Brief History of Optics
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PHYSICS 4420 Physical Optics Fall 2017 Lecture Section 001, Physics Room 311, MWF 11:00–11:50 A.M
PHYSICS 4420 Physical Optics Fall 2017 Lecture Section 001, Physics Room 311, MWF 11:00–11:50 a.m. Recitation Sections 201, Physics Room 311, W 1–1:50 p.m. Professor: Bibhudutta Rout Rout’s Office: Physics Bldg., Room 007 Telephone: (940) 369-8127 E-mail: [email protected] Office Hours: M 9:30a.m.–10:30 a.m., and by appointment Prerequisite: PHYS 2220 Text: Principles of Physical Optics, by C.A. Bennett, Wiley 2008, ISBN 10 0-470-12212-9. A useful reference is Optics, 4th Edition, by Eugene Hecht, Pearson 2002, ISBN 0-8053-8566-5. Exams: There will be two in-class exams during the semester, and a comprehensive final exam. Exam questions will be based on material covered in the lecture, contained in the text, and in the homework assignments. There will be no makeup exams. Homework: Homework sets will be assigned and collected each week. You may collaborate on the homework, but the solutions you hand in must represent your own intellectual effort. You must present complete explanations to receive full credit. Participation: Part of your grade will be based on your participation in recitation, in which problem solutions will be discussed and students will be expected to contribute. You will also be required to give a 10 minute talk in recitation on an approved topic of interest to you related to optics and not covered in class. Grade: The grading in the course will be based on the total points earned from exams and homework as follows: Exams 20 points for each of the two in-class exams 30 points for the final Homework 20 points Participation/Attendance 10 points Total 100 points Note: This document is for informational purposes only and is subject to change upon notification. -
Fresnel Rhombs As Achromatic Phase Shifters for Infrared Nulling Interferometry: First Experimental Results
Fresnel Rhombs as Achromatic Phase Shifters for Infrared Nulling Interferometry: First experimental results Hanot c.a, Mawet D.a, Loicq J.b, Vandormael D.b, Plesseria J.Y.b, Surdej J.a, Habraken s.a,b alnstitut d'Astrophysique et de Geophysique, University of Liege, 17 allee du 6 Aout, B-4000, Sart Tilman, Belgium; bCentre Spatial de Liege, Avenue du Pre-Aily, B-4031, Liege-Angleur, Belgium ABSTRACT One of the most critical units of nulling interferometers is the Achromatic Phase Shifter. The concept we propose here is based on optimized Fresnel rhombs, using the total internal reflection phenomenon, modulated or not. The total internal reflection induces a phase shift between the polarization components of the incident light. We present the principles, the current status of the prototype manufacturing and testing operations, as well as preliminary experiments on a ZnSe Fresnel rhomb in the visible that have led to a first error source assessment study. Thanks to these first experimental results using a simple polarimeter arrangement, we have identified the bulk scattering as being the main error source. Fortunately, we have experimentally verified that the scattering can be mitigated using spatial filters and does not decrease the phase shifting capabilities of the ZnSe Fresnel rhomb. Keywords: Fresnel Rhomb, Achromatic Phase Shifters, nulling interferometry, subwavelength gratings, Zinc Selenide, bulk scattering 1. INTRODUCTION The detection of extrasolar planets and later on the presence of life on them is one of the most interesting and ambitious astrophysical projects for the next decades. Up to now, despite our technological progresses, most exoplanets have been detected using indirect methods. -
Determination of Focal Length of a Converging Lens and Mirror
Physics 41- Lab 5 Determination of Focal Length of A Converging Lens and Mirror Objective: Apply the thin-lens equation and the mirror equation to determine the focal length of a converging (biconvex) lens and mirror. Apparatus: Biconvex glass lens, spherical concave mirror, meter ruler, optical bench, lens holder, self-illuminated object (generally a vertical arrow), screen. Background In class you have studied the physics of thin lenses and spherical mirrors. In today's lab, we will analyze several physical configurations using both biconvex lenses and concave mirrors. The components of the experiment, that is, the optics device (lens or mirror), object and image screen, will be placed on a meter stick and may be repositioned easily. The meter stick is used to determine the position of each component. For our object, we will make use of a light source with some distinguishing marking, such as an arrow or visible filament. Light from the object passes through the lens and the resulting image is focused onto a white screen. One characteristic feature of all thin lenses and concave mirrors is the focal length, f, and is defined as the image distance of an object that is positioned infinitely far way. The focal lengths of a biconvex lens and a concave mirror are shown in Figures 1 and 2, respectively. Notice the incoming light rays from the object are parallel, indicating the object is very far away. The point, C, in Figure 2 marks the center of curvature of the mirror. The distance from C to any point on the mirror is known as the radius of curvature, R. -
How Does the Light Adjustable Lens Work? What Should I Expect in The
How does the Light Adjustable Lens work? The unique feature of the Light Adjustable Lens is that the shape and focusing characteristics can be changed after implantation in the eye using an office-based UV light source called a Light Delivery Device or LDD. The Light Adjustable Lens itself has special particles (called macromers), which are distributed throughout the lens. When ultraviolet (UV) light from the LDD is directed to a specific area of the lens, the particles in the path of the light connect with other particles (forming polymers). The remaining unconnected particles then move to the exposed area. This movement causes a highly predictable change in the curvature of the lens. The new shape of the lens will match the prescription you selected during your eye exam. What should I expect in the period after cataract surgery? Please follow all instructions provided to you by your eye doctor and staff, including wearing of the UV-blocking glasses that will be provided to you. As with any cataract surgery, your vision may not be perfect after surgery. While your eye doctor selected the lens he or she anticipated would give you the best possible vision, it was only an estimate. Fortunately, you have selected the Light Adjustable Lens! In the next weeks, you and your eye doctor will work together to optimize your vision. Please make sure to pay close attention to your vision and be prepared to discuss preferences with your eye doctor. Why do I have to wear UV-blocking glasses? The UV-blocking glasses you are provided with protect the Light Adjustable Lens from UV light sources other than the LDD that your doctor will use to optimize your vision. -
Holographic Optics for Thin and Lightweight Virtual Reality
Holographic Optics for Thin and Lightweight Virtual Reality ANDREW MAIMONE, Facebook Reality Labs JUNREN WANG, Facebook Reality Labs Fig. 1. Left: Photo of full color holographic display in benchtop form factor. Center: Prototype VR display in sunglasses-like form factor with display thickness of 8.9 mm. Driving electronics and light sources are external. Right: Photo of content displayed on prototype in center image. Car scenes by komba/Shutterstock. We present a class of display designs combining holographic optics, direc- small text near the limit of human visual acuity. This use case also tional backlighting, laser illumination, and polarization-based optical folding brings VR out of the home and in to work and public spaces where to achieve thin, lightweight, and high performance near-eye displays for socially acceptable sunglasses and eyeglasses form factors prevail. virtual reality. Several design alternatives are proposed, compared, and ex- VR has made good progress in the past few years, and entirely perimentally validated as prototypes. Using only thin, flat films as optical self-contained head-worn systems are now commercially available. components, we demonstrate VR displays with thicknesses of less than 9 However, current headsets still have box-like form factors and pro- mm, fields of view of over 90◦ horizontally, and form factors approach- ing sunglasses. In a benchtop form factor, we also demonstrate a full color vide only a fraction of the resolution of the human eye. Emerging display using wavelength-multiplexed holographic lenses that uses laser optical design techniques, such as polarization-based optical folding, illumination to provide a large gamut and highly saturated color. -
Scattering Characteristics of Simplified Cylindrical Invisibility Cloaks
Scattering characteristics of simplified cylindrical invisibility cloaks Min Yan, Zhichao Ruan, Min Qiu Department of Microelectronics and Applied Physics, Royal Institute of Technology, Electrum 229, 16440 Kista, Sweden [email protected] (M.Q.) Abstract: The previously reported simplified cylindrical linear cloak is improved so that the cloak’s outer surface is impedance-matched to free space. The scattering characteristics of the improved linear cloak is compared to the previous counterpart as well as the recently proposed simplified quadratic cloak derived from quadratic coordinate transforma- tion. Significant improvement in invisibility performance is noticed for the improved linear cloak with respect to the previously proposed linear one. The improved linear cloak and the simplified quadratic cloak have comparable invisibility performances, except that the latter however has to fulfill a minimum shell thickness requirement (i.e. outer radius must be larger than twice of inner radius). When a thin cloak shell is desired, the improved linear cloak is much more superior than the other two versions of simplified cloaks. ©2007 OpticalSocietyofAmerica OCIS codes: (290.5839) Scattering, invisibility; (260.0260) Physical optics; (999.9999) Invis- ibility cloak. References and links 1. J. B. Pendry, D. Schurig, and D. R. Smith, “Controlling electromagnetic fields,” Science 312, 1780–1782 (2006). 2. U. Leonhardt, “Optical conformal mapping,” Science 312, 1777–1780 (2006). 3. A. Al`u, and N. Engheta, “Achieving transparency with plasmonic and metamaterial coatings,” Phys. Rev. E 72, 016,623 (2005). 4. Z. Ruan, M. Yan, C. W. Neff, and M. Qiu, “Ideal cylindrical cloak: Perfect but sensitive to tiny perturbations,” Phys. Rev. Lett. 99, 113,903 (2007). -
Davis Vision's Contact Lens Benefits FAQ's
Davis Vision’s Contact Lens Benefits FAQ’s for Council of Independent Colleges in Virginia Benefits Consortium, Inc. How your contact lens benefit works when you visit a Davis Vision network provider. As a Davis Vision member, you are entitled to receive contact lenses in lieu of eyeglasses during your benefit period. When you visit a Davis Vision network provider, you will first receive a comprehensive eye exam (which requires a $15 copayment) to determine the health of your eyes and the vision correction needed. If you choose to use your eyewear benefit for contacts, your eye care provider or their staff will need to further evaluate your vision care needs to prescribe the best lens options. Below is a summary of how your contact lens benefit works in the Davis Vision plan. What is the Davis Vision Contact you will have a $60 allowance after a $15 copay plus Lens Collection? 15% discount off of the balance over that amount. You will also receive a $130 allowance toward the cost of As with eyeglass frames, Davis Vision offers a special your contact lenses, plus 15% discount/1 off of the balance Collection of contact lenses to members, which over that amount. You will pay the balance remaining after greatly minimizes out-of-pocket costs. The Collection your allowance and discounts have been applied. is available only at independent network providers that also carry the Davis Vision Collection frames. Members may also choose to utilize their $130 allowance You can confirm which providers carry Davis Vision’s towards Non-Collection contacts through a provider’s own Collection by logging into the member website at supply. -
CHAPTER 1 PHYSICAL OPTICS: INTERFERENCE • Introduction
CHAPTER 1 PHYSICAL OPTICS: INTERFERENCE What is “physical optics”? • Introduction The methods of physical optics are used when the • Waves wavelength of light and dimensions of the system are of • Principle of superposition a comparable order of magnitude, when the simple ray • Wave packets approximation of geometric optics is not valid. So, it is • Phasors • Interference intermediate between geometric optics, which ignores • Reflection of waves wave effects, and full wave electromagnetism, which is a precise theory. • Young’s double-slit experiment • Interference in thin films and air gaps In General Physics II you studied some aspects of geometrical optics. Geometrical optics rests on the assumption that light propagates along straight lines and is reflected and refracted according to definite laws, such Or the use of a convex lens as a magnifying lens: as Fermat’s principle and Snell’s Law. As a result the positions of images in mirrors and through lenses, etc. can be determined by scaled drawings. For example, the s ! s production of an image in a concave mirror. s Object object y Image • F • C f f y ! image 2 s ! 1 But many optical phenomena cannot be adequately The colors you see in a soap bubble are also due to an explained by geometrical optics. For example, the interference effect between light rays reflected from the iridescence that makes the colors of a hummingbird so front and back surfaces of the thin film of soap making brilliant are not due to pigment but to an interference the bubble. The color depends on the thickness of film, effect caused by structures in the feathers. -
Lecture 37: Lenses and Mirrors
Lecture 37: Lenses and mirrors • Spherical lenses: converging, diverging • Plane mirrors • Spherical mirrors: concave, convex The animated ray diagrams were created by Dr. Alan Pringle. Terms and sign conventions for lenses and mirrors • object distance s, positive • image distance s’ , • positive if image is on side of outgoing light, i.e. same side of mirror, opposite side of lens: real image • s’ negative if image is on same side of lens/behind mirror: virtual image • focal length f positive for concave mirror and converging lens negative for convex mirror and diverging lens • object height h, positive • image height h’ positive if the image is upright negative if image is inverted • magnification m= h’/h , positive if upright, negative if inverted Lens equation 1 1 1 푠′ ℎ′ + = 푚 = − = magnification 푠 푠′ 푓 푠 ℎ 푓푠 푠′ = 푠 − 푓 Converging and diverging lenses f f F F Rays refract towards optical axis Rays refract away from optical axis thicker in the thinner in the center center • there are focal points on both sides of each lens • focal length f on both sides is the same Ray diagram for converging lens Ray 1 is parallel to the axis and refracts through F. Ray 2 passes through F’ before refracting parallel to the axis. Ray 3 passes straight through the center of the lens. F I O F’ object between f and 2f: image is real, inverted, enlarged object outside of 2f: image is real, inverted, reduced object inside of f: image is virtual, upright, enlarged Ray diagram for diverging lens Ray 1 is parallel to the axis and refracts as if from F. -
Introduction to Optics
2.71/2.710 Optics 2.71/2.710 Optics • Instructors: Prof. George Barbastathis Prof. Colin J. R. Sheppard • Assistant Instructor: Dr. Se Baek Oh • Teaching Assistant: José (Pepe) A. Domínguez-Caballero • Admin. Assistant: Kate Anderson Adiana Abdullah • Units: 3-0-9, Prerequisites: 8.02, 18.03, 2.004 • 2.71: meets the Course 2 Restricted Elective requirement • 2.710: H-Level, meets the MS requirement in Design • “gateway” subject for Doctoral Qualifying exam in Optics • MIT lectures (EST): Mo 8-9am, We 7:30-9:30am • NUS lectures (SST): Mo 9-10pm, We 8:30-10:30pm MIT 2.71/2.710 02/06/08 wk1-b- 2 Image of optical coherent tomography removed due to copyright restrictions. Please see: http://www.lightlabimaging.com/image_gallery.php Images from Wikimedia Commons, NASA, and timbobee at Flickr. MIT 2.71/2.710 02/06/08 wk1-b- 3 Natural & artificial imaging systems Image by NIH National Eye Institute. Image by Thomas Bresson at Wikimedia Commons. Image by hyperborea at Flickr. MIT 2.71/2.710 Image by James Jones at Wikimedia Commons. 02/06/08 wk1-b- 4 Image removed due to copyright restrictions. Please see http://en.wikipedia.org/wiki/File:LukeSkywalkerROTJV2Wallpaper.jpg MIT 2.71/2.710 02/06/08 wk1-b- 5 Class objectives • Cover the fundamental properties of light propagation and interaction with matter under the approximations of geometrical optics and scalar wave optics, emphasizing – physical intuition and underlying mathematical tools – systems approach to analysis and design of optical systems • Application of the physical concepts to topical -
A Sensitive Spectropolarimeter for the Measurement
A SENSITIVE SPECTROPOLARIMETER FOR THE MEASUREMENT OF CIRCULAR POLARIZATION OF LUMINESCENCE A Thesis Presented to The Faculty of the College of Engineering and Technology Ohio University In Partial Fulfillment of the Requirements for the Degree Master of Science By Ziad I. AI-Akir, June, 1990 DlHtft7~~·"E:RsaTY LI~~RY ACKNOWLEDGEMENT With gratitude and constancy, I praise the Almighty Allah for the grace and favors that He bestowed on me. Without His guidance and blessing, I would not be able to achieve any good deed in this life. I wish to extend my genuine appreciation to my advisor Dr. Henryk Lozykowski, for his teachings, assistance, encouragement and helpful suggestions. A special appreciation goes to Mr. V. K. Shastri and Mr. T. Lee for their assistance and valuable help during the preparation of this thesis. Finally, I would like to thank my brothers: Mohammed EI-Gamal, Amer AI-shawa, Abdulbaset AI-Abadleh and Rabah Odeh for their encouragement and all the brothers who helped me without knowing it. DEDICATION This thesis is dedicated to my family in Palestine and Kuwait, who have been a great source of blessing, motivation and encouragement. CONTENTS CHAPTER ONE Introduction 1 1.1 Circular Polarization of Luminescence 2 1.2 SPC in Luminescence Measurements 3 1.3 Objectives........... 5 CHAPTER TWO Literature Review......... 8 2.1 The Nature ofLight 8 2.2 Light in Matter 12 2.3 Semiconductor Materials 13 2.3.1 Intrinsic and Extrinsic Semiconductors. 15 2.3.2 Direct and Indirect Semiconductors ............... 16 2.4 Photoluminescence in Semiconductors...................... 18 2.5 Polarization 22 2.5.1 Linear Polarization 22 2.5.2 Circular Polarization 24 2.5.3 Elliptical Polarization.................................. -
Polarized Light 1
EE485 Introduction to Photonics Polarized Light 1. Matrix treatment of polarization 2. Reflection and refraction at dielectric interfaces (Fresnel equations) 3. Polarization phenomena and devices Reading: Pedrotti3, Chapter 14, Sec. 15.1-15.2, 15.4-15.6, 17.5, 23.1-23.5 Polarization of Light Polarization: Time trajectory of the end point of the electric field direction. Assume the light ray travels in +z-direction. At a particular instance, Ex ˆˆEExy y ikz() t x EEexx 0 ikz() ty EEeyy 0 iixxikz() t Ex[]ˆˆEe00xy y Ee e ikz() t E0e Lih Y. Lin 2 One Application: Creating 3-D Images Code left- and right-eye paths with orthogonal polarizations. K. Iizuka, “Welcome to the wonderful world of 3D,” OSA Optics and Photonics News, p. 41-47, Oct. 2006. Lih Y. Lin 3 Matrix Representation ― Jones Vectors Eeix E0x 0x E0 E iy 0 y Ee0 y Linearly polarized light y y 0 1 x E0 x E0 1 0 Ẽ and Ẽ must be in phase. y 0x 0y x cos E0 sin (Note: Jones vectors are normalized.) Lih Y. Lin 4 Jones Vector ― Circular Polarization Left circular polarization y x EEe it EA cos t At z = 0, compare xx0 with x it() EAsin tA ( cos( t / 2)) EEeyy 0 y 1 1 yxxy /2, 0, E00 EA Jones vector = 2 i y Right circular polarization 1 1 x Jones vector = 2 i Lih Y. Lin 5 Jones Vector ― Elliptical Polarization Special cases: Counter-clockwise rotation 1 A Jones vector = AB22 iB Clockwise rotation 1 A Jones vector = AB22 iB General case: Eeix A 0x A B22C E0 i y bei B iC Ee0 y Jones vector = 1 A A ABC222 B iC 2cosEE00xy tan 2 22 EE00xy Lih Y.