PHYS20312 Wave Optics -‐ Section 2: Polarization
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Polarization Optics Polarized Light Propagation Partially Polarized Light
The physics of polarization optics Polarized light propagation Partially polarized light Polarization Optics N. Fressengeas Laboratoire Mat´eriaux Optiques, Photonique et Syst`emes Unit´ede Recherche commune `al’Universit´ede Lorraine et `aSup´elec Download this document from http://arche.univ-lorraine.fr/ N. Fressengeas Polarization Optics, version 2.0, frame 1 The physics of polarization optics Polarized light propagation Partially polarized light Further reading [Hua94, GB94] A. Gerrard and J.M. Burch. Introduction to matrix methods in optics. Dover, 1994. S. Huard. Polarisation de la lumi`ere. Masson, 1994. N. Fressengeas Polarization Optics, version 2.0, frame 2 The physics of polarization optics Polarized light propagation Partially polarized light Course Outline 1 The physics of polarization optics Polarization states Jones Calculus Stokes parameters and the Poincare Sphere 2 Polarized light propagation Jones Matrices Examples Matrix, basis & eigen polarizations Jones Matrices Composition 3 Partially polarized light Formalisms used Propagation through optical devices N. Fressengeas Polarization Optics, version 2.0, frame 3 The physics of polarization optics Polarization states Polarized light propagation Jones Calculus Partially polarized light Stokes parameters and the Poincare Sphere The vector nature of light Optical wave can be polarized, sound waves cannot The scalar monochromatic plane wave The electric field reads: A cos (ωt kz ϕ) − − A vector monochromatic plane wave Electric field is orthogonal to wave and Poynting vectors -
Lab 8: Polarization of Light
Lab 8: Polarization of Light 1 Introduction Refer to Appendix D for photos of the appara- tus Polarization is a fundamental property of light and a very important concept of physical optics. Not all sources of light are polarized; for instance, light from an ordinary light bulb is not polarized. In addition to unpolarized light, there is partially polarized light and totally polarized light. Light from a rainbow, reflected sunlight, and coherent laser light are examples of po- larized light. There are three di®erent types of po- larization states: linear, circular and elliptical. Each of these commonly encountered states is characterized Figure 1: (a)Oscillation of E vector, (b)An electromagnetic by a di®ering motion of the electric ¯eld vector with ¯eld. respect to the direction of propagation of the light wave. It is useful to be able to di®erentiate between 2 Background the di®erent types of polarization. Some common de- vices for measuring polarization are linear polarizers and retarders. Polaroid sunglasses are examples of po- Light is a transverse electromagnetic wave. Its prop- larizers. They block certain radiations such as glare agation can therefore be explained by recalling the from reflected sunlight. Polarizers are useful in ob- properties of transverse waves. Picture a transverse taining and analyzing linear polarization. Retarders wave as traced by a point that oscillates sinusoidally (also called wave plates) can alter the type of polar- in a plane, such that the direction of oscillation is ization and/or rotate its direction. They are used in perpendicular to the direction of propagation of the controlling and analyzing polarization states. -
Static and Dynamic Effects of Chirality in Dielectric Media
Static and dynamic effects of chirality in dielectric media R. S. Lakes Department of Engineering Physics, Department of Materials Science, University of Wisconsin, 1500 Engineering Drive, Madison, WI 53706-1687 [email protected] January 31, 2017 adapted from R. S. Lakes, Modern Physics Letters B, 30 (24) 1650319 (9 pages) (2016). Abstract Chiral dielectrics are considered from the perspective of continuum representations of spatial heterogeneity. Static effects in isotropic chiral dielectrics are predicted, provided the electric field has nonzero third spatial derivatives. The effects are compared with static chiral phenomena in Cosserat elastic materials which obey generalized continuum constitutive equations. Dynamic monopole - like magnetic induction is predicted in chiral dielectric media. keywords: chirality, dielectric, Cosserat 1 Introduction Chirality is well known in electromagnetics 1; it gives rise to optical activity in which left or right handed cir- cularly polarized waves propagate at different velocities. Known effects are dynamic only; there is considered to be no static effect 2. The constitutive equations for a directionally isotropic chiral material are 3, 4. @H D = kE − g (1) @t @E B = µH + g (2) @t in which E is electric field, D is electric displacement, B is magnetic field, H is magnetic induction, k is the dielectric permittivity, µ is magnetic permeability and g is a measure of the chirality. Optical rotation of polarized light of wavelength λ by an angle Φ (in radians per meter) is given by Φ = (2π/λ)2cg with c as the speed of light. The quantity g embodies the length scale of the chiral structure because cg has dimensions of length. -
Principles of Retarders
Polarizers PRINCIPLES OF RETARDERS etarders are used in applications where control or Ranalysis of polarization states is required. Our retarder products include innovative polymer and liquid crystal materials. Crystalline materials such as quartz and Retarders magnesium fluoride are also available upon request. Please call for a custom quote. A retarder (or waveplate) is an optical device that resolves a light wave into two orthogonal linear polarization components and produces a phase shift between them. The resulting light wave is generally of a different polarization form. Ideally, retarders do not polarize, nor do they induce an intensity change in the Crystals Liquid light beam, they simply change its polarization form. state. The transmitted light leaves the retarder elliptically All standard catalog Meadowlark Optics’ retarders are polarized. made from birefringent, uniaxial materials having two Retardance (in waves) is given by: different refractive indices – the extraordinary index ne = tր and the ordinary index no. Light traveling through a retarder has a velocity v where: dependent upon its polarization direction given by  = birefringence (ne - no) Spatial Light Modulators v = c/n = wavelength of incident light (in nanometers) t = thickness of birefringent element where c is the speed of light in a vacuum and n is the (in nanometers) refractive index parallel to that polarization direction. Retardance can also be expressed in units of length, the By definition, ne > no for a positive uniaxial material. distance that one polarization component is delayed For a positive uniaxial material, the extraordinary axis relative to the other. Retardance is then represented by: is referred to as the slow axis, while the ordinary axis is ␦Ј ␦  referred to as the fast axis. -
Polarization of EM Waves
Light in different media A short review • Reflection of light: Angle of incidence = Angle of reflection • Refraction of light: Snell’s law Refraction of light • Total internal reflection For some critical angle light beam will be reflected: 1 n2 c sin n1 For some critical angle light beam will be reflected: Optical fibers Optical elements Mirrors i = p flat concave convex 1 1 1 p i f Summary • Real image can be projected on a screen • Virtual image exists only for observer • Plane mirror is a flat reflecting surface Plane Mirror: ip • Convex mirrors make objects smaller • Concave mirrors make objects larger 1 Spherical Mirror: fr 2 Geometrical Optics • “Geometrical” optics (rough approximation): light rays (“particles”) that travel in straight lines. • “Physical” Classical optics (good approximation): electromagnetic waves which have amplitude and phase that can change. • Quantum Optics (exact): Light is BOTH a particle (photon) and a wave: wave-particle duality. Refraction For y = 0 the same for all x, t Refraction Polarization Polarization By Reflection Different polarization of light get reflected and refracted with different amplitudes (“birefringence”). At one particular angle, the parallel polarization is NOT reflected at all! o This is the “Brewster angle” B, and B + r = 90 . (Absorption) o n1 sin n2 sin(90 ) n2 cos n2 tan Polarizing Sunglasses n1 Polarized Sunglasses B Linear polarization Ey Asin(2x / t) Vertically (y axis) polarized wave having an amplitude A, a wavelength of and an angular velocity (frequency * 2) of , propagating along the x axis. Linear polarization Vertical Ey Asin(2x / t) Horizontal Ez Asin(2x / t) Linear polarization • superposition of two waves that have the same amplitude and wavelength, • are polarized in two perpendicular planes and oscillate in the same phase. -
Polarization (Waves)
Polarization (waves) Polarization (also polarisation) is a property applying to transverse waves that specifies the geometrical orientation of the oscillations.[1][2][3][4][5] In a transverse wave, the direction of the oscillation is perpendicular to the direction of motion of the wave.[4] A simple example of a polarized transverse wave is vibrations traveling along a taut string (see image); for example, in a musical instrument like a guitar string. Depending on how the string is plucked, the vibrations can be in a vertical direction, horizontal direction, or at any angle perpendicular to the string. In contrast, in longitudinal waves, such as sound waves in a liquid or gas, the displacement of the particles in the oscillation is always in the direction of propagation, so these waves do not exhibit polarization. Transverse waves that exhibit polarization include electromagnetic [6] waves such as light and radio waves, gravitational waves, and transverse Circular polarization on rubber sound waves (shear waves) in solids. thread, converted to linear polarization An electromagnetic wave such as light consists of a coupled oscillating electric field and magnetic field which are always perpendicular; by convention, the "polarization" of electromagnetic waves refers to the direction of the electric field. In linear polarization, the fields oscillate in a single direction. In circular or elliptical polarization, the fields rotate at a constant rate in a plane as the wave travels. The rotation can have two possible directions; if the fields rotate in a right hand sense with respect to the direction of wave travel, it is called right circular polarization, while if the fields rotate in a left hand sense, it is called left circular polarization. -
Lecture 14: Polarization
Matthew Schwartz Lecture 14: Polarization 1 Polarization vectors In the last lecture, we showed that Maxwell’s equations admit plane wave solutions ~ · − ~ · − E~ = E~ ei k x~ ωt , B~ = B~ ei k x~ ωt (1) 0 0 ~ ~ Here, E0 and B0 are called the polarization vectors for the electric and magnetic fields. These are complex 3 dimensional vectors. The wavevector ~k and angular frequency ω are real and in the vacuum are related by ω = c ~k . This relation implies that electromagnetic waves are disper- sionless with velocity c: the speed of light. In materials, like a prism, light can have dispersion. We will come to this later. In addition, we found that for plane waves 1 B~ = ~k × E~ (2) 0 ω 0 This equation implies that the magnetic field in a plane wave is completely determined by the electric field. In particular, it implies that their magnitudes are related by ~ ~ E0 = c B0 (3) and that ~ ~ ~ ~ ~ ~ k · E0 =0, k · B0 =0, E0 · B0 =0 (4) In other words, the polarization vector of the electric field, the polarization vector of the mag- netic field, and the direction ~k that the plane wave is propagating are all orthogonal. To see how much freedom there is left in the plane wave, it’s helpful to choose coordinates. We can always define the zˆ direction as where ~k points. When we put a hat on a vector, it means the unit vector pointing in that direction, that is zˆ=(0, 0, 1). Thus the electric field has the form iω z −t E~ E~ e c = 0 (5) ~ ~ which moves in the z direction at the speed of light. -
Circular Polarization and Nonreciprocal Propagation in Magnetic Media Circular Polarization and Nonreciprocal Propagation in Magnetic Media Gerald F
• DIONNE, ALLEN, Haddad, ROSS, AND LaX Circular Polarization and Nonreciprocal Propagation in Magnetic Media Circular Polarization and Nonreciprocal Propagation in Magnetic Media Gerald F. Dionne, Gary A. Allen, Pamela R. Haddad, Caroline A. Ross, and Benjamin Lax n The polarization of electromagnetic signals is an important feature in the design of modern radar and telecommunications. Standard electromagnetic theory readily shows that a linearly polarized plane wave propagating in free space consists of two equal but counter-rotating components of circular polarization. In magnetized media, these circular modes can be arranged to produce the nonreciprocal propagation effects that are the basic properties of isolator and circulator devices. Independent phase control of right-hand (+) and left-hand (–) circular waves is accomplished by splitting their propagation velocities through differences in the e±m± parameter. A phenomenological analysis of the permeability m and permittivity e in dispersive media serves to introduce the corresponding magnetic- and electric-dipole mechanisms of interaction length with the propagating signal. As an example of permeability dispersion, a Lincoln Laboratory quasi-optical Faraday- rotation isolator circulator at 35 GHz (l ~ 1 cm) with a garnet-ferrite rotator element is described. At infrared wavelengths (l = 1.55 mm), where fiber-optic laser sources also require protection by passive isolation of the Faraday-rotation principle, e rather than m provides the dispersion, and the frequency is limited to the quantum energies of the electric-dipole atomic transitions peculiar to the molecular structure of the magnetic garnet. For optimum performance, bismuth additions to the garnet chemical formula are usually necessary. Spectroscopic and molecular theory models developed at Lincoln Laboratory to explain the bismuth effects are reviewed. -
Polarization of Light Demonstration This Demonstration Explains Transverse Waves and Some Surprising Properties of Polarizers
Polarization of Light Demonstration This demonstration explains transverse waves and some surprising properties of polarizers. Number of Participants: Unlimited Audience: Middle (ages 11-13) and up Duration: 5-10 min Microbehunter Difficulty: Level 1 Materials Required: • 3 sheets of polarizing film – at least (20mm)2 • Long spring or Slinky Setup: 1. If necessary, prepare polarizing sheets by cutting a larger sheet into smaller pieces. While larger pieces of polarizing material are preferred, the demonstration works with smaller pieces. Presenter Brief: Light is a transverse wave because its two components, electric and magnetic fields, oscillate perpendicular to the direction of propagation. In general, a beam of light will consist of many photons traveling in the same direction but with arbitrary alignment of their electric and magnetic fields. Specifically, for an unpolarized light beam the electromagnetic components of each photon, while confined to a plane, are not aligned. If light is polarized, photons have aligned electromagnetic components and travel in the same direction. Polarization of Light Vocabulary: • Light – Electromagnetic radiation, which can be in the visible range. • Electromagnetic – A transverse wave consisting of oscillating electric and magnetic components. • Transverse wave – A wave consisting of oscillations perpendicular to the direction of propagation. • Polarized light – A beam of photons propagating with aligned oscillating components.Polarizer – A material which filters homogenous light along a singular axis and thus blocks arbitrary orientations and allows a specific orientation of oscillations. Physics & Explanation: Middle (ages 11-13) and general public: Light, or an electromagnetic wave, is a transverse wave with oscillating electric and magnetic components. Recall that in a transverse wave, the vibrations,” or oscillations, are perpendicular to the direction of propagation. -
Glossary of Terms Used in Photochemistry, 3Rd Edition (IUPAC
Pure Appl. Chem., Vol. 79, No. 3, pp. 293–465, 2007. doi:10.1351/pac200779030293 © 2007 IUPAC INTERNATIONAL UNION OF PURE AND APPLIED CHEMISTRY ORGANIC AND BIOMOLECULAR CHEMISTRY DIVISION* SUBCOMMITTEE ON PHOTOCHEMISTRY GLOSSARY OF TERMS USED IN PHOTOCHEMISTRY 3rd EDITION (IUPAC Recommendations 2006) Prepared for publication by S. E. BRASLAVSKY‡ Max-Planck-Institut für Bioanorganische Chemie, Postfach 10 13 65, 45413 Mülheim an der Ruhr, Germany *Membership of the Organic and Biomolecular Chemistry Division Committee during the preparation of this re- port (2003–2006) was as follows: President: T. T. Tidwell (1998–2003), M. Isobe (2002–2005); Vice President: D. StC. Black (1996–2003), V. T. Ivanov (1996–2005); Secretary: G. M. Blackburn (2002–2005); Past President: T. Norin (1996–2003), T. T. Tidwell (1998–2005) (initial date indicates first time elected as Division member). The list of the other Division members can be found in <http://www.iupac.org/divisions/III/members.html>. Membership of the Subcommittee on Photochemistry (2003–2005) was as follows: S. E. Braslavsky (Germany, Chairperson), A. U. Acuña (Spain), T. D. Z. Atvars (Brazil), C. Bohne (Canada), R. Bonneau (France), A. M. Braun (Germany), A. Chibisov (Russia), K. Ghiggino (Australia), A. Kutateladze (USA), H. Lemmetyinen (Finland), M. Litter (Argentina), H. Miyasaka (Japan), M. Olivucci (Italy), D. Phillips (UK), R. O. Rahn (USA), E. San Román (Argentina), N. Serpone (Canada), M. Terazima (Japan). Contributors to the 3rd edition were: A. U. Acuña, W. Adam, F. Amat, D. Armesto, T. D. Z. Atvars, A. Bard, E. Bill, L. O. Björn, C. Bohne, J. Bolton, R. Bonneau, H. -
Chapter 9 Refraction and Polarization of Light
Chapter 9 Refraction and Polarization of Light Name: Lab Partner: Section: 9.1 Purpose The purpose of this experiment is to demonstrate several consequences of the fact that materials have di↵erent indexes of refraction for light. Refraction, total internal reflection and the polarization of light reflecting from a nonmetallic surface will be investigated 9.2 Introduction Light can travel through many transparent media such as water, glass and air. When this happens the speed of light is no longer c =3 108 m/s (the speed in vacuum), but is less. This reduction in the speed depends on the material.⇥ This change in speed and direction is called refraction and is governed by Snell’s Law of Refraction. n1sin✓1 = n2sin✓2 (9.1) The ratio of the speed of light in vacuum to that in the medium is called the index of refraction (n). The index of refraction is a number greater than or equal to one. The angles (✓1 and ✓2)aremeasuredwithrespecttothenormal(perpendicular)totheinterfacebetween the two media (See Figure 9.1). When light passes from a medium of higher index of refraction to a medium with a lower index of refraction, the light ray can be refracted at 900.Thisphenomenoniscalledtotal internal reflection.Forincidentanglesgreaterthan✓c,thereisnorefractedbeam.The transmission of light by fiber-optic cable uses this e↵ect. The critical angle of incidence where total internal reflection occurs is given by: n2 sin✓c = n1 >n2 (9.2) n1 If this angle and the index of refraction of one of the two media is known, the index of refraction of the other medium can be found. -
Understanding Polarization
Semrock Technical Note Series: Understanding Polarization The Standard in Optical Filters for Biotech & Analytical Instrumentation Understanding Polarization 1. Introduction Polarization is a fundamental property of light. While many optical applications are based on systems that are “blind” to polarization, a very large number are not. Some applications rely directly on polarization as a key measurement variable, such as those based on how much an object depolarizes or rotates a polarized probe beam. For other applications, variations due to polarization are a source of noise, and thus throughout the system light must maintain a fixed state of polarization – or remain completely depolarized – to eliminate these variations. And for applications based on interference of non-parallel light beams, polarization greatly impacts contrast. As a result, for a large number of applications control of polarization is just as critical as control of ray propagation, diffraction, or the spectrum of the light. Yet despite its importance, polarization is often considered a more esoteric property of light that is not so well understood. In this article our aim is to answer some basic questions about the polarization of light, including: what polarization is and how it is described, how it is controlled by optical components, and when it matters in optical systems. 2. A description of the polarization of light To understand the polarization of light, we must first recognize that light can be described as a classical wave. The most basic parameters that describe any wave are the amplitude and the wavelength. For example, the amplitude of a wave represents the longitudinal displacement of air molecules for a sound wave traveling through the air, or the transverse displacement of a string or water molecules for a wave on a guitar string or on the surface of a pond, respectively.