Kinoform refraction lens with diffraction calculation

Similar documents
PROBLEM OF X-RAY SYNCHROTRON BEAM COLLIMATION BY ZONE PLATE

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

PRINCIPLES OF PHYSICAL OPTICS

Lecture 19 Optical MEMS (1)

Heating Beam Pattern Optical Design CO2 Laser Thermal Compensation Bench

PHY410 Optics Exam #3

Phys 531 Lecture 27 6 December 2005

Gaussian beam diffraction in inhomogeneous media of cylindrical symmetry

LECTURE 11 ELECTROMAGNETIC WAVES & POLARIZATION. Instructor: Kazumi Tolich

n The visual examination of the image of a point source is one of the most basic and important tests that can be performed.

LC circuit: Energy stored. This lecture reviews some but not all of the material that will be on the final exam that covers in Chapters

Lecture 11: Introduction to diffraction of light

21. Propagation of Gaussian beams

EE485 Introduction to Photonics

Vector diffraction theory of refraction of light by a spherical surface

3.5 Cavities Cavity modes and ABCD-matrix analysis 206 CHAPTER 3. ULTRASHORT SOURCES I - FUNDAMENTALS

Laser Intensity Modulation by Nonabsorbing Defects. M. D. Feit A. M. Rubenchik

Modeling of the propagation of Bessel beams in a uniaxial crystal at different positions of the crystal axis

Chapter 2 Basic Optics

Lecture 9: Introduction to Diffraction of Light

and the radiation from source 2 has the form. The vector r points from the origin to the point P. What will the net electric field be at point P?

1. Consider the biconvex thick lens shown in the figure below, made from transparent material with index n and thickness L.

P5 Revision Questions

RADIATION SOURCES AT SIBERIA-2 STORAGE RING

A Single-Beam, Ponderomotive-Optical Trap for Energetic Free Electrons

Synchrotron Radiation Representation in Phase Space

Beyond the Geometric toward the Wave Optical Approach in the Design of Curved Crystal and Multilayer Optics for EDXAS

Supplementary Materials for

3.1 The Plane Mirror Resonator 3.2 The Spherical Mirror Resonator 3.3 Gaussian modes and resonance frequencies 3.4 The Unstable Resonator

Computational Physics Approaches to Model Solid-State Laser Resonators

THE PARAXIAL WAVE EQUATION GAUSSIAN BEAMS IN UNIFORM MEDIA:

Waves & Oscillations

1 ESO's Compact Laser Guide Star Unit Ottobeuren, Germany Beam optics!


Optics for Engineers Chapter 9

Lecture 2: Geometrical Optics 1. Spherical Waves. From Waves to Rays. Lenses. Chromatic Aberrations. Mirrors. Outline

Light as Wave Motion p. 1 Huygens' Ideas p. 2 Newton's Ideas p. 8 Complex Numbers p. 10 Simple Harmonic Motion p. 11 Polarized Waves in a Stretched

Canalization of Sub-wavelength Images by Electromagnetic Crystals

Light.notebook May 03, 2016

Introduction to optical waveguide modes

LIST OF TOPICS BASIC LASER PHYSICS. Preface xiii Units and Notation xv List of Symbols xvii

Optics for Engineers Chapter 9

Course Secretary: Christine Berber O3.095, phone x-6351,

Atomic Diffraction Microscope of the de Broglie Waves

Nondifractive propagation of light in photonic crystals

Measurements in Optics for Civil Engineers

1. Waves and Particles 2. Interference of Waves 3. Wave Nature of Light

1/d o +1/d i =1/f. Chapter 24 Wave Optics. The Lens Equation. Diffraction Interference Polarization. The Nature of Light

Supporting Information

Physics of Light and Optics

PHYSICS PAPER 1 (THEORY)

Numerical Simulation of Light Propagation Through Composite and Anisotropic Media Using Supercomputers

A beam of coherent monochromatic light from a distant galaxy is used in an optics experiment on Earth.

OPSE FINAL EXAM Fall 2016 YOU MUST SHOW YOUR WORK. ANSWERS THAT ARE NOT JUSTIFIED WILL BE GIVEN ZERO CREDIT.

Michelson Interferometer

Lasers and Electro-optics

PHYSICS 253 SAMPLE FINAL EXAM. Student Number. The last two pages of the exam have some equations and some physical constants.

Astronomy 203 practice final examination

Single Emitter Detection with Fluorescence and Extinction Spectroscopy

Modeling microlenses by use of vectorial field rays and diffraction integrals

Optical Systems Program of Studies Version 1.0 April 2012

Two-Dimensional simulation of thermal blooming effects in ring pattern laser beam propagating into absorbing CO2 gas

arxiv: v1 [physics.optics] 1 May 2011

Step index planar waveguide

Electricity & Optics

IMPRS: Ultrafast Source Technologies

Einstein Classes, Unit No. 102, 103, Vardhman Ring Road Plaza, Vikas Puri Extn., Outer Ring Road New Delhi , Ph. : ,

Formation of the Holographic Image of a Diffuse Object in Second-Harmonic Radiation Generated by a Nonlinear Medium

Telescopes. Astronomy 320 Wednesday, February 14, 2018

OPSE FINAL EXAM Fall 2015 YOU MUST SHOW YOUR WORK. ANSWERS THAT ARE NOT JUSTIFIED WILL BE GIVEN ZERO CREDIT.

Application of nondiffracting beams to wireless optical communications

Exact radiation trapping force calculation based on vectorial diffraction theory

gives rise to multitude of four-wave-mixing phenomena which are of great

Curriculum interpretation

Analysis of second-harmonic generation microscopy under refractive index mismatch

Outline of College Physics OpenStax Book

OPTI 511L Fall A. Demonstrate frequency doubling of a YAG laser (1064 nm -> 532 nm).

Focal shift in vector beams

Labor für Photonik Prof. Dr. U. Wittrock. Executive. Summary

LECTURE 11 ELECTROMAGNETIC WAVES & POLARIZATION. Instructor: Kazumi Tolich

Spatial filtering with photonic crystals

Vågrörelselära och optik

Nature of Light Part 2

Physics 3312 Lecture 7 February 6, 2019

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

Designing a Computer Generated Hologram for Testing an Aspheric Surface

Modeling of the fringe shift in multiple beam interference for glass fibers

Optical/IR Observational Astronomy Telescopes I: Optical Principles. David Buckley, SAAO. 24 Feb 2012 NASSP OT1: Telescopes I-1

The physics of the perfect lens

Efficient sorting of orbital angular momentum states of light

If the wavelength is larger than the aperture, the wave will spread out at a large angle. [Picture P445] . Distance l S

FIBER OPTICS. Prof. R.K. Shevgaonkar. Department of Electrical Engineering. Indian Institute of Technology, Bombay. Lecture: 07

Design and Correction of optical Systems

Spatial Frequency and Transfer Function. columns of atoms, where the electrostatic potential is higher than in vacuum

On the possibility to create a prototype of laser system for space debris movement control on the basis of the 3-meter telescope.

Chapter 24 Photonics Question 1 Question 2 Question 3 Question 4 Question 5

Optics.

Optical Properties of Left-Handed Materials by Nathaniel Ferraro 01

a) Write expressions for the total E-field and total H-field amplitudes in the half-space z 0.

Plasmonics. The long wavelength of light ( μm) creates a problem for extending optoelectronics into the nanometer regime.

Transcription:

Kinoform refraction lens with diffraction calculation L.I.Ognev Nuclear fusion institute Russian Research Center «Kurchatov institute», Moscow, Russia Abstract By direct numerical simulations of the kinoform refractive lens within the quazioptical approach the effects of shape misalinement were investigated. The effect of π shift compensation was calculated for different orders and imperfections. The performance of kinoform lens was compared with the compound refractive lens and thin lens approximation. Introduction The diffraction model for forming of the x-ray beam passing through refractive lens [1,] was investigated. In contrast to the paraxial model of the refractive lens with the parabolic refraction profile [3] an arbitrary lens shape can be considered including the teethlike ( alligator ) lens []. The diffraction model is based on the integration of the parabolic equation for the complex amplitude of the electric field of the synchrotron radiation A(x,z). The longitudinal axis Z is oriented along the optical axis of the lens. The transversal coordinate is X. 0 0 ik A / z = A + k [( ε ε ) / ε ] A, (1) where k = ε ( ω / ) is wave vector, ε is dielectric permittivity of the material the lens is 0 c made. The initial value of the amplitude before the lens depends on the distance of the radiation source and its size. For coherent source A ( x, z = 0) = A 0 ( x ). () In the calculations the Gaussian beam was used A( x, z = 0) = exp( x / r 0 + iϕkx). Where ϕ is input angle to the lens axis. In most calculations was assumed ϕ=0. In the calculations the value for real part of the dielectric permittivity is (1-ε)=10-5 and imaginary

part is 10-7 for the x-ray beam energy 1.4 kev. The equation was integrated using step-bystep method [5]. For each step δz the splitting procedure was applied where the beam propagation between z and z+δz was calculated as diffraction in empty space and phase effects for refraction were added afterwards. The error of this procedure was estimated as O((δz) ) [6]. The results for the parabolic lens were compared with geometric optics model. The focus length of the single refractive lens can be obtained as F=R/(1-ε), (3) Where R is radius of curvature of the parabolic lens. For the given parameters of the lens the focus length was estimated as 665 mm. It can be seen that the results of the equation (1) are in a good agreement with thin lens approximation. High x-ray absorption in most material limits beam aperture for refractive lens [3]. To overcome this limitation the attempt to withdraw thickness of the length giving n π phase shift for given x-ray energy [4]. The most eleborated prototype of the device is kinoform fern-like planar lens consisting of many orders of parabolic lenses with subtracted n π phase shift thickness. The thickness step for the subtracted layer can be calculated as δd = nλ /(1 ε ) (4) In this work only first order kinoform profile was considered. The idea is illustrated with Fig.1, where parabolic shape is splitted in two parts with centaral parabolic zone and outer part with subtracted constant thickness. Fig. 1. The kinoform thickness model of the lens with n π phase shift subtraction. The outer parts of the planar lens are parabolas shifted to the bottom and the split between the parts is apodized on the 0.7 µm range. The transversal coordinate is shown in microns.

Results of calculations The transmission of x-ray beam through single refractive lens was calculated both for pure parabolic lens and kinoform 4π-phase shift lens and for lenses with reduced thickness by integrating of equation (1). The intensity on the axis behind the parabolic lens depending on the distance is shown on the Fig. with the solid line. The same calculation for the 4π-phase shift kinoform lens with equal curvature of central zone reveals small oscillations of the intensity (lines-points) and higher intensity peak in the focus. The effect may be understood as the result of smaller absorption. The effect is small in this case because the width of the Gaussian beam r 0 equals to the width of the central zone. So the portion of the beam transmitting through thick peripherals of the lens was rather small. Fig. The dependence of the intensity of x-ray beam on the optical axis on the distance behind the refractive lens for coherent 1.4 kev narrow beam for the parabolic lens (solid) and kinoform lens (lines-points) with 40 µm thickness of 0-zone. The distance is measured in millimeters. The variation of the kinoform lens thickness should effect the intensity of the focused beam behind the lens. The result of the symmetric deviation of the kinoform phase matching from its optimal value was shown on Fig. 3. When the thickness of the lens is reduced by 3

1.5% from its optimal thickness the intensity is lower by 10% than for the parabolic lens with same curvature. The initial beam width in this case was about the zero-order inner lens width and the initial beam had Gaussian intensity shape. Transversal intensity structure of the focal spot has nearly Gaussian profile. Fig.3 The on axis intensity distribution behind the parabolic lens (solid) and kinoform lens (lines-points) with 35 µm thickness of 0-zone. The distance is measured in millimeters. The same method was used for investigation of multiple lens which is a repetition of many individual lenses separated by empty space as it was made in the fern-like holographic lens [4]. The near field intensity distribution behind the lens is shown on Fig. 4. Both the increased absorption and the phase gap at the edge of the central refraction zone result in intensity fringes behind the lens. The intensity fringes are shown on Fig. 4. In the bottom of the figure the effective thickness of the lens in the vicinity of the gap is shown for comparison. The drop of the intensity in the vicinity of the kinoform gap is due to absorption of the beam. The oscillations look like interference pattern after the sharp edge. 4

Fig.4 Intensity distribution behind the single kinoform lens. In the bottom of the figure the effective thickness of the refractive lens lens in the visinity of the thickness gap is shown as the check point. 5

The effect of symmetrical phase mismatch of individual lenses on multiple kinoform lens Fig. 5 The on-axis intensity behind multiple kinoform refractive lens containing 0 components with symmetrically distorted phase matching. The distance between simple lenses was 40 µm. was investigated both in the near field intensity and far field on axis intensity near the focal spot. The individual lenses had reduced by 7% thickness. The near field fringes after the lens are similar to the case shown on Fig. 4 before. But the on-axis intensity behind multiple kinoform refractive lens containing 0 components with symmetrically distorted phase matching reveal pronounced interference oscillations as shown on Fig.5. Distance between simple lenses was 40 µm as in the optimal case. The stucture of the focal spot is shown on Fig. 6. No strong spacial peculiarities can be noticed in the case of symmetric distortions. 6

Fig. 6 Focal spot structure behind multiple kinoform refractive lens containing 0 components with distorted phase matching. Distance between simple lenses was 40 µm. Conclusion The diffraction model of the kinoform refractive x-ray lens shows that sharp edge at the border between 0-order and 1-order zones gives rise to near field intensity fringes. The effect can be experimentally observed. But in the far field zone there no drastic effect and focal spot has simple structure. The thickness symmetric variation of the kinoform lens results in intensity oscillations on the optical axis and reduction of the intensity in the focal spot compared to the parabolic lens. But no strong variations of the focal structure were found. The model can be extended to statistical variation of individual lenses shape and to partially coherent x-ray beams. 7

References 1. A. Snigirev, V. Kohn, I. Snigireva, B. Leneler, A compound refractive lens for focusing high-energy X-ray, Nature, v.384, n.7, p.49-51 (1996).. B. Cedestrom, R. Cahn, M. Danielsson, M. Lundquist, D. R. Nygren, Focusing hard X-rays with old LPs, Nature, v.404, 951 (000). 3. V. G. Kohn, On the Theory of X-ray Refractive Optics: Exact Solution for a Parabolic Medium, JETP Letters, v.76, n.10, pp. 600-603 (00). 4. I. Snigireva, A. Snigirev, C. Rau, T. Weitkamp, V. Aristov, M. Grigoriev, S. Kuznetsov, L. Shabelnikov, V. Yunkin, M. Hoffman, E. Voges, Holographic x-ray optical elements: transition between refraction and diffraction, NIM (A), v.a467-468, p.98-985 (001). 5. T. A. Bobrova, L. I. Ognev "Numerical simulation of gliding reflection of X-ray beam from rough surface", Preprint of Kurchatov Institute, IAE-6051/11, Moscow, 1997. http://arxiv.org/abs/physics/9807033. 6. J. A. Fleck Jr., J.R.Morris, M.D. Feit, Time-dependent propagation of high energy laser beams through the atmosphere, Applied Physics, v.10, n., p.19-160 (1976). 8