifting inks. For example, the “100” in the lower right of the front face of a U.S. $100 bill contains color-shifting ink. If you look directly down on the number, it is red or red-yellow. If you then tilt the bill and look at it obliquely, the color shifts to green. A copy machine can duplicate color from only one perspective and therefore cannot duplicate this shift in color you see when you change your perspective. One of the major goals of physics is to understand the nature of light. This goal has been difficult to achieve simply because light is complicated (Einstein had ever said that). This complication means that light offers many opportunities for applications, and some of the richest opportunities involve the interference of light waves — optical interference. Huygens The first person to advance a convincing wave theory for light was Dutch physicist Christian Huygens, in 1678. Although much less comprehensive than the later electromagnetic theory of Maxwell, Huygens’ theory was simpler mathematically and remains useful today. Its great advantages are that it accounts for the laws of reflection and refraction in terms of waves and gives physical meaning to the index of refraction. Huygens’ wave theory: where a given wavefront of optical wave will be at any time in the future if we know its present position. This construction is based on Huygens’ principle: 惠更斯原理: 光波波前上的每一點都可視為一新的波源, 以 波 速 向 四 面 八 方 擴 散 出 球 面 次 級 子 波 (secondary wavelets),經過一段時間後,這些次級子波的公切面[即 包跡(envelope)]將形成新的波前。 A given wavefront (plane ab) at t=0, where will the wavefront be at time Δt later ? Sources of spherical secondary wavelets (次級子波波源) At time Δt, the radius of all these spherical wavelets will have grown to cΔt. ¨ New wavefront (各 次級子波的公切面) Fig. 35-2 We can use Huygens’ principle to derive the law of refraction: n1sinθ1=n2sinθ2. λ1 and λ2: wavelength in medium 1 and 2 v1 and v2: velocity of light in air and in glass (v1>v2) 位於波峰之波前 Fig. 35-3 <由惠更斯原理出發推導光波折射定律> [Fig. 35-3a] θ1: angle between the incident wavefront and the interface = angle of incidence (亦即入射角). Self-study [Fig. 35-3b] As the wave moves into the glass, point “e” (由惠更斯原理知波前上 每一點都可當成一新的波源) will expand to pass through point “c”, at a distance of λ1 from point “e”. ¨ Δt1=λ1/v1. Now note that in this same Δt, point “h” (另一新的波源) will expand to pass through point “g”, at the reduced speed v2 and with λ2. ¨ Δt2=λ2/v2. By Δt1 = Δt2, we obtain Fig. 35-3 θ 2: angle between the refracted wavefront and the interface, is actually the angle of refraction (亦即折射角). For the right triangles “hce” and “hcg” in Fig. 35-3b we may write Fig. 35-3 Dividing the first of these two equations by the second and using Eq. 35-1, we find We can define the index of refraction n for each medium as the ratio of the speed of light in vacuum c to the speed of light v in the medium. Thus, In particular, for our two media, we have If we combine Eqs. 35-2 and 35-4, we find ¨ 1 The wavelength of light changes when the speed of the light changes, as happens when light crosses an interface from one medium into another [Eq. (35-1): v1/v2=λ1/λ2]. 2 The speed of light in any medium depends on the index of refraction of the medium (n=c/v)(進入介質,波速變慢 n倍). By 12, λ of light in any medium depends on “n” of the medium. Let a certain monochromatic light have wavelength λ and speed c in vacuum and wavelength λn and speed v in a medium with an index of refraction “n”. From Eq. 35-1 Using Eq. 35-3 yields This equation tells us that the greater the index of refraction of a medium, the smaller the wavelength of light in that medium (進入介質,波長變短n倍) What about the frequency of the light? Let fn represent the frequency of the light in a medium with index of refraction n. Then from the general relation of Eq. 16-13 (v=λ/T=λf), we can write Substituting Eqs. 35-8 into fn then gives us where f is the frequency of the light in vacuum. Although the speed and wavelength of light in the medium are different (reduced) from what they are in vacuum, the frequency of the light in the medium is the same as it is in vacuum. Equation 35-8 is important in the interference of light waves. In Fig. 35-4, waves 1 and 2 have identical wavelengths λ and are initially in phase in air (n ≈ 1). One of the waves travels through medium 1 (n1) and length L. The other travels through medium 2 (n2) and the same length L. When the waves leave the two media, they will have the same wavelength — their wavelength λ in air. However, because their wavelengths differed in the two media, the two waves may no longer be in phase after exiting the media. Wave 2 Wave 1 In phase (phase difference=0) Not in phase (new phase difference≠0) Fig. 35-4 To find their new phase difference in terms of wavelengths, we count the number N1 of wavelengths there are in the length L of medium 1. The wavelength in medium 1 is λn1=λ/n1; so We count the number N2 of wavelengths there are in the length L of medium 2, where the wavelength is λn2=λ/n2: Assuming n2 > n1, we obtain Suppose Eq. 35-11 tells us that the waves now have a phase difference of 45.6λ. A shift of an integer number of wavelengths (such as 45λ) would put the waves back in phase; so it is only the decimal fraction (0.6λ) that is important. ¨ A phase difference of 45.6λ is equivalent to an effective phase difference of 0.6λ. 1 A phase difference of 0.5λ (半個波長) puts two waves exactly out of phase (完全反相). If the waves had equal amplitudes and were to reach some common point, they would then undergo fully destructive interference (完全破壞 性干涉), producing total darkness at that point. 2 With a phase difference of 0λ or integer×λ, they would undergo fully constructive interference (完全建設性干涉), resulting in maximum brightness at the common point. 3 Our phase difference of 0.55λ is an intermediate situation but closer to fully destructive interference, and the waves would produce a dimly (灰暗の) illuminated common point. We can also express phase difference in terms of radians and degrees. A phase difference of one λ is equivalent to phase differences of 2π radius or 360o. → Δφ = 2π(N2-N1) = (2π/λ)L(n2-n1) In Section 33-8, we discussed how the colors of sunlight are separated into a rainbow when sunlight travels through falling raindrops. Here we can see that different parts of an incoming wave will travel different paths within the drop. That means waves will emerge from the drop with different phases. Thus, we can see that at some angles (~42o) the emerging light will be in phase and give constructive interference. The rainbow is the result of such constructive interference. in phase (a) By the phase difference between the two waves via the media: (b) Here the effective phase difference of 0.84 wavelength is > 0.5 wavelength (for fully destructive interference) < 1.0 wavelength (for fully constructive interference), but ~ 1.0 wavelength. Thus, the waves would produce intermediate interference that is closer to fully constructive interference — they would produce a relatively bright spot. Example of diffraction At a beach in Israel, plane water waves pass through two openings in a breakwall. Notice the diffraction effect — the waves exit the openings with circular wave fronts. Notice also how the beach has been shaped by the circular wave fronts. In the next section we shall discuss the experiment – young’s double-slits interference – that first proved that light is a wave. To prepare for that discussion, we must introduce the idea of diffraction of waves: If a wave encounters a barrier that has an opening of dimensions similar to the wavelength (a~λ), the part of the wave that passes through the opening will spread out — will diffract — into the region beyond the barrier. a λ Fig. 35-6 An incident plane wave of wavelength λ encounters a slit that has width a=6.0λ. The part of the wave that passes through the slit flares out (呈喇叭狀展開) on the far side. Figures 35-7b (with a=3.0λ) and 35-7c (a=1.5λ) illustrate the main feature of diffraction: “the narrower the slit, the greater the diffraction.” Fig. 35-7 The narrower the slit, the greater the diffraction. Diffraction limits geometrical optics, in which we represent an EM wave with a ray: If we actually try to form a ray by sending light through a narrow slit, or through a series of narrow slits, diffraction will always defeat our effort because it always causes the light to spread. Indeed, the narrower we make the slits, the greater the spreading is. Thus, geometrical optics (ray optics) holds only when slits or other apertures (孔洞) do not have dimensions comparable to or smaller than the wavelength of the light (that is, a >> λ) such that the diffraction effect can be neglected. In 1801, Thomas Young first experimentally proved that light is a wave, contrary to (對立於) what most other scientists then thought ̶ light is particle-like, not a wave. He did so by demonstrating that light undergoes interference, as do water waves, sound waves, and waves of all other types (視為波才會有 干涉現象,視為粒子則不會). In addition, Young was able to measure the average wavelength of sunlight; his value, 570 nm, is impressively close to the modern accepted value of 555 nm. Diffraction Diffraction of the light by these two slits sends overlapping cylindrical waves into the region between screens B and C, where the waves from one slit interfere with the waves from the other slit. Interference between two diffracted waves from S1 & S2 Monochromatic (單色光) Fig. 35-8 Basic arrangement of Young’s experiment. A interference of the overlapping waves shows on screen C: 1 Bright regions → fully constructive interference → bright fringes (maxima) 2 Dark regions → fully destructive interference → dark fringes (minima) h The pattern of bright and dark fringes on screen C is called an interference pattern. bright fringes Fig. 35-9 Interference pattern dark fringes screen C What exactly determines the locations of the interference fringes ? We pick an arbitrary point P on screen C, at angle θ (方位角) to the central axis. This point intercepts the wave of ray r1 from the bottom slit and the wave of ray r2 from the top slit. Incident waves are in phase when they arrive S1 & S2 because there they are just portions of the same incident wave. However, once they have passed the slits, the two waves must travel different distances to reach P via r1 & r2, respectively. h 產 生 phase difference Central axis Fig. 35-10a ¨ 到達不同觀察點P,r1 與r2 走的路徑差不同→相位差不同→ 亮暗程度不同 Consider two waves initially exactly in phase, traveling along paths with a path length difference ΔL, and then arriving at some common point P. 1 When ΔL=mλ (m=0, 1, 2…), the waves arrive at P exactly in phase and they interfere fully constructively there. → bright fringe 2 When ΔL=(m)λ/2 (m=1, 3, 5…), the waves arrive at P exactly out of phase and they interfere fully destructively there. → dark fringe The path length difference ΔL (between r1 & r2) = S1b: As the distance from the slits to the observed point of the screen >> the slit separation, we can approximate rays r1 and r2 as being parallel to each other and at angle θ to the central axis (Fig. 35-10b). We can also approximate the triangle formed by S1S2b as being a right triangle, and approximate the angle inside that triangle at S2 as being θ. Fig. 35-10b Then, sinθ = ΔL/d and thus Fig. 35-10b ΔL 1 For a bright fringe, we saw that ΔL=mλ (m=0, 1, 2…). We can write this requirement as ¨ For m=0, Eq. 35-14 tells us that a bright fringe is at θ=0 and thus on the central axis. This central maximum ( 中 央 極 大 ) is the point at which waves arriving from the two slits have a path length difference ΔL=0, hence phase difference=0. For m=2, Eq. 35-14 tells us that bright fringes are at the angle Waves from the two slits arrive at these two fringes with ΔL=2λ and with a phase difference of 2λ. These fringes are said to be the second-order bright fringes (m=2) or second maxima. 2 For a dark fringe, ΔL=(m)λ/2 (m=1, 3, 5…). We can write this requirement as ¨ For m=1, Eq. 35-16 tells us that dark fringes are at the angle Waves from the two slits arrive at these two fringes with ΔL=1.5λ. These fringes are called the second-order dark fringes or second minima. (The first dark fringes, or first minima, are at locations for which m=0 in Eq. 35-16.) 第 一 極 大 第 二 極 小 中 央 極 大 第 一 極 小 第 一 極 大 第 一 極 小 第 二 極 小 By Fig. 35-10a (mth 階亮紋發生的位置) From Eq. 35-14 (mth 階亮紋發生條件) Then using the approximation sinθ ≈ tanθ for small θ P For the interference pattern to appear on screen C, the two light waves from S1 and S2 reaching any point P on the screen must have a phase difference that does not vary in time. → That is the case in Fig. 35-8 because the waves passing through slits S1 and S2 are portions of the single light wave that illuminates the slits. Because the phase difference remains constant (不隨時間變化) at any point of P on screen C, the light from slits S1 and S2 is said to be completely coherent (同調/相干). If we replace the double slits with two similar but independent monochromatic light sources, the phase difference between the two waves emitted by the two sources varies rapidly and randomly. h The two waves are not coherent. P φ1(t) φ2(t) Δφ(t) at P changes with time randomly & rapidly Δφ(t) changes with time randomly & rapidly As a result, at any given point P on the viewing screen, the interference between the waves from the two sources varies rapidly and randomly【phase difference varies rapidly and randomly because the phase change of each wave is as quickly as > 109 Hz】between fully constructive and fully destructive during the response time of human eyes. The eye cannot follow such rapid changes, and no (longterm stable) interference pattern can be seen. The fringes disappear, and the screen is seen as being uniformly illuminated. Equations 35-14 and 35-16 show the maxima and minima of the double-slit interference pattern as a function of the angle θ ( 方 位 角 ). Here we wish to get an expression for the intensity I of the interfering fringes as a function of θ h I=I(θ) Assuming that the light waves from the two slits are not in phase when they arrive at point P. The electric field components of those waves at point P are not in phase and vary with time as Phase difference (由於路徑差造成): φ Because the phase difference does not vary with time (φ = const.), the two waves are coherent. These two waves will combine at P to produce an intensity I given by dsinθ = 路徑差 I0: intensity of the light through S1 or S2. Equations 35-22 and 35-23, which necessarily contain information about the location of the maxima and minima. (1) The intensity maxima will occur when (from Eq. 35-22) If we put this result into Eq. 35-23, we find ¨ which is exactly Eq. 35-14. (2) The minima in the fringe pattern occur when (from Eq. 35-22) If we combine this relation with Eq. 35-23, we are led to which is just Eq. 35-16. Figure 35-12 (a plot of Eq. 35-22) shows the intensity of the double-slit interference pattern as a function of φ. The horizontal solid line is I0. Note in Eq. 35-22 and the graph that the intensity I varies from 0 at the fringe minima to 4I0 at the fringe maxima. Fig. 35-12 If the waves from the two sources (slits) were incoherent, so that no enduring (固定の) phase relation existed between them (相位差隨時間瞬時任意變化), there would be no fringe pattern and the intensity would have the uniform value 2I0 for all points on the screen. Interference cannot create or destroy energy but merely redistributes ( 重 新 分 佈 ) it over the screen. Thus, the average intensity on the screen must be the same 2I0 regardless of whether the sources are coherent. This follows from Eq. 35-22; if we substitute ½, the average value of the cos2-function, this equation reduces to Iavg=2I0. → Self-study (利用相量作圖法) The phase difference φ between E1 and E2 is associated with the path length difference S1b. If S1b is λ/2, then φ is π; if S1b is λ, then φ is 2π, and so on. This suggests 相位差 = (2π/λ)×路徑差 (important!!) Fig. 35-10b Fig. 35-10b The path length difference S1b in Fig. 35-10b is dsinθ ; so Eq. 35-30 for the phase difference between the two waves arriving at point P on the screen becomes which is same as Eq. 35-23. The colors we see when sunlight illuminates a soap bubble or an oil slick on the road are caused by the interference of light waves reflected from the front and back surfaces of a thin transparent film. The thickness (L) of the soap or oil film (for causing the interference fringes) is typically of the order of magnitude of the wavelength of the (visible) light involved. (L~λ) Figure 35-15 shows a thin transparent film (thickness L, index of refraction n2) illuminated by bright light of wavelength λ from a distant point source. Assuming that n1=n3=nair. For simplicity, θ ≈ 0o. air air θ≈0o λ Fig. 35-15 thin film If reflected waves r1 and r2 are exactly in phase at the eyes ¨ interference maximum and region ac on the film is bright to the observer. If reflected waves r1 and r2 are exactly out of phase (相差180o), they produce an interference minimum and region ac is dark to the observer. If reflected waves r1 and r2 have some intermediate phase difference, there are intermediate interference and brightness. air air θ≈0o λ Fig. 35-15 thin film The key to what the observer sees is the phase difference between reflected waves r1 and r2. Because θ (入射角) is ~ 0o, we approximate the path length difference (路徑差) between the waves r1 and r2 as 2L (r2在n2薄膜內多走了2L). However, to find the phase difference between the waves, we cannot just find the number of wavelengths λ that is equivalent to a path length difference of 2L. This simple approach is impossible for two reasons: air (i) The path length difference occurs in a medium other than air (因為在 介質中折射率與在空氣中不同). (ii) Reflections are involved, which can change the phase. air θ≈0o λ Fig. 35-15 thin film Refraction at an interface never causes a phase change — but reflection can, depending on the indexes of refraction on the two sides of the interface. Figure 35-16 shows what happens when reflection causes a phase change, using as an example pulses on a denser string and a lighter string. Similarly, for light (光密→光疏) (光疏→光密) denser lighter 同相 同相 denser lighter 同相 反相 Fig. 35-16 There are 3 ways in which the phase difference between two waves can be generated: 1. by reflection 2. by the waves traveling along paths of different lengths (路徑差) 3. by the waves traveling through media of different indexes of refraction (折射率差) When light reflects from a thin film, producing the waves of rays r1 and r2 shown in Fig. 35-15, all 3 ways described above are involved. air air θ≈0o λ Fig. 35-15 thin film <反射造成相差之解析> 反射造成相差之解析 On the 1st interface, the incident wave (in air) reflects from the medium n2 (n2>nair) ; so the wave r1 has its phase shifted by wavelength (π radius 或 180o). On the 2nd interface, the incident wave reflects from the medium (air) having the lower of the two indexes of refraction; so the wave r2 reflected there is not shifted in phase by the reflection. 1st So far, as a result of the reflection phase shifts, the waves of r1 and r2 have a phase difference of wavelength and thus are exactly out of phase (相差180o). 2nd r2 r1 incident light Fig. 35-17 < 光程差(路徑差×折射率)與反射造成相差之解析> 與反射造成相差之解析 n If the reflected waves of r1 and r2 are to be exactly in phase so that they produce fully constructive interference, the path length 2L must contribute an additional phase difference of 0.5, 1.5, 2.5, . . . wavelengths. Then the net phase difference [ 路徑差×折射率+反射(π或 λ)] is an integer number of wavelengths. Thus, for a bright film (完 全建設性干涉), we must have λn2: the light in the medium with n2 Fig. 35-17 o If the waves are to be exactly out of phase so that there is fully destructive interference, the path length 2L must contribute an additional phase difference of 0, 1, 2, 3, . . . wavelengths. Then the net phase difference be an odd number of half-wavelengths. For a dark film (完全破 壞性干涉), we must have λn2: the light in the medium n2 Fig. 35-17 Use Eq. 35-8 (λn=λ/n) to write the wavelength of the wave of ray r2 inside the film as where λ is the wavelength of the incident light in vacuum. Substituting Eq. 35-35 into Eq. 35-32 and replacing “odd number/2” with (m+) give us Similarly, with m replacing “integer,” Eq. 35-34 yields (干涉極大) (干涉極小) (L « λ) A special situation arises when a film is so thin that L << λ (L<λ/10). Then the path length difference 2L can be neglected, and the phase difference between r1 and r2 is due only to reflection phase shifts (π). → The film we see is dark, regardless of λ. L λ λ>>L Thin film Figure 35-18 shows a vertical soap film whose thickness increases from top to bottom because gravitation has caused the film to slump (下降). L<<λ → dark (r1與r2反相,破壞性干涉) Color interference fringes (L夠厚,厚度造成之相差不可 忽略 → 隨厚度改變 → 不同波 長反射光在不同厚度位置產生 干涉極大 → 彩色干涉條紋) Fig. 35-18 air θ=0 λ=400-690nm water air 完全破壞性干涉 θ=0 π π Fig. 35-20 θ=0 π π Homeworks Ans: Ans: (a) 50º (b) 0.14 ps Ans: (a) 0.833 (b) intermediate but closer to fully constructive Ans: 140 bright fringes Ans: Ans: Ans: (a) 34 bright rings (b) 46 bright rings Ans: (a) 22o (b) The angle of incidence is gradually reduced due to refraction. Eventually after many refractions, θ2 will be virtually zero. This is why most waves come in normal to a shore Ans: (a) 1.6 (b) 1.4 Ans: tzig zag – tdirect =(n1L/c)-[n12L/(n2c)] =51.6 ns. Ans: x= (m+)(D/2a)λ. Ans: (a) (b) Ans: (a) (b) Ans: (a) (b)