INTRODUCTION. Definition:-

Similar documents
Lecture # 04 January 27, 2010, Wednesday Energy & Radiation

The Scattering of Light by Small Particles. Advanced Laboratory, Physics 407 University of Wisconsin Madison, Wisconsin 53706

Nanoacoustics II Lecture #4 Brillouin scattering

1. The most important aspects of the quantum theory.

Skoog Chapter 6 Introduction to Spectrometric Methods

Absorption and scattering

Vibrational Spectroscopies. C-874 University of Delaware

ECE280: Nano-Plasmonics and Its Applications. Week8

24/ Rayleigh and Raman scattering. Stokes and anti-stokes lines. Rotational Raman spectroscopy. Polarizability ellipsoid. Selection rules.

IR Spectrography - Absorption. Raman Spectrography - Scattering. n 0 n M - Raman n 0 - Rayleigh

Nonlinear Effects in Optical Fiber. Dr. Mohammad Faisal Assistant Professor Dept. of EEE, BUET

Temperature ( o C)

Chemistry Instrumental Analysis Lecture 2. Chem 4631

Model Answer (Paper code: AR-7112) M. Sc. (Physics) IV Semester Paper I: Laser Physics and Spectroscopy

CHEM*3440. Photon Energy Units. Spectrum of Electromagnetic Radiation. Chemical Instrumentation. Spectroscopic Experimental Concept.

Application of IR Raman Spectroscopy

Laser trapping of non-spherical particles

The Electromagnetic Properties of Materials

Molecular spectroscopy

ElectroMagnetic Radiation (EMR) Lecture 2-3 August 29 and 31, 2005

What happens when light falls on a material? Transmission Reflection Absorption Luminescence. Elastic Scattering Inelastic Scattering

HYPER-RAYLEIGH SCATTERING AND SURFACE-ENHANCED RAMAN SCATTERING STUDIES OF PLATINUM NANOPARTICLE SUSPENSIONS

Nanophotonics: principle and application. Khai Q. Le Lecture 4 Light scattering by small particles

Laser Beam Interactions with Solids In absorbing materials photons deposit energy hc λ. h λ. p =

Lecture 06. Fundamentals of Lidar Remote Sensing (4) Physical Processes in Lidar

Lecture 2: Global Energy Cycle

Optical Fiber Signal Degradation

Chapter 18. Fundamentals of Spectrophotometry. Properties of Light

LIGHT WAVES AND PARTICLES

Advanced Spectroscopy Laboratory

Lecture 26. Regional radiative effects due to anthropogenic aerosols. Part 2. Haze and visibility.

Energy and Radiation. GEOG/ENST 2331 Lecture 3 Ahrens: Chapter 2

Material Analysis. What do you want to know about your sample? How do you intend to do for obtaining the desired information from your sample?

p(θ,φ,θ,φ) = we have: Thus:

Nonlinear effects in optical fibers - v1. Miguel A. Muriel UPM-ETSIT-MUIT-CFOP

The Scattering of Light by Small Particles. Advanced Laboratory, Physics 407 University of Wisconsin Madison, Wisconsin 53706

Brillouin-Light-Scattering Spectroscopy

Example of a Plane Wave LECTURE 22

7. Aerosols and Climate

Secondary Ion Mass Spectrometry (SIMS)

Blackbody Radiation. A substance that absorbs all incident wavelengths completely is called a blackbody.

Chapter 3. Electromagnetic Theory, Photons. and Light. Lecture 7

Correlation Spectroscopy in Polymer Physics Methodenseminar im Wahlpflichtfach Basics diffusion and brownian motion correlations functions

Optics, Light and Lasers

Atmospheric Radiation

CHAPTER 6 INTRODUCTION TO SPECTROPHOTOMETRIC METHODS Interaction of Radiation With Matter

CHAPTER 6 INTRODUCTION TO SPECTROPHOTOMETRIC METHODS Interaction of Radiation With Matter

Infrared Spectroscopy: Identification of Unknown Substances

Liquid Crystals IAM-CHOON 1(1100 .,4 WILEY 2007 WILEY-INTERSCIENCE A JOHN WILEY & SONS, INC., PUBLICATION. 'i; Second Edition. n z

Chapter 6. Fiber Optic Thermometer. Ho Suk Ryou

Lecture 07. Fundamentals of Lidar Remote Sensing (5) Physical Processes in Lidar

SPECTRUM. Dispersion. This phenomenon can be observed in a lab environment using a

The Interaction of Acoustic Phonons and Photons in the Solid State

Lecture 06. Fundamentals of Lidar Remote Sensing (4) Physical Processes in Lidar

Lecture 0. NC State University

Preview from Notesale.co.uk Page 1 of 38

Lecture 6: Radiation Transfer. Global Energy Balance. Reflection and Scattering. Atmospheric Influences on Insolation

Lecture 6: Radiation Transfer

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information

3.4 Elliptical Parameters of the Polarization Ellipse References

Chapter 7: Optical Properties of Solids. Interaction of light with atoms. Insert Fig Allowed and forbidden electronic transitions

Building Blocks for Quantum Computing Part IV. Design and Construction of the Trapped Ion Quantum Computer (TIQC)

Light and Matter: Reading Messages from the Cosmos Pearson Education, Inc.

Ch Guided Reading Sound and Light

Raman and stimulated Raman spectroscopy of chlorinated hydrocarbons

PRINCIPLES OF REMOTE SENSING. Electromagnetic Energy and Spectral Signatures

Q1 and Q2 Review large CHEMISTRY

Nanophysics: Main trends

Rotational Raman Spectroscopy

ME 476 Solar Energy UNIT TWO THERMAL RADIATION

B 2 P 2, which implies that g B should be

Why is the sky blue?

Characterisation of vibrational modes of adsorbed species

Radiation in the atmosphere

Polarized Light. Second Edition, Revised and Expanded. Dennis Goldstein Air Force Research Laboratory Eglin Air Force Base, Florida, U.S.A.

CLASSICS. Handbook of Solar Radiation Data for India

Experiment AM3b: Raman scattering in transparent solids and liquids

Physics 9e/Cutnell. correlated to the. College Board AP Physics 2 Course Objectives

October Entrance Examination: Condensed Matter Multiple choice quizzes

Radiative Transfer Multiple scattering: two stream approach 2

Nanomagnetism a perspective from the dynamic side

CHEM6416 Theory of Molecular Spectroscopy 2013Jan Spectroscopy frequency dependence of the interaction of light with matter

Lecture 14. Principles of active remote sensing: Lidars. Lidar sensing of gases, aerosols, and clouds.

Lecture 4* Inherent optical properties, IOP Theory. Loss due to absorption. IOP Theory 12/2/2008

Spring 2009 EE 710: Nanoscience and Engineering

Lecture 05. Fundamentals of Lidar Remote Sensing (3)

Photochemical principles

9/12/2011. Training Course Remote Sensing - Basic Theory & Image Processing Methods September 2011

Chapter 33 Nature and Propagation of Light. From vision to digital camera to rainbows to pictures of the early universe light is all around us

Optical Characterization of Solids

Radiation in the Earth's Atmosphere. Part 1: Absorption and Emission by Atmospheric Gases

Lecture 28. Aerosol Lidar (4) HSRL for Aerosol Measurements

Introduction to Electromagnetic Radiation and Radiative Transfer

Laser Optics-II. ME 677: Laser Material Processing Instructor: Ramesh Singh 1

Optical Spectroscopy of Advanced Materials

Rb, which had been compressed to a density of 1013

Module 4 : Third order nonlinear optical processes. Lecture 28 : Inelastic Scattering Processes. Objectives

object objective lens eyepiece lens

INTRODUCTION Radiation differs from conduction and convection in that it does not require the presence of a material medium to take place.

The Raman Effect. A Unified Treatment of the Theory of Raman Scattering by Molecules. DerekA. Long

Transcription:

INTRODUCTION Definition:- Light scatteringis a form ofscatteringin whichlightis the form of propagating energy which is scattered. Light scattering can be thought of as the deflection of arayfrom a straight path, for example by irregularities in the propagationmedium,particles, or in the interface between two media. Scattering is a general physical process whereby some forms of radiation, such as light or moving particles, for example, are forced to deviate from a straight trajectory by one or more localized non-uniformities in the medium through which it passes.

Most objects that one sees are visible due to light scattering from their surfaces. Indeed, this is our primary mechanism of physical observation. Scattering of light depends on thewavelengthorfrequencyof the light being scattered. Since visible light has wavelength on the order of amicrometre, objects much smaller than this cannot be seen, even with the aid of a microscope. Colloidal particles as small as 1µm have been observed directly in aqueous suspension.

IMPORTANCE OF SCATTERING OF LIGHT The interaction of light with matter give important information about the structure and dynamics of the material being examined. If thescattering centres are in motion, then the scattered radiation is Doppler shifted. An analysis of the spectrum of scattered light can thus yield information regarding the motion of the scattering center. Periodicity or structural repetition in the scattering medium will cause interference in the spectrum of scattered light.

Thus, a study of the scattered light intensity as a function of scattering angle gives information about the structure, spatial configuration, or morphology of the scattering medium. With regard to light scattering inliquidsandsolids, primary material considerations include: 1. Crystallinestructure: Howclose-packedits atoms or molecules are, and whether or not the atoms or molecules exhibit the long-range order evidenced in crystalline solids. 2. Glassystructure: Scattering centres include fluctuations in density and/or composition. 3. Microstructure: Scattering centres include internal surfaces in liquids due largely to density fluctuations, and micro structural defects in solids such as grains, grain boundaries, and microscopic pores. In the process of light scattering, the most critical factor is the length scale of any or all of these structural features relative to the wavelength of the light being scattered.

General Process:- When light passes through a substance or gas, a part of it is absorbed and the rest scattered away. The basic process in scattering is absorption of light by the molecules followed by re-radiation in different directions. The strength of scattering can be measured by the loss of energy in the light beam as it passes through the medium. In absorption the light energy is converted into the internal energy of the medium and in scattering the light energy is radiated in other directions. Note :- The strength of scattering depends on the size of the particle causing the scattering and the wavelength of light.

Types Of Scattering Tyndall Scattering Mie Scattering Brillouin Scattering Raman Scattering Rayleigh Scattering

Tyndall Scattering TheTyndall effect, also known astyndall scattering, islight scatteringby particles in acolloidor particles in a finesuspension. It is named after the 19th century physicistjohn Tyndall. In this, the intensity of the scattered light depends on the fourth powerof the frequency, so blue light is scattered much more strongly than red light. Under the Tyndall effect, the longer-wavelength light is more transmitted while the shorterwavelength light is more reflected via scattering.

The Tyndall effect is seen when lightscattering particulate-matter is dispersedin a light-transmitting medium, when the crosssection of an individualparticulateis the range of roughly between 40 and 900 nanometres, i.e., somewhat below or near the wavelength of visible light (400 750 nanometres). The Tyndall effect is commercially exploited to determine the size and density of particles in aerosols and other colloidal matter.

Diagrammatic Representation

Mie Scattering Mie scatteringis a broad class of scattering of light by spherical particles of any diameter. The scattering intensity is generally not strongly dependent on the wavelength, but is sensitive to the particle size. Mie scattering coincides with Rayleigh scattering in the special case where the diameter of the particles is much smaller than the wavelength of the light; in this limit, however, the shape of the particles no longer matters. Mie scattering intensity for large particles is proportional to the square of the particle diameter.

Mie Scattering Codes Mie solutions are implemented in a number of codes written in different computer languages such as Fortran, Matlab, Mathematica. These solutions are in terms of infinite series and include calculation of scattering phase function, extinction, scattering, and absorption efficiencies, and other parameters such as asymmetry of parameter or radiation torque. Current usage of "Mie solution" indicate series approximation to solution of Maxwell's equations. There are several known objects which allow such a solution: spheres, concentric spheres, infinite cylinders, cluster of spheres and cluster of cylinders, there are also known series solutions for scattering on ellipsoidal particles.

Diagrammatic representation:-

Brillouin Scattering Brillouin scattering, named afterléon Brillouin, occurs whenlightin a medium (such as air,wateror acrystal) interacts with time-dependent opticaldensityvariations and changes its energy (frequency) and path.

The density variations may be due to acoustic modes, such asphonons, magnetic modes, such as magnons, or temperature gradients. Mechanism From a quantum perspective, Brillouin scattering is an interaction between an electromagnetic wave and a density wave (photonphonon scattering), magnetic spin wave (photon-magnon scattering), or other low frequency quasiparticle. The scattering is inelastic: the photon may lose energy to create a quasiparticle (Stokes process) or gain energy by destroying one (anti- Stokes process). This shift in photon frequency, known as the Brillouin shift. This is equal to the energy of the interacting phonon or magnon and thus Brillouin scattering can be used to measure phonon or magnon energies. The Brillouin shift is commonly measured by the use of a Brillouin spectrometer, based on a Fabry Pérot interferometer.

Comparison:-

Raman Scattering Raman scatteringis another form of inelastic light scattering, but instead of scattering from acoustic phonons, as in Brillouin scattering, the light interacts with optical phonons, which are predominantly intra-molecular vibrations and rotations with energies larger than acoustic phonons.

Raman scattering may therefore be used to determine chemical composition and molecular structure. Since most Raman lines are stronger than Brillouin lines, and have higher energies, standard spectrometers using scanningmonochromatorsmay be used to measure them. Raman spectrometers are standard equipment in many chemical laboratories.

Application:- Raman spectroscopyemploys the Raman effect for materials analysis. The spectrum of the Raman-scattered light depends on the molecular constituents present and their state, allowing the spectrum to be used for material identification and analysis. Raman spectroscopy is used to analyze a wide range of materials, including gases, liquids, and solids. Highly complex materials such as biological organisms and human tissue can also be analyzed by Raman spectroscopy. For solid materials, Raman scattering is used as a tool to detect high-frequency phonon and magnon excitations. Ramanlidaris used in atmospheric physics to measure the atmospheric extinction coefficient and the water vapour vertical distribution. Stimulated Raman transitions are also widely used for manipulating a trapped ion's energy levels, and thus basis qubit states. Raman amplification is used in optical amplifiers.

Rayleigh Scattering Rayleigh scatteringis theelasticscattering of light by molecules andparticulate mattermuch smaller than the wavelength of the incident light. The particles may be individual atoms or molecules. It can occur when light travels through transparent solids and liquids, but is most prominently seen in gases. Rayleigh scattering intensity has a very strong dependence on the size of the particles.

NOTE:- It is proportional the sixth power of the diameter of the particle. It is inversely proportional to the fourth power of the wavelength of light. This type of scattering is therefore responsible This type of scattering is therefore responsible for the blue colorof the sky during the day and the orange colorsduring sunrise and sunset. Rayleigh scattering is the main cause of signal loss in optical fibres.