Chapter 35, example problems:

Similar documents
6) How wide must a narrow slit be if the first diffraction minimum occurs at ±12 with laser light of 633 nm?

AP Physics B Ch. 23 and Ch. 24 Geometric Optics and Wave Nature of Light

Interference. Physics 102 Workshop #3. General Instructions

PHYS 222 Spring 2012 Final Exam. Closed books, notes, etc. No electronic device except a calculator.

Physics 10. Lecture 29A. "There are two ways of spreading light: to be the candle or the mirror that reflects it." --Edith Wharton

Physical Science Study Guide Unit 7 Wave properties and behaviors, electromagnetic spectrum, Doppler Effect

Physics 41 Chapter 38 HW Key

Solution Derivations for Capa #14

Waves and Light Extra Study Questions

v = fλ PROGRESSIVE WAVES 1 Candidates should be able to :

Diffraction of Laser Light

EXPERIMENT O-6. Michelson Interferometer. Abstract. References. Pre-Lab

INTERFERENCE OBJECTIVES PRE-LECTURE. Aims

Interference and Diffraction

Question based on Refraction and Refractive index. Glass Slab, Lateral Shift.

Waves Sound and Light

How To Understand Light And Color

Holography 1 HOLOGRAPHY

WAVELENGTH OF LIGHT - DIFFRACTION GRATING

Interferometers. OBJECTIVES To examine the operation of several kinds of interferometers. d sin = n (1)

Overview. What is EMR? Electromagnetic Radiation (EMR) LA502 Special Studies Remote Sensing

Experiment 5. Lasers and laser mode structure

The Physics of Guitar Strings

P R E A M B L E. Facilitated workshop problems for class discussion (1.5 hours)

FTIR Instrumentation

ILLUSTRATIVE EXAMPLE: Given: A = 3 and B = 4 if we now want the value of C=? C = = = 25 or 2

Rutgers Analytical Physics 750:228, Spring 2016 ( RUPHY228S16 )

Law of Cosines. If the included angle is a right angle then the Law of Cosines is the same as the Pythagorean Theorem.

Physics 202 Problems - Week 8 Worked Problems Chapter 25: 7, 23, 36, 62, 72

After a wave passes through a medium, how does the position of that medium compare to its original position?

Imaging Systems Laboratory II. Laboratory 4: Basic Lens Design in OSLO April 2 & 4, 2002

One example: Michelson interferometer

SOLUTIONS TO CONCEPTS CHAPTER 17

Spring Simple Harmonic Oscillator. Spring constant. Potential Energy stored in a Spring. Understanding oscillations. Understanding oscillations

Physics 111 Homework Solutions Week #9 - Tuesday

LIGHT REFLECTION AND REFRACTION

1 of 9 2/9/2010 3:38 PM

AP PHYSICS C Mechanics - SUMMER ASSIGNMENT FOR

Reflection and Refraction

4.4 WAVE CHARACTERISTICS 4.5 WAVE PROPERTIES HW/Study Packet

Friday 18 January 2013 Morning

Study Guide for Exam on Light

ANALYTICAL METHODS FOR ENGINEERS

STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves

Interference of Light Waves

Conceptual Physics Review (Chapters 25, 26, 27 & 28) Chapter 25 Describe the period of a pendulum. Describe the characteristics and properties of

Diffraction and Young s Single Slit Experiment

Crystal Optics of Visible Light

PHYS 101-4M, Fall 2005 Exam #3. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Physics 30 Worksheet # 14: Michelson Experiment

EDEXCEL NATIONAL CERTIFICATE/DIPLOMA UNIT 5 - ELECTRICAL AND ELECTRONIC PRINCIPLES NQF LEVEL 3 OUTCOME 4 - ALTERNATING CURRENT

C) D) As object AB is moved from its present position toward the left, the size of the image produced A) decreases B) increases C) remains the same

ATOMIC SPECTRA. Apparatus: Optical spectrometer, spectral tubes, power supply, incandescent lamp, bottles of dyed water, elevating jack or block.

Cross-beam scanning system to detect slim objects. 100 mm in

Parallel and Perpendicular. We show a small box in one of the angles to show that the lines are perpendicular.

The University of the State of New York REGENTS HIGH SCHOOL EXAMINATION INTEGRATED ALGEBRA. Thursday, August 16, :30 to 11:30 a.m.

PHYSICS 202 Practice Exam Waves, Sound, Reflection and Refraction. Name. Constants and Conversion Factors

Refraction of Light at a Plane Surface. Object: To study the refraction of light from water into air, at a plane surface.

Code number given on the right hand side of the question paper should be written on the title page of the answerbook by the candidate.

SOLVING TRIGONOMETRIC EQUATIONS

THE IMPOSSIBLE DOSE HOW CAN SOMETHING SIMPLE BE SO COMPLEX? Lars Hode

Review for Test 3. Polarized light. Action of a Polarizer. Polarized light. Light Intensity after a Polarizer. Review for Test 3.

Science In Action 8 Unit C - Light and Optical Systems. 1.1 The Challenge of light

PHYSICAL QUANTITIES AND UNITS

Absorbance Spectrophotometry: Analysis of FD&C Red Food Dye #40

(15.) To find the distance from point A to point B across. a river, a base line AC is extablished. AC is 495 meters

AP1 Waves. (A) frequency (B) wavelength (C) speed (D) intensity. Answer: (A) and (D) frequency and intensity.

9.4. The Scalar Product. Introduction. Prerequisites. Learning Style. Learning Outcomes

6. Vectors Scott Surgent (surgent@asu.edu)

Amplification of the Radiation from Two Collocated Cellular System Antennas by the Ground Wave of an AM Broadcast Station

Physics 25 Exam 3 November 3, 2009

Experiment #12: The Bohr Atom. Equipment: Spectroscope Hydrogen and Helium Gas Discharge Tubes, Holder, and Variac Flashlight

4. How many integers between 2004 and 4002 are perfect squares?

Basic Optics System OS-8515C

Waves-Wave Characteristics

DIFFRACTION AND INTERFERENCE

Waves - Transverse and Longitudinal Waves

THE BOHR QUANTUM MODEL

SOLUTIONS TO CONCEPTS CHAPTER 15

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics

1) The time for one cycle of a periodic process is called the A) wavelength. B) period. C) frequency. D) amplitude.

Ch 25 Chapter Review Q & A s

Wednesday 15 January 2014 Morning Time: 2 hours

Practice Test SHM with Answers

You must have: Ruler graduated in centimetres and millimetres, protractor, compasses, pen, HB pencil, eraser, calculator. Tracing paper may be used.

1 Laboratory #5: Grating Spectrometer

Upon completion of this lab, the student will be able to:

Review Vocabulary spectrum: a range of values or properties

Solution Derivations for Capa #13

GRID AND PRISM SPECTROMETERS

PHYSICS PAPER 1 (THEORY)

What s so special about the laser?

A Guide to Acousto-Optic Modulators

Q1. The diagram below shows the range of wavelengths and frequencies for all the types of radiation in the electromagnetic spectrum.

Giant Slinky: Quantitative Exhibit Activity

ALGEBRA 2/TRIGONOMETRY

Copyright 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

Answer the following questions during or after your study of Wave Properties. 4. How are refraction and the speed of wave in different media related?

Photons. ConcepTest ) red light 2) yellow light 3) green light 4) blue light 5) all have the same energy. Which has more energy, a photon of:

Math 115 Spring 2011 Written Homework 5 Solutions

Transcription:

Chapter 35, example problems: (35.02) Two radio antennas A and B radiate in phase. B is 120 m to the right of A. Point Q along extension of line AB. 40 m to the right of B. Frequency and wavelength can be varied. A B Q (a) Destructive interference at Q. Longest wavelength? AQ BQ = (1/2)λ 120 m = (1/2)λ λ = 240 m. (Note: If you change (1/2) to (3/2), (5/2), etc., you will get other possible shorter wavelengths. But the problem asks for the longest wavelength.) (b) Constructive interference at Q. Longest wavelength? Since AQ BQ can not be zero, we demand AQ BQ = λ. 120 m = λ λ = 120 m. (35.16) Coherent light. Frequency 6.32 10 14 Hz. Pass through two thin slits. Fall on a screen 85.0 cm away. 3 rd bright fringe occurs at ±3.11 cm on either side of center bright fringe. (a) Slit separation d. d sin θ = mλ = 3 (3 10 8 m/s / 6.32 10 14 Hz) tan θ = 3.11 cm / 85 m. But this θ is clearly very small. So sin θ tan θ ( θ in rad.) d = 3 (3 10 8 m/s / 6.32 10 14 Hz) / (3.11 cm / 85 cm) = 3.89 10-5 m or d = 3.89 10-3 cm. (Note: The unit Hz is just s 1.) (b) Location of the third dark fringe? The first dark fringe occurs midway between the center (zeroth) bright fringe and the first bright fringe. So the third dark fringe occurs midway between the second and third bright fringes. Hence we solve dθ = 2.5 (3 10 8 m/s / 6.32 10 14 Hz) to get θ = 0.0305. Multiplying it by 85 cm gives 0.0259 m, or 2.59 cm being the distance on the screen between the third dark fringe and the center of the center bright fringe. (35.26) Two antennas, 9.00 m apart. Radiate in Phase at 120 MHz. Receiver, placed 150 m from both antennas measured an intensity I 0. Receiver moved so that it is now 1.8 m closer to one antenna than to the other. (a) phase difference: = 2π 1.8 m / λ = 2π 1.8 m / (3.00 10 8 m/s / 120 10 6 Hz) = 4.524 rad. (b) Intensity at new position: I = I 0 cos 2 ( /2) = 0.4064 I 0. Why I = I 0 cos 2 ( /2)? Recall the phasor diagram at right: / 2

(35.30) Glass plate, 9.00 cm long, placed in contact with a second plate. Held at a small angle by a metal strip 0.0800 mm thick under one end. Air between the plates. Illuminated from above by light with wavelength λ = 656 nm. Number of interference fringes per centimeter? The interference is between light reflected from the bottom surface of the top plate, and the top surface of the bottom plate. Other surfaces are not relevant. (If you want to know why it is so, come to class and listen to the lectures.) The left end is the center of a dark fringe, because the lower reflection gets a 180 phase shift due to reflection by a denser medium, but not the upper Reflection, which is a reflection by a lighter medium. The difference in path lengths between the two paths is zero on the left edge, and it increases continuously to the maximum value of 2 0.0800 mm = 0.1600 mm on the right edge for light coming down essentially perpendicular to the plates (called normal incidence). The phase difference between the two paths on the right edge of the plates is 2π (path length difference / λ) = 2π (0.1600 mm / 656 nm) = 574.68 rad., but for this problem, it is only necessary to look at the part (0.1600 mm / 656 nm) = 243.9, which is slightly below 244. It means that there are almost 244 wavelengths in this maximum path-length difference. Thus the center of the 244 th dark fringe besides the one on the left edge of the plates is just outside the right edge of the plates and therefore can not be seen. But the bright fringe just to the left of this not-fully-observable dark fringe needs only a path-length difference of 243.5 wavelengths, and is therefore already fully developed. Since there is a bright fringe to the left of each dark fringe, including the first one, it is clear that the total number of bright fringes that can be seen is 244. Dividing it by 9.00 cm gives 27.11 bright fringes per centimeter that can be seen. (Note that the inverse of 27.11 number per centimeter is 0.0369 cm. This is the spacing between the neighboring bright fringes that can be seen from above.) (35.38) Michelson interferometer. Jan uses λ 1 = 606 nm. He moved the movable mirror away from him by some distance, and counted 818 bright fringes. Then Linda changes to λ 2 = 502 nm, and moved the movable mirror toward her by some distance, and counted also 818 bright fringes. The fringes moved in opposite directions across the line. Find the distances moved by the movable mirror in each case. (a) Jan moved the mirror 818 606 nm / 2 = 2.479 10-4 m away from him, and Linda moved the mirror 818 502 nm / 2 = 2.053 10-4 m toward her. (Note: Light travels to the movable mirror and back, so the distance moved by the mirror should be counted twice.) (b) The resultant displacement of the mirror = 2.479 10-4 m - 2.053 10-4 m = 0.426 10-4 m, or 4.26 10-5 m.

(35.44) Two radio antennas, 200 m apart, at A and B, radiate in phase. Frequency 5.80 MHz. Receiver at C. BC is perpendicular to AB. Find location of C for destructive interference. We need AC BC = (1/2) λ. x 2 + (200 m) 2 x = (1/2) (3 10 8 m/s / 5.80 10 6 Hz) = 25.86 m, or, after adding x to both sides and then squaring both sides, we obtain: x 2 + (200 m) 2 = x 2 + 25.86 m x + (25.86 m) 2. After simplifying, we obtain 25.86 m x = 39331 m 2, giving x = 1521 m. A B x C (35.50) Two-slit interference. The two slits are of different widths. Distant screen. Amplitude from the first slit = E. Amplitude from the second slit = 2E. (a) I ( ) =? The intensity is proportional to the net amplitude squared. A phasor diagram tells you how to find the net amplitude. For = 0, the net amplitude is 3E. For 0, the net amplitude follows the law of cosine (as suggested by the diagram): (2E) 2 + (E) 2 2 (2E) (E) cos (180 ) = 5E 2 + 4E 2 cos. The ratio of the two net amplitudes is (5/9) + (4/9) cos. Therefore, I ( ) = I 0 [(5/9) + (4/9) cos ], where I 0 is just I ( ) at = 0. (Note: To get amplitude 2E from one slit and E from the other slit, all one needs to do is to make the first narrow slit twice as wide as the second narrow slit.) (b) Graph of I ( ) = I 0 [(5/9) + (4/9) cos ] (for between -5π and +5π) : I / I 0 1 0.8 0.6 0.4 0.2-5π -15-10 -5 5 10 15 0 5π

(35.51) Red light, wavelength 700 nm, passes through two slits. Monochromatic visible light of another wavelength also passes through the two slits. Center of the third bright fringe (m = 3) of the red light appears red, with no mixture of the other color. Possible wavelength for the second visible light? We use the formula d sin θ = 3 λ 1 for the red light, and d sin θ = (m + 1/2) λ 2 for the second visible light. Clearly, It is the same d in both formulas (same two slits), and it is the same θ in both formulas (same spot on the screen). Thus we must have 3 700 nm = (m + 1/2) λ2. Taking m = 0 gives λ 2 = 1400 nm not visible, discard. Taking m = 1 gives λ 2 = 466.7 nm visible, accept. Taking m = 2 gives λ 2 = 280.0 nm not visible, discard. There is clearly no need to try larger m. So the second visible light must have the wavelength 466.7 nm. It is clear that we do not need to know d, because we can eliminate it between the two equations. (To do this problem, you need to know that visible light has wavelength between 400 nm and 700 nm.) (35.54) White light reflects at normal incidence from top and bottom surface of a glass Plate (n = 1.52). Air above and below. Constructive interference observed for λ 1 = 477.0 nm (in air). Next longer wavelength for constructive interference is λ 2 = 540.6 nm. Plate thickness t =? We must have: 2t = (m 1 +1/2) λ 1 = (m 2 +1/2) λ 2, where m 1 and m 2 are integers. (The ½ part is needed because the reflection from the top surface is from a denser medium, which gets a π phase shift, but not that from the bottom surface. Here λ 1 and λ 2 are both those in the medium with n = 1.52. So using the wavelengths in air the equation changes to 2nt = (m 1 +1/2) λ 1 = (m 2 +1/2) λ 2. Thus the ratio of λ 1 and λ 2 should be the ratio of two half odd integers. Let us first evaluate this ratio: λ 1 / λ 2 = 477 / 540.6 = 0.8824 = 15 /17 = 7.5 / 8.5. Thus m 2 must be 7 and m 1 must be 8. We therefore find t = (m 1 +1/2) λ 1 / 2n = 8.5 477.0 nm / 2 1.52 = 1334 nm = 1.334 μm. Of course, you can also obtain the same answer using t = (m 2 +1/2) λ 2 / 2n. (35.58) An oil tanker spills a larger amount of oil (n = 1.45) into the sea (n = 1.33). (a) Looking down from overhead. Predominant wavelength of light seen at where oil thickness = 380 nm? In this case, the reflection from the top surface of oil film gets a π phase shift, but not that from the bottom surface of the oil film. So to get the dominant color seen, we apply 2t = (m +1/2) λ / n, and try all integers for m until a visible wavelength is found. For m = 0, we get λ 0 = 2204 nm too long. For m = 1, we get λ 1 = 2204 nm / 3 = 734.7 nm too long. For m = 2, we get λ 2 = 2204 nm / 5 = 440.8 nm visible, accept. For m = 3, we get λ 3 = 2204 nm / 7 = 314.9 nm too short. We clearly do not need to try any larger m. Thus, the predo minant visible wavelength is 440.8 nm. Its color is blue (c.f., Table 32.1).

(b) For the predominant transmitted-light wavelength, we need destructive interference for the reflected light so no reflection occurs. Thus we solve 2t = m λ / n, and again try all integer m. For m = 1, we get λ 1 = 1102 nm too long. For m = 2, we get λ 2 = 1102 nm / 2 = 551 nm visible, accept. For m = 3, we get λ 3 = 1102 nm / 3 = 367.3 nm too short. Thus the predominant transmitted visible light has λ = 551 nm (in air). The color is green (c.f., Table 32.1).