Stokes Parameters in the Unfolding of an Optical Vortex Through a Birefringent Crystal
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Polarization of Electron and Photon Beams
Revista Brasileira de Física, Vol. 11, NP 4, 1981 Polarization of Electron and Photon Beams ?. R. S. GOMES Instituto de Física, Universidade Federal Fluminense, Niterdi, RJ. Recebido eni 17 de Fevereiro de 1981 In this work the concepts of polarization of photons and re- lativistic electrons are introduced in a simplified form. Although there are important differences in the concepts of photon and electron polarization, it is shown that the saine formal ism may be used to des- cribe them, which is very useful in the study oF interactions concer- ned with polarizations of both photons and electrons, as in the yho- toelectric and Compton effects. Photons are considered, in this work, as a special case of relativistic spin 1 particles, with zero rest mass. Neste trabalho são apresentados, de uma forma simplificada, os conceitos de polarização de fotons e eletrons. Embora existam im- portantes diferenças nos conceitos de polarizaçao de fot0ns.e eletrons, mostra-se que o mesmo formalismo pode ser usado para descreve-los, o que é muito útil no estudo de interações envolvendo polarizações de ambos, fotons e eletrons, como em efeitos fotoelétrico e Compton. Nes- te trabalho os fotons são considerados como um caso especial de partí- culas relativísticas de spin 1, com massa de repouso nula. 1. INTRODUCTION Dur ing a research progi-am concerned xi th correlat ions between polarizãtions of photons and electror~sin relativistic photoelectric effect, i t was noticed the lack of a text which brings together thecon- cepts and simplified descriptions of polarization of electron and pho- ton beams . That was the reason for trying to write such a text. -
Ellipsometry
AALBORG UNIVERSITY Institute of Physics and Nanotechnology Pontoppidanstræde 103 - 9220 Aalborg Øst - Telephone 96 35 92 15 TITLE: Ellipsometry SYNOPSIS: This project concerns measurement of the re- fractive index of various materials and mea- PROJECT PERIOD: surement of the thickness of thin films on sili- September 1st - December 21st 2004 con substrates by use of ellipsometry. The el- lipsometer used in the experiments is the SE 850 photometric rotating analyzer ellipsome- ter from Sentech. THEME: After an introduction to ellipsometry and a Detection of Nanostructures problem description, the subjects of polar- ization and essential ellipsometry theory are covered. PROJECT GROUP: The index of refraction for silicon, alu- 116 minum, copper and silver are modelled us- ing the Drude-Lorentz harmonic oscillator model and afterwards measured by ellipsom- etry. The results based on the measurements GROUP MEMBERS: show a tendency towards, but are not ade- Jesper Jung quately close to, the table values. The mate- Jakob Bork rials are therefore modelled with a thin layer of oxide, and the refractive indexes are com- Tobias Holmgaard puted. This model yields good results for the Niels Anker Kortbek refractive index of silicon and copper. For aluminum the result is improved whereas the result for silver is not. SUPERVISOR: The thickness of a thin film of SiO2 on a sub- strate of silicon is measured by use of ellip- Kjeld Pedersen sometry. The result is 22.9 nm which deviates from the provided information by 6.5 %. The thickness of two thick (multiple wave- NUMBERS PRINTED: 7 lengths) thin polymer films are measured. The polymer films have been spin coated on REPORT PAGE NUMBER: 70 substrates of silicon and the uniformities of the surfaces are investigated. -
Huygen's Explanation of Double Refraction
06/08/2018 Before this lecture there were two lectures: 1. Introduction about this course. 2. Qualitative description about the various polarizations. Retarders • In retarders, one polarization gets ‘retarded’, or delayed, with respect to the other one. There is a final phase difference between the 2 components of the polarization. Therefore, the polarization is changed. • Most retarders are based on birefringent materials (quartz, mica, polymers) that have different indices of refraction depending on the polarization of the incoming light. 3 Phase shift of half wavelength Quarter Wave plate Circular polarization (IV) 7 How to generate Polarized Light? 1.Dichroic materials 2.Polarizer 3.Birefringent materials 4.Reflection 5.Scattering Wire grid polarizer Polaroid How to generate Polarized Light? 1.Dichroic materials 2.Polarizer 3.Birefringent materials 4.Reflection 5.Scattering Birefringence How to generate Polarized Light? 1.Dichroic materials 2.Polarizer 3.Birefringent materials 4.Reflection 5.Scattering Polarized Reflecting Light • When an unpolarized light wave reflects off a non-metallic surface, it can be completely polarized, partially polarized or unpolarized depending on the angle of incidence. A completely polarized wave occurs for an angle called Brewster’s angle (named after Sir David Brewster) Snell's law Incident Reflected ray ray p n 90o 1 n2 r n1sin P = n2sin r n1sin P = n2sin r = n2sin (90-P) = n2cos P tan P = n2/n1 P = Brewster’s angel Reflection • When an unpolarized wave reflects off a nonmetallic surface, the reflected wave is partially plane polarized parallel to the surface. The amount of polarization depends upon the angle (more later). The reflected ray contains more vibrations parallel to the reflecting surface while the transmitted beam contains more vibrations at right angles to these. -
Results from the QUIET Q-Band Observing Season COLUMBIA
Results from the QUIET Q-Band Observing Season Robert Nicolas Dumoulin Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Science COLUMBIA UNIVERSITY 2011 ©2011 Robert Nicolas Dumoulin All Rights Reserved Abstract Results from the QUIET Q-Band Observing Season Robert Nicolas Dumoulin The Q/U Imaging ExperimenT (QUIET) is a ground-based telescope located in the high Atacama Desert in Chile, and is designed to measure the polarization of the Cosmic Mi- crowave Background (CMB) in the Q and W frequency bands (43 and 95 GHz respec- tively) using coherent polarimeters. From 2008 October to 2010 December, data from more than 10,000 observing hours were collected, first with the Q-band receiver (2008 October to 2009 June) and then with the W-band receiver (until the end of the 2010 ob- serving season). The QUIET data analysis effort uses two independent pipelines, one consisting of a max- imum likelihood framework and the other consisting of a pseudo-C` framework. Both pipelines employ blind analysis methods, and each provides analysis of the data using large suites of null tests specific to the pipeline. Analysis of the Q-band receiver data was completed in November of 2010, confirming the only previous detection of the first acoustic peak of the EE power spectrum and setting competitive limits on the scalar-to- tensor ratio, r. In this dissertation, the results from the Q-band observing season using the maximum likelihood pipeline will be presented. Contents 1 The Cosmic Microwave Background 1 1.1 The Origins and Features of the CMB . -
How to Generate Polarized Light?
Before this lecture there were two lectures: 1. Qualitative description of polarization and generation of various polarized light. 2. Quantitative derivation and explaining the observations. 08/08/2017 How to generate Polarized Light? 1.Dichroic materials 2.Polarizer 3.Birefringent materials 4.Reflection 5.Scattering Wire grid polarizer Birefringence Polarized Reflecting Light • When an unpolarized light wave reflects off a non-metallic surface, it can be completely polarized, partially polarized or unpolarized depending on the angle of incidence. A completely polarized wave occurs for an angle called Brewster’s angle (named after Sir David Brewster) Snell's law Incident Reflected ray ray p n 90o 1 n2 r n1sin P = n2sin r n1sin P = n2sin r = n2sin (90-P) = n2cos P tan P = n2/n1 P = Brewster’s angel Reflection • When an unpolarized wave reflects off a nonmetallic surface, the reflected wave is partially plane polarized parallel to the surface. The amount of polarization depends upon the angle (more later). The reflected ray contains more vibrations parallel to the reflecting surface while the transmitted beam contains more vibrations at right angles to these. Applications • Knowing that reflected light or glare from surfaces is at least partially plane polarized, one can use Polaroid sunglasses. The polarization axes of the lenses are vertical as the glare usually comes from reflection off horizontal surfaces. Polarized Lens on a Camera Reduce Reflections Polarization by Scattering • When a light wave passes through a gas, it will be absorbed and then re-radiated in a variety of directions. This process is called scattering. y Gas molecule z O Unpolarized x sunlight Light scattered at right angles is plane-polarized Polarization by Scatterings Retarders • In retarders, one polarization gets ‘retarded’, or delayed, with respect to the other one. -
Arxiv:1309.5454V1 [Astro-Ph.SR] 21 Sep 2013 E-Mail: Stenfl[email protected] 2 J.O
The Astronomy and Astrophysics Review manuscript No. (will be inserted by the editor) Solar magnetic fields as revealed by Stokes polarimetry J.O. Stenflo Received: 10 July 2013 / Accepted: 4 September 2013 Abstract Observational astrophysics started when spectroscopy could be applied to astronomy. Similarly, observational work on stellar magnetic fields became possible with the application of spectro-polarimetry. In recent decades there have been dramatic advances in the observational tools for spectro- polarimetry. The four Stokes parameters that provide a complete represen- tation of partially polarized light can now be simultaneously imaged with megapixel array detectors with high polarimetric precision (10−5 in the degree of polarization). This has led to new insights about the nature and properties of the magnetic field, and has helped pave the way for the use of the Hanle effect as a diagnostic tool beside the Zeeman effect. The magnetic structuring continues on scales orders of magnitudes smaller than the resolved ones, but various types of spectro-polarimetric signatures can be identified, which let us determine the field strengths and angular distributions of the field vectors in the spatially unresolved domain. Here we review the observational properties of the magnetic field, from the global patterns to the smallest scales at the magnetic diffusion limit, and relate them to the global and local dynamos. Keywords Sun: atmosphere · magnetic fields · polarization · dynamo · magnetohydrodynamics (MHD) 1 Historical background The discovery and classification by Joseph Fraunhofer of the absorption lines in the Sun's spectrum and the demonstration by Bunsen and Kirchhoff that such lines represent “fingerprints" of chemical elements marked the birth of modern astrophysics. -
Polarisation
Polarisation In plane polarised light, the plane containing the direction of POLARISATION vibration and propagation of light is called plane of vibration. Polarisation Plane which is perpendicular to the plane of vibration is called plane of polarisation. The phenomenon due to which vibrations of light waves are restricted in a particular plane is called polarisation. In an ordinary beam of light from a source, the vibrations occur normal to the direction of propagation in all possible planes. Such beam of light called unpolarised light. If by some methods (reflection, refraction or scattering) a beam of light is produced in which vibrations are confined to only one plane, then it is called as plane polarised light. Hence, polarisation is the phenomenon of producing plane polarised light from unpolarised light. In above diagram plane ABCD represents the plane of vibration and EFGH represents the plane of polarisation. There are three type of polarized light 1) Plane Polarized Light 2) Circularly Polarized Light 3) Elliptically Polarized Light Page 1 of 12 Prof. A. P. Manage DMSM’s Bhaurao Kakatkar College, Belgaum Polarisation Huygen’s theory of double refraction According to Huygen’s theory, a point in a doubly refracting or birefringent crystal produces 2 types of wavefronts. The wavefront corresponding to the O-ray is spherical wavefront. The ordinary wave travels with same velocity in all directions and so the corresponding wavefront is spherical. The wavefront corresponding to the E-ray is ellipsoidal wavefront. Extraordinary waves have different velocities in Polarised light can be produced by either reflection, different directions, so the corresponding wavefront is elliptical. -
Quantum State Tomography of Single Qubit Using Density Matrix
PROC. INTERNAT. CONF. SCI. ENGIN. ISSN 1504607797 Volume 4, February 2021 E-ISSN 1505707533 Page 27-32 Quantum State Tomography of Single Qubit Using Density Matrix Syafi’i Fahmi Bastian1, Pruet Kalasuwan2, Joko Purwanto1 1Physics Education Department, Faculty of Science and Technology, Universitas Islam Negeri Sunan Kalijaga 2Department of Physics, Faculty of Science, Prince of Songkla University, Hat Yai, Thailand Email: [email protected] Abstract. The quantum state tomography is a fundamental part in the development of quantum technologies. It can be used to know the signal characterization of small particle called photon in the nanoscale. In this study, photon number has been measured in order to produce the states tomography. Optical devices and quantum-mechanical approaches were explored to obtain the quantum state tomography. Due to a single qubit state density matrix can be revealed by Stokes parameters, so there are four set-ups to measure the Stokes parameters for each sample. The density matrix is used because the pure state only appear theoreticaly. In the real experiment, It always exibits a mixed state. The samples of tomography measurements consist of linear state, cicular state and the IR 808nm. In this study, state tomography is shown by 2x2 density matrix. This experiment also provides the fidelities of experiment result. And it shows the good agreement. From this experiment, the state of IR 808nm has been detected. The laser that examined is showing a vertical state with fidelity F=97,34%. Keywords: a single qubit, density matrix, quantum state INTRODUCTION |퐻⟩ is acting for horizontal state and |푉⟩ is acting for Quantum physics is capable to reveal the behavior of vertical state. -
Maxwell's Equations, Electromagnetic Waves, and Stokes Parameters B
MAXWELL’S EQUATIONS, ELECTROMAGNETIC WAVES, AND STOKES PARAMETERS MICHAEL I. MISHCHENKO AND LARRY D. TRAVIS NASA Goddard Institute for Space Studies, 2880 Broadway, New York, NY 10025, USA 1. Introduction The theoretical basis for describing elastic scattering of light by particles and surfaces is formed by classical electromagnetics. In order to make this volume sufficiently self-contained, this introductory chapter provides a summary of those concepts and equations of electromagnetic theory that will be used extensively in later chapters and introduces the necessary notation. We start by formulating the macroscopic Maxwell equations and constitutive relations and discussing the fundamental time-harmonic plane- wave solution that underlies the basic optical idea of a monochromatic parallel beam of light. This is followed by the introduction of the Stokes parameters and a discussion of their ellipsometric content. Then we consider the concept of a quasi-monochromatic beam of light and its implications and briefly discuss how the Stokes parameters of monochromatic and quasi- monochromatic light can be measured in practice. In the final two sections, we discuss another fundamental solution of Maxwell’s equations in the form of a time-harmonic outgoing spherical wave and introduce the concept of the coherency dyad, which plays a vital role in the theory of multiple light scattering by random particle ensembles. 2. Maxwell’s equations and constitutive relations The theory of classical optics phenomena is based on the set of four Maxwell’s equations for the macroscopic electromagnetic field at interior points in matter, which in SI units read: ∇ ⋅D(r, t) = ρ(r, t), (2.1) ∂B(r, t) ∇ ×E(r, t) = − , (2.2) ∂t ∇ ⋅B(r, t) = 0, (2.3) 1 G. -
Conical Diffraction: Complexifying Hamilton's Diabolical Legacy Mike
Conical Diffraction: Complexifying Hamilton’s Diabolical Legacy Mike R. Jeffrey A thesis submitted to the University of Bristol in accordance with the requirements of the degree of Ph.D. in the Faculty of Science H. H. Wills Physics Laboratory September 2007 word count 32,795 Abstract The propagation of light along singular directions in anisotropic media teems with rich asymptotic phenomena that are poorly understood. We study the refraction and diffraction of light beams through crystals exhibiting biaxial birefringence, optical activity, and dichroism. The optical properties and length of the crystal are related to the beam’s width, wavenumber, and alignment, by just three parameters defined by the effect of the crystal on a paraxial plane wave. Singular axes are crystal directions in which the refractive indices are degenerate. In transparent biaxial crystals they are a pair of optic axes corresponding to conical intersections of the propagating wave surface. This gives rise to the well understood phenomenon of conical diffraction. Our interest here is in dichroic and optically active crystals. Dichroism splits each optic axis into pairs or rings of singular axes, branch points of the complex wave surface. Optical activity destroys the optic axis degeneracy but creates a ring of wave surface inflection points. We study the unknown effect of these degeneracy structures on the diffracted light field, predicting striking focusing and interference phenomena. Focusing is understood by the coalescence of real geometric rays, while geometric interference is included by endowing rays with phase to constitute complex rays. Optical activity creates a rotationally symmetric cusped caustic surface threaded by an axial focal line, which should be easy to observe experimentally. -
Arxiv:1401.1911V1 [Astro-Ph.IM] 9 Jan 2014 Rpitpeae Yteauthor the by Prepared Preprint .PLRGNSS
Journal of The Korean Astronomical Society (Preprint - no DOI assigned) 00: 1 25, 2013 December ISSN:1225-4614 Preprint∼ prepared by the author http://jkas.kas.org POLARIZATION AND POLARIMETRY: A REVIEW Sascha Trippe Department of Physics and Astronomy, Seoul National University, Seoul 151-742, South Korea E-mail: [email protected] (Received 30 August 2013; Revised 17 December 2013; Accepted 28 December 2013) ABSTRACT Polarization is a basic property of light and is fundamentally linked to the internal geometry of a source of radiation. Polarimetry complements photometric, spectroscopic, and imaging analyses of sources of radiation and has made possible multiple astrophysical discoveries. In this article I review (i) the phys- ical basics of polarization: electromagnetic waves, photons, and parameterizations; (ii) astrophysical sources of polarization: scattering, synchrotron radiation, active media, and the Zeeman, Goldreich- Kylafis, and Hanle effects, as well as interactions between polarization and matter (like birefringence, Faraday rotation, or the Chandrasekhar-Fermi effect); (iii) observational methodology: on-sky geom- etry, influence of atmosphere and instrumental polarization, polarization statistics, and observational techniques for radio, optical, and X/γ wavelengths; and (iv) science cases for astronomical polarime- try: solar and stellar physics, planetary system bodies, interstellar matter, astrobiology, astronomical masers, pulsars, galactic magnetic fields, gamma-ray bursts, active galactic nuclei, and cosmic microwave background radiation. Key words : Polarization — Methods: polarimetric — Radiation mechanisms: general Contents 3.8.4. Faraday Depolarization . 12 3.8.5. Polarization Conversion . 13 1. INTRODUCTION ................. 2 3.8.6. Chandrasekhar-Fermi Effect . 13 2. PHYSICALBASICS ................ 2 4. OBSERVATIONS ................. 13 2.1. Electromagnetic Waves . 2 4.1. -
Advanced Polarimetric Synthetic Aperture Radar (Sar) and Electro-Optical (Eo) Data Fusion Through Unified Coherent Formulation of the Scattered Em Field
Progress In Electromagnetics Research, PIER 84, 189–203, 2008 ADVANCED POLARIMETRIC SYNTHETIC APERTURE RADAR (SAR) AND ELECTRO-OPTICAL (EO) DATA FUSION THROUGH UNIFIED COHERENT FORMULATION OF THE SCATTERED EM FIELD R. Sabry and P. W. Vachon Radar Application & Space Technology Defence R&D Canada — Ottawa 3701 Carling Avenue, Ottawa, Ontario, K1A 0Z4, Canada Abstract—Exploitation of the backscattered field polarization over the wide electromagnetic spectrum, from visible to microwave frequencies, provides an approach to advanced target recognition in remote sensing applications. The framework for full coherent characterization of the scattered field that is established here, maximizes the extracted target information. It is also shown that such a methodology, which is theoretically similar to the concept of “partial or compact polarimetry”, yields comparable results to full or quadrature-polarized systems by incorporating judicious assumptions and assuming/implementing optimal transmitted or illumination field polarizations. On this basis, common characteristic features, interworking and fusion of different polarimetric sensor products in different regions of spectrum, e.g., radar/SAR and Electro-Optical, are investigated and formulated within a robust framework based on full coherent treatment of the scattered field. 1. INTRODUCTION Exploiting polarization characteristics of the backscattered electromag- netic (EM) waveform provides significant insight into the nature of targets, and additional information for target recognition compared to conventional remote sensing sources. This is supported by the well- established physics of EM fields and waves [1–5]. In short, EM po- larimetry, from microwave to visible frequencies, provides an enhanced capability for advanced target recognition in remote sensing applica- tions. 190 Sabry and Vachon The objective here is to explore the interworking and fusion of EM polarimetric observables and measurables associated with certain classes of targets in different regions of the EM spectrum.