Light Scattering Theory

Total Page:16

File Type:pdf, Size:1020Kb

Light Scattering Theory LIGHT SCATTERING THEORY Laser Diffraction (Static Light Scattering) © 2007 HORIBA, Ltd. All rights reserved. When a Light beam Strikes a Particle Some of the light is: z Diffracted Reflected Refracted z Reflected z Refracted Absorbed and z Absorbed and Reradiated Reradiated Diffracted Small particles require knowledge of optical properties: z Real Index (degree of refraction) z Imaginary Index (absorption of light within particle) z Light must be collected over large range of angles z Index values less significant for large particles © 2007 HORIBA, Ltd. All rights reserved. Diffraction Pattern © 2007 HORIBA, Ltd. All rights reserved. Diffraction Patterns © 2007 HORIBA, Ltd. All rights reserved. Young’s Experiment © 2007 HORIBA, Ltd. All rights reserved. Single vs. Double Slit Patterns Single slit diffraction pattern Double slit diffraction pattern © 2007 HORIBA, Ltd. All rights reserved. Fraunhofer Diffraction: Young’s Double Slit Distance between slits is INVERSELY proportional to angle (θ) nλ =d sin θ d=nλ / sin θ For a given measurement system with a fixed θ wavelength, the product nλ is constant n= order of diffraction λ = wavelength of light d= distance between slits θ = angle of diffraction © 2007 HORIBA, Ltd. All rights reserved. Fraunhofer Diffraction: Pinhole The diameter of the pinhole is INVERSELY proportional to angle (θ) nλ =d sin θ d=nλ / sin θ For a given measurement system with a fixed θ wavelength, the product nλ is constant n= order of diffraction λ = wavelength of light d= distance between slits θ = angle of diffraction © 2007 HORIBA, Ltd. All rights reserved. FRAUNHOFER DIFFRACTION - PARTICLE Angle of scatter from a particle is INVERSELY proportional to angle (θ) nλ =d sin θ d=nλ / sin θ For a given measurement system with a fixed θ wavelength, the product nλ is constant n = order of diffraction λ = wavelength of light d = distance between slits θ = angle of diffraction © 2007 HORIBA, Ltd. All rights reserved. Edge Scattering Phenomenon Light Scatter occurs whether from a slit, a pinhole or a particle. It occurs at the edge of an object. A SLIT and θ PARTICLE of the same size produce the same diffraction pattern θ θ © 2007 HORIBA, Ltd. All rights reserved. Fraunhofer Diffraction: Particles Large particles scatter light through SMALLER angles θ Small particles scatter light through LARGER angles Large Particle θ Small Particle © 2007 HORIBA, Ltd. All rights reserved. Diffraction Pattern: Large vs. Small Particles LARGE PARTICLE: z Low angle scatter z Large signal Wide Pattern - Low intensity SMALL PARTICLE: z High Angle Scatter z Small Signal Narrow Pattern - High intensity © 2007 HORIBA, Ltd. All rights reserved. Angle of Scatter vs. Particle Size Fraunhofer Diffraction describes forward scatter technology. Scatter angles are relatively small, less than 30° ANGLE OF SCATTER is INVERSELY proportional to particle size. SMALL particles scatter at larger angles than large particles. The AMOUNT OF LIGHT scattered is DIRECTLY proportional to particle size. LARGE particles scatter MORE light than small particles. © 2007 HORIBA, Ltd. All rights reserved. Light Scattering S1(Θ) and S2(Θ) are dimensionless, complex functions defined in general scattering theory, describing the change of amplitude in respectively the perpendicular and the parallel polarized light as a function of angle Θ with respect to the forward direction. Computer algorithms have been developed in order to allow computation of these functions and, thus, of I(Θ). © 2007 HORIBA, Ltd. All rights reserved. Plot of Airy Function I (W) λ = Wavelength of light A = Radius of Particle W = Angle with respect to optic axis 1.22λ 1.22λ 2.23λ 2.23λ 2A 2A 3.24λ 2A 2A 3.24λ 2A 2A W © 2007 HORIBA, Ltd. All rights reserved. Comparison of Models Fraunhofer (left) vs. Mie (right) © 2007 HORIBA, Ltd. All rights reserved. Fraunhofer Approximation dimensionless size parameter α = πx/λ; J1 is the Bessel function of the first kind of order unity. Assumptions: a) all particles are much larger than the light wavelength (only scattering at the contour of the particle is considered; this also means that the same scattering pattern is obtained as for thin two-dimensional circular disks) b) only scattering in the near-forward direction is considered (Q is small). Limitation: (diameter at least about 40 times the wavelength of the light, or a >>1)* If λ=680nm (.68 μm), then 40 x .68 = 27 μm If the particle size is larger than about 50 μm, then the Fraunhofer approximation gives good results. © 2007 HORIBA, Ltd. All rights reserved. Fraunhofer Approximation © 2007 HORIBA, Ltd. All rights reserved. Mie Theory © 2007 HORIBA, Ltd. All rights reserved. Mie vs. Fraunhofer 1.E+05 100 μm 1.E+04 1.E+03 3 μm 1.E+02 1.E+01 1.E+00 1.E-01 Relative Intensity 3.0 µm by Mie 1.E-02 3.0 µm by Fraunhofer 100.0 µm by Mie 1.E-03 100.0 µm by Fraunhofer 1.E-04 0.01 0.1 1 10 100 Angle in degrees Figure A.3 -- Comparison of scattering patterns of non-absorbing particles according to Fraunhofer and Mie calculations (Np = 1,59 – 0,0; nwater = 1,33; wavelength = 633 nm) © 2007 HORIBA, Ltd. All rights reserved. Extinction Efficiencies 4 5 Legend shows Legend shows 4.5 3.5 Particle Particle refractive index 4 Refractive Index 3 3.5 2.5 3 Efficiency 2 2.5 2 1.5 1.46 - 0.001 1.39 - 0.0 Extinction 1.5 Extinction Efficiency Extinction 1 1.46 - 0.02 1.59 - 0.0 1.46 - 0.05 1 1.79 - 0.0 0.5 1.46 - 0.1 0.5 1.99 - 0.0 1.46 - 0.2 2.19 - 0.0 0 0 0.1 1 10 100 0.1 1 10 100 Particle Size μm Particle Size μm Figure A.2 -- Extinction efficiencies in relation to particle size and refractive index (Mie prediction). (np and kp as indicated; nwater = 1,33; wavelength = 633 nm) (Fraunhofer assumes an extinction efficiency of 2 for all particle sizes) Good agreement for transparent particles >50 μm “ “ “ opaque particles > 2 μm © 2007 HORIBA, Ltd. All rights reserved. Scattering intensity pattern for single particles in relation to size 1.0E+11 For single 1.0E+10 Legend Particle 0.1 particles 1.0E+09 Size μm 1.0E+08 0.5 range from 1.0E+07 2 0.1 to 100 μm 1.0E+06 5 is 1013 1.0E+05 10 1.0E+04 100 Reduce by 1.0E+03 weighting to 1.0E+02 volume Relative Intensity 1.0E+01 1.0E+00 1.0E-01 1.0E-02 1.0E-03 1.0E-04 0.1 1 10 100 1000 Angle degrees Mie calculation; wavelength 633 nm; Np = 1,59 – 0,0 i; nm = 1,33 © 2007 HORIBA, Ltd. All rights reserved. Light intensity scattering patterns for equal particle volumes in relation to size 1.E+05 Weighting 1.E+04 Legend Particle 0.1 to third Size μm 0.5 power of 1.E+03 2 size 1.E+02 5 10 1.E+01 100 1.E+00 Relative Intensity 1.E-01 1.E-02 1.E-03 0.1 1 10 100 1000 Angle in degrees Mie calculation; wavelength 633 nm; Np = 1,59 – 0,0 ; nm = 1,33 © 2007 HORIBA, Ltd. All rights reserved. Influence of particle size on angular light intensity scattering patterns Width = 1% (COV) © 2007 HORIBA, Ltd. All rights reserved. Influence of imaginary parts of RI (absorbancies) Width = 1% (COV) © 2007 HORIBA, Ltd. All rights reserved. Influence of distribution width on angular light intensity scattering patterns © 2007 HORIBA, Ltd. All rights reserved. Result Calculation © 2007 HORIBA, Ltd. All rights reserved. Iterations © 2007 HORIBA, Ltd. All rights reserved. Iterations How many times to calculate new (better) results before reporting final result? For LA-930 standard = 30, sharp = 150 For LA-950 standard = 15, sharp = 1000 Fewer iterations = broader peak More iterations = narrow peak Too many iterations = fit to noise, over-resolved © 2007 HORIBA, Ltd. All rights reserved. Viewing Raw Data © 2007 HORIBA, Ltd. All rights reserved. LA-950 Optics © 2007 HORIBA, Ltd. All rights reserved. Why 2 Wavelengths? 30, 40, 50, 70 nm latex standards © 2007 HORIBA, Ltd. All rights reserved. Practical Application of Theory: Mie vs. Fraunhofer for Glass Beads © 2007 HORIBA, Ltd. All rights reserved. Practical Application of Theory: Mie vs. Fraunhofer for CMP Slurry © 2007 HORIBA, Ltd. All rights reserved. Conclusions It helps to know some of the theory to best use a laser diffraction particle size analyzer z Small particles – wide angles z Large particles – low angles Look at Intensity curves, R parameter & Chi square calculations Use Mie theory at all times (default whenever choosing an RI kernel other than Fraunhofer) © 2007 HORIBA, Ltd. All rights reserved..
Recommended publications
  • Glossary Physics (I-Introduction)
    1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay.
    [Show full text]
  • 12 Light Scattering AQ1
    12 Light Scattering AQ1 Lev T. Perelman CONTENTS 12.1 Introduction ......................................................................................................................... 321 12.2 Basic Principles of Light Scattering ....................................................................................323 12.3 Light Scattering Spectroscopy ............................................................................................325 12.4 Early Cancer Detection with Light Scattering Spectroscopy .............................................326 12.5 Confocal Light Absorption and Scattering Spectroscopic Microscopy ............................. 329 12.6 Light Scattering Spectroscopy of Single Nanoparticles ..................................................... 333 12.7 Conclusions ......................................................................................................................... 335 Acknowledgment ........................................................................................................................... 335 References ...................................................................................................................................... 335 12.1 INTRODUCTION Light scattering in biological tissues originates from the tissue inhomogeneities such as cellular organelles, extracellular matrix, blood vessels, etc. This often translates into unique angular, polari- zation, and spectroscopic features of scattered light emerging from tissue and therefore information about tissue
    [Show full text]
  • Solving the Quantum Scattering Problem for Systems of Two and Three Charged Particles
    Solving the quantum scattering problem for systems of two and three charged particles Solving the quantum scattering problem for systems of two and three charged particles Mikhail Volkov c Mikhail Volkov, Stockholm 2011 ISBN 978-91-7447-213-4 Printed in Sweden by Universitetsservice US-AB, Stockholm 2011 Distributor: Department of Physics, Stockholm University In memory of Professor Valentin Ostrovsky Abstract A rigorous formalism for solving the Coulomb scattering problem is presented in this thesis. The approach is based on splitting the interaction potential into a finite-range part and a long-range tail part. In this representation the scattering problem can be reformulated to one which is suitable for applying exterior complex scaling. The scaled problem has zero boundary conditions at infinity and can be implemented numerically for finding scattering amplitudes. The systems under consideration may consist of two or three charged particles. The technique presented in this thesis is first developed for the case of a two body single channel Coulomb scattering problem. The method is mathe- matically validated for the partial wave formulation of the scattering problem. Integral and local representations for the partial wave scattering amplitudes have been derived. The partial wave results are summed up to obtain the scat- tering amplitude for the three dimensional scattering problem. The approach is generalized to allow the two body multichannel scattering problem to be solved. The theoretical results are illustrated with numerical calculations for a number of models. Finally, the potential splitting technique is further developed and validated for the three body Coulomb scattering problem. It is shown that only a part of the total interaction potential should be split to obtain the inhomogeneous equation required such that the method of exterior complex scaling can be applied.
    [Show full text]
  • Solutions 7: Interacting Quantum Field Theory: Λφ4
    QFT PS7 Solutions: Interacting Quantum Field Theory: λφ4 (4/1/19) 1 Solutions 7: Interacting Quantum Field Theory: λφ4 Matrix Elements vs. Green Functions. Physical quantities in QFT are derived from matrix elements M which represent probability amplitudes. Since particles are characterised by having a certain three momentum and a mass, and hence a specified energy, we specify such physical calculations in terms of such \on-shell" values i.e. four-momenta where p2 = m2. For instance the notation in momentum space for a ! scattering in scalar Yukawa theory uses four-momenta labels p1 and p2 flowing into the diagram for initial states, with q1 and q2 flowing out of the diagram for the final states, all of which are on-shell. However most manipulations in QFT, and in particular in this problem sheet, work with Green func- tions not matrix elements. Green functions are defined for arbitrary values of four momenta including unphysical off-shell values where p2 6= m2. So much of the information encoded in a Green function has no obvious physical meaning. Of course to extract the corresponding physical matrix element from the Greens function we would have to apply such physical constraints in order to get the physics of scattering of real physical particles. Alternatively our Green function may be part of an analysis of a much bigger diagram so it represents contributions from virtual particles to some more complicated physical process. ∗1. The full propagator in λφ4 theory Consider a theory of a real scalar field φ 1 1 λ L = (@ φ)(@µφ) − m2φ2 − φ4 (1) 2 µ 2 4! (i) A theory with a gφ3=(3!) interaction term will not have an energy which is bounded below.
    [Show full text]
  • Zero-Point Energy of Ultracold Atoms
    Zero-point energy of ultracold atoms Luca Salasnich1,2 and Flavio Toigo1 1Dipartimento di Fisica e Astronomia “Galileo Galilei” and CNISM, Universit`adi Padova, via Marzolo 8, 35131 Padova, Italy 2CNR-INO, via Nello Carrara, 1 - 50019 Sesto Fiorentino, Italy Abstract We analyze the divergent zero-point energy of a dilute and ultracold gas of atoms in D spatial dimensions. For bosonic atoms we explicitly show how to regularize this divergent contribution, which appears in the Gaussian fluctuations of the functional integration, by using three different regular- ization approaches: dimensional regularization, momentum-cutoff regular- ization and convergence-factor regularization. In the case of the ideal Bose gas the divergent zero-point fluctuations are completely removed, while in the case of the interacting Bose gas these zero-point fluctuations give rise to a finite correction to the equation of state. The final convergent equa- tion of state is independent of the regularization procedure but depends on the dimensionality of the system and the two-dimensional case is highly nontrivial. We also discuss very recent theoretical results on the divergent zero-point energy of the D-dimensional superfluid Fermi gas in the BCS- BEC crossover. In this case the zero-point energy is due to both fermionic single-particle excitations and bosonic collective excitations, and its regu- larization gives remarkable analytical results in the BEC regime of compos- ite bosons. We compare the beyond-mean-field equations of state of both bosons and fermions with relevant experimental data on dilute and ultra- cold atoms quantitatively confirming the contribution of zero-point-energy quantum fluctuations to the thermodynamics of ultracold atoms at very low temperatures.
    [Show full text]
  • Discrete Variable Representations and Sudden Models in Quantum
    Volume 89. number 6 CHLMICAL PHYSICS LEITERS 9 July 1981 DISCRETEVARlABLE REPRESENTATIONS AND SUDDEN MODELS IN QUANTUM SCATTERING THEORY * J.V. LILL, G.A. PARKER * and J.C. LIGHT l7re JarrresFranc/t insrihrre and The Depwrmcnr ofC7temtsrry. Tire llm~crsrry of Chrcago. Otrcago. l7lrrrors60637. USA Received 26 September 1981;m fin11 form 29 May 1982 An c\act fOrmhSm In which rhe scarrcnng problem may be descnbcd by smsor coupled cqumons hbclcd CIIIW bb bans iuncltons or quadrature pomts ISpresented USCof each frame and the srnrplyculuatcd unitary wmsformatlon which connects them resulis III an cfliclcnt procedure ror pcrrormrnpqu~nrum scxrcrrn~ ca~cubr~ons TWO ~ppro~mac~~~ arc compxcd wrh ihe IOS. 1. Introduction “ergenvalue-like” expressions, rcspcctnely. In each case the potential is represented by the potcntud Quantum-mechamcal scattering calculations are function Itself evahrated at a set of pomts. most often performed in the close-coupled representa- Whjle these models have been shown to be cffcc- tion (CCR) in which the internal degrees of freedom tive III many problems,there are numerousambiguities are expanded in an appropnate set of basis functions in their apphcation,especially wtth regardto the resulting in a set of coupled diiierentral equations UI choice of constants. Further, some models possess the scattering distance R [ 1,2] _The method is exact formal difficulties such as loss of time reversal sym- IO w&in a truncation error and convergence is ob- metry, non-physical coupling, and non-conservation tained by increasing the size of the basis and hence the of energy and momentum [ 1S-191. In fact, it has number of coupled equations (NJ While considerable never been demonstrated that sudden models fit into progress has been madein the developmentof efficient any exactframework for solutionof the scattering algonthmsfor the solunonof theseequations [3-71, problem.
    [Show full text]
  • The S-Matrix Formulation of Quantum Statistical Mechanics, with Application to Cold Quantum Gas
    THE S-MATRIX FORMULATION OF QUANTUM STATISTICAL MECHANICS, WITH APPLICATION TO COLD QUANTUM GAS A Dissertation Presented to the Faculty of the Graduate School of Cornell University in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy by Pye Ton How August 2011 c 2011 Pye Ton How ALL RIGHTS RESERVED THE S-MATRIX FORMULATION OF QUANTUM STATISTICAL MECHANICS, WITH APPLICATION TO COLD QUANTUM GAS Pye Ton How, Ph.D. Cornell University 2011 A novel formalism of quantum statistical mechanics, based on the zero-temperature S-matrix of the quantum system, is presented in this thesis. In our new formalism, the lowest order approximation (“two-body approximation”) corresponds to the ex- act resummation of all binary collision terms, and can be expressed as an integral equation reminiscent of the thermodynamic Bethe Ansatz (TBA). Two applica- tions of this formalism are explored: the critical point of a weakly-interacting Bose gas in two dimensions, and the scaling behavior of quantum gases at the unitary limit in two and three spatial dimensions. We found that a weakly-interacting 2D Bose gas undergoes a superfluid transition at T 2πn/[m log(2π/mg)], where n c ≈ is the number density, m the mass of a particle, and g the coupling. In the unitary limit where the coupling g diverges, the two-body kernel of our integral equation has simple forms in both two and three spatial dimensions, and we were able to solve the integral equation numerically. Various scaling functions in the unitary limit are defined (as functions of µ/T ) and computed from the numerical solutions.
    [Show full text]
  • (2021) Transmon in a Semi-Infinite High-Impedance Transmission Line
    PHYSICAL REVIEW RESEARCH 3, 023003 (2021) Transmon in a semi-infinite high-impedance transmission line: Appearance of cavity modes and Rabi oscillations E. Wiegand ,1,* B. Rousseaux ,2 and G. Johansson 1 1Applied Quantum Physics Laboratory, Department of Microtechnology and Nanoscience-MC2, Chalmers University of Technology, 412 96 Göteborg, Sweden 2Laboratoire de Physique de l’École Normale Supérieure, ENS, Université PSL, CNRS, Sorbonne Université, Université de Paris, 75005 Paris, France (Received 8 December 2020; accepted 11 March 2021; published 1 April 2021) In this paper, we investigate the dynamics of a single superconducting artificial atom capacitively coupled to a transmission line with a characteristic impedance comparable to or larger than the quantum resistance. In this regime, microwaves are reflected from the atom also at frequencies far from the atom’s transition frequency. Adding a single mirror in the transmission line then creates cavity modes between the atom and the mirror. Investigating the spontaneous emission from the atom, we then find Rabi oscillations, where the energy oscillates between the atom and one of the cavity modes. DOI: 10.1103/PhysRevResearch.3.023003 I. INTRODUCTION [43]. Furthermore, high-impedance resonators make it pos- sible for light-matter interaction to reach strong-coupling In the past two decades, circuit quantum electrodynamics regimes due to strong coupling to vacuum fluctuations [44]. (circuit QED) has become a field of growing interest for quan- In this article, we investigate the spontaneous emission tum information processing and also to realize new regimes of a transmon [45] capacitively coupled to a 1D TL that is in quantum optics [1–11].
    [Show full text]
  • The Basic Interactions Between Photons and Charged Particles With
    Outline Chapter 6 The Basic Interactions between • Photon interactions Photons and Charged Particles – Photoelectric effect – Compton scattering with Matter – Pair productions Radiation Dosimetry I – Coherent scattering • Charged particle interactions – Stopping power and range Text: H.E Johns and J.R. Cunningham, The – Bremsstrahlung interaction th physics of radiology, 4 ed. – Bragg peak http://www.utoledo.edu/med/depts/radther Photon interactions Photoelectric effect • Collision between a photon and an • With energy deposition atom results in ejection of a bound – Photoelectric effect electron – Compton scattering • The photon disappears and is replaced by an electron ejected from the atom • No energy deposition in classical Thomson treatment with kinetic energy KE = hν − Eb – Pair production (above the threshold of 1.02 MeV) • Highest probability if the photon – Photo-nuclear interactions for higher energies energy is just above the binding energy (above 10 MeV) of the electron (absorption edge) • Additional energy may be deposited • Without energy deposition locally by Auger electrons and/or – Coherent scattering Photoelectric mass attenuation coefficients fluorescence photons of lead and soft tissue as a function of photon energy. K and L-absorption edges are shown for lead Thomson scattering Photoelectric effect (classical treatment) • Electron tends to be ejected • Elastic scattering of photon (EM wave) on free electron o at 90 for low energy • Electron is accelerated by EM wave and radiates a wave photons, and approaching • No
    [Show full text]
  • Optical Light Manipulation and Imaging Through Scattering Media
    Optical light manipulation and imaging through scattering media Thesis by Jian Xu In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2020 Defended September 2, 2020 ii © 2020 Jian Xu ORCID: 0000-0002-4743-2471 All rights reserved except where otherwise noted iii ACKNOWLEDGEMENTS Foremost, I would like to express my sincere thanks to my advisor Prof. Changhuei Yang, for his constant support and guidance during my PhD journey. He created a research environment with a high degree of freedom and encouraged me to explore fields with a lot of unknowns. From his ethics of research, I learned how to be a great scientist and how to do independent research. I also benefited greatly from his high standards and rigorous attitude towards work, with which I will keep in my future path. My committee members, Professor Andrei Faraon, Professor Yanbei Chen, and Professor Palghat P. Vaidyanathan, were extremely supportive. I am grateful for the collaboration and research support from Professor Andrei Faraon and his group, the helpful discussions in optics and statistics with Professor Yanbei Chen, and the great courses and solid knowledge of signal processing from Professor Palghat P. Vaidyanathan. I would also like to thank the members from our lab. Dr. Haojiang Zhou introduced me to the wavefront shaping field and taught me a lot of background knowledge when I was totally unfamiliar with the field. Dr. Haowen Ruan shared many innovative ideas and designs with me, from which I could understand the research field from a unique perspective.
    [Show full text]
  • 3 Scattering Theory
    3 Scattering theory In order to find the cross sections for reactions in terms of the interactions between the reacting nuclei, we have to solve the Schr¨odinger equation for the wave function of quantum mechanics. Scattering theory tells us how to find these wave functions for the positive (scattering) energies that are needed. We start with the simplest case of finite spherical real potentials between two interacting nuclei in section 3.1, and use a partial wave anal- ysis to derive expressions for the elastic scattering cross sections. We then progressively generalise the analysis to allow for long-ranged Coulomb po- tentials, and also complex-valued optical potentials. Section 3.2 presents the quantum mechanical methods to handle multiple kinds of reaction outcomes, each outcome being described by its own set of partial-wave channels, and section 3.3 then describes how multi-channel methods may be reformulated using integral expressions instead of sets of coupled differential equations. We end the chapter by showing in section 3.4 how the Pauli Principle re- quires us to describe sets identical particles, and by showing in section 3.5 how Maxwell’s equations for electromagnetic field may, in the one-photon approximation, be combined with the Schr¨odinger equation for the nucle- ons. Then we can describe photo-nuclear reactions such as photo-capture and disintegration in a uniform framework. 3.1 Elastic scattering from spherical potentials When the potential between two interacting nuclei does not depend on their relative orientiation, we say that this potential is spherical. In that case, the only reaction that can occur is elastic scattering, which we now proceed to calculate using the method of expansion in partial waves.
    [Show full text]
  • Lecture 7: Propagation, Dispersion and Scattering
    Satellite Remote Sensing SIO 135/SIO 236 Lecture 7: Propagation, Dispersion and Scattering Helen Amanda Fricker Energy-matter interactions • atmosphere • study region • detector Interactions under consideration • Interaction of EMR with the atmosphere scattering absorption • Interaction of EMR with matter Interaction of EMR with the atmosphere • EMR is attenuated by its passage through the atmosphere via scattering and absorption • Scattering -- differs from reflection in that the direction associated with scattering is unpredictable, whereas the direction of reflection is predictable. • Wavelength dependent • Decreases with increase in radiation wavelength • Three types: Rayleigh, Mie & non selective scattering Atmospheric Layers and Constituents JeJnesnesne n2 020505 Major subdivisions of the atmosphere and the types of molecules and aerosols found in each layer. Atmospheric Scattering Type of scattering is function of: 1) the wavelength of the incident radiant energy, and 2) the size of the gas molecule, dust particle, and/or water vapor droplet encountered. JJeennsseenn 22000055 Rayleigh scattering • Rayleigh scattering is molecular scattering and occurs when the diameter of the molecules and particles are many times smaller than the wavelength of the incident EMR • Primarily caused by air particles i.e. O2 and N2 molecules • All scattering is accomplished through absorption and re-emission of radiation by atoms or molecules in the manner described in the discussion on radiation from atomic structures. It is impossible to predict the direction in which a specific atom or molecule will emit a photon, hence scattering. • The energy required to excite an atom is associated with short- wavelength, high frequency radiation. The amount of scattering is inversely related to the fourth power of the radiation's wavelength (!-4).
    [Show full text]