The Anomalous Zeeman Splitting of the Sodium 3P States
|
|
- Steven Gregory
- 6 years ago
- Views:
Transcription
1 Advanced Optics Laboratory The Anomalous Zeeman Splitting of the Sodium 3P States David Galey Lindsay Stanceu Prasenjit Bose April 5, 010
2 Objectives Calibrate Fabry-Perot interferometer Determine the Zeeman splitting of the 3P energy state of the Sodium atom Determine effective nuclear charge of sodium atom Determine strength of internal magnetic field
3 Zeeman Effect - Historical Origin Zeeman Effect is named after Dutch Physicist, Pieter Zeeman. The experimental Evidence of this effect was published in: i) P. Zeeman, "The" Effect of Magnetisation on the Nature of Light Emitted by a Substance" Nature 55: 347. (1897) ii) P. Zeeman, "Doubles" and triplets in the spectrum produced by external magnetic forces". Phil. Mag. 44: 55. (1897) He obtained the Nobel Prize for Physics in 190. Dr. Pieter Zeeman
4 Zeeman Effect Zeeman Effect is the splitting of spectral lines into multiple lines in the presence of a static magnetic field Modern Uses: Nuclear magnetic Resonance Spectroscopy Electron-spin resonance spectroscopy Magnetic Resonance Imaging Mössbauer spectroscopy
5 Sodium Doublet A sodium Yellow doublet transition happens because of transition from 3p to 3s transition. The 3p level is split into states with total angular momentum (jl+s l+s) ) of j3/ and j1/ by the magnetic energy of the electron spin in the presence of the internal magnetic field caused by the orbital motion. In the case of the sodium doublet, the difference in energy for the 3p 3/ and 3p 1/ comes from a change of 1 unit in the spin orientation with the orbital part presumed to be the same.
6 Sodium Doublet Continued Energy Difference For Sodium doublet, j 1 as there is only spin shift from 1/ to -1/ or viceversa (m remains same) g Gyromagnetic ratio B magnetic field produced by the Nucleus when observed from the electron reference frame (Classical View point)
7 The Fabry-Perot Interferometer Path Difference for bright fringe: n f d(cos( θ )) mλ Fringes result from interference between multiple reflected beams, with bright fringes corresponding to constructive interference and dark fringes to destructive interference
8 Theory Fringe Patterns from Wavelength Components of light source coincide when: OPL OPL m λ m λ 1 1 Next Coincidence occurs at: ( m λ 1 + n) λ 1 ( m + n + 1) Where n number of fringes between coincidences λ λ λ 1 λ n
9 Theory Number of fringes is can be related to the mirror displacement by: Therefore, the difference in wavelengths is approximately: λ n d λ 1 λ 1 λ d d However, using average wavelength gives a more accurate result: λ avg () λ d (1) Since the average requires both wavelengths to be known, with only 1 wavelength, equation 1 can be used to get a first approximation. The results can then be used with equation to get a more accurate value.
10 For reflectivity of R0.85, Coefficient of Finesse: Theory Question 1/ π ( F) Finesse: F Minimum Wavelength Increment: ( λ ) F λ0 Finesse*n 4R (1 R) 4*0.85 (1 0.85) ( nm) 19.31* *1*159149nm 0 min f d Free Spectral Range: ( min nm λ0 ) FSR Finesse*( λ0) 19.31* nm ( λ 0 ) FSR nm Resolving Power: R λ nm * 10 nm ( λ ) nm 0 min
11 Theory Question Minimum Frequency Increment: ( υ 0 ) min c ( λ ) c ( λ ) min 5.319Hz 8 3*10 m / s *10 m ( υ0) min 0 Free Spectral Frequency Range: 8 3*10 m / 1.089*10 ( υ0) FSR 9 0 FSR s m ( υ 17 0) min.755* 10 Hz
12 Experimental Setup Laser Source Mirrors Diverging lens Telescope Micrometer Mirrors
13 Experimental Setup Telescope Movable mirror Collector lens Stationary mirror Mirror adjustment bar Micrometer
14 Procedure Calibration Assemble Fabry-Perot interferometer with the mirrors close, but not touching Record the value on the micrometer Rotate micrometer and count the number of fringes that pass Record the micrometer reading every 50 fringes until 500 fringes have passed
15 Procedure Calibration
16 Procedure Calibration Convert fringe count to mirror displacement and plot mirror displacement vs. micrometer displacement Slope of graph is the calibration factor, the amount the mirror moves per tic on the micrometer
17 Experimental Setup - Sodium Sodium lamp Filter Precision leveling device (Handbook of Mathematical Functions) Interferometer (same setup as laser)
18 Procedure Sodium Doublet Replace laser source with sodium source Sodium produces sets of fringe patterns Adjust mirror separation until patterns are coincident (each fringe is made up of closely spaced lines) Rotate micrometer in both directions and record position where the close lines start to blur, average the two numbers to determine the position of coincidence Rotate micrometer further and find another position of coincidence Repeat for 6+ coincidences
19 Procedure Sodium Doublet
20 Procedure Sodium Doublet
21 Procedure Sodium Doublet
22 Procedure Sodium Doublet Convert micrometer displacements to mirror displacements using previous calibration factor Plot mirror displacement vs. coincidence number Slope is d, the distance the mirror must move between two coincidences Calculate the energy difference between the two 3p states Using that, calculate the effective nuclear charge and the magnetic field
23 Results - Calibration MirrorDisp lacement FringeCoun t *Wavelength
24 Results - Calibration Calibratio nfactor ( ± E 3) µ m
25 Results Sodium Double (Trial 1) AvgCirc Re ading Circular Re ading1+ Circular Re ading CircDisplacement AvgCirc Re ading MirrorDisp lace CircDispla cement * Calibratio nfactor
26 Results Sodium Doublet (Trial 1) d ( ± 0.65) µm
27 Results Sodium Doublet (Trial 1) λ 1theo λ 1theo : nm λ 1 : d nm λ : λ λ 1 for i λ λ 1theo λ ( ) λ 1theo + λ λ avg λ λ avg d λ λ theo nm λ : λ 1theo λ : 0.597nm λ theo : nm nm ( ) 100 λ λ theo %err λ :.13 λ theo ( ) 100 λ λ theo %err λ : λ theo
28 Results Sodium Doublet (Trial 1) Energy separation between states: E : ( h c λ ) λ avg J Internal magnetic field: E E ev : J %err : ( ) 100 E ev E evtheo E evtheo Effective nuclear charge: n : 3 l : 1 E evtheo : m s : e : C h b : s m e : kg B : E ev h b m s e ( B 18T) 100 %err B : 18T m e T E ev n 3 l ( l + 1) Z eff :
29 Results Sodium Double (Trial ) AvgCirc Re ading Circular Re ading1+ Circular Re ading CircDispla cement AvgCirc Re ading MirrorDisp lace CircDispla cement * Calibratio nfactor
30 Results Sodium Doublet (Trial ) d ( 83.7 ± ) µm
31 Results Sodium Doublet (Trial ) λ 1theo : nm λ 1theo λ 1 : d nm λ : λ λ 1 for i λ λ 1theo λ ( ) λ 1theo + λ λ avg λ λ avg d λ nm λ theo : 0.597nm ( ) 100 λ λ theo %err λ :.507 λ theo λ : λ 1theo λ ( ) nm λ λ theo %err λ : λ theo
32 Results Sodium Doublet (Trial ) Energy separation between states: E : ( h c λ ) λ avg J Internal magnetic field: E E ev : J %err : ( ) 100 E ev E evtheo E evtheo Effective nuclear charge: n : 3 l : 1 E evtheo : m s : e : C h b : s m e : kg B : E ev h b m s e m e ( B 18T) 100 %err B : 18T T E ev n 3 l ( l + 1) Z eff :
33 Conclusions Wavelength separation λ nm ( ) 100 λ λ theo %err λ :.13 λ theo λ nm ( ) 100 λ λ theo %err λ :.507 λ theo Energy difference E : ( h c λ ) λ avg J E : ( h c λ ) λ avg J E E ev : J %err : ( ) 100 E ev E evtheo E evtheo %err : E E ev : J ( ) E ev E evtheo E evtheo
34 Conclusions Effective nuclear charge E ev n 3 l ( l + 1) E ev n 3 l ( l + 1) Z eff : Z eff : Magnetic field B : E ev h b m s e m e T ( B 18T) 100 %err B : 18T B : E ev h b m s e m e ( B 18T) 100 %err B : 18T T 4.659
35 Conclusions/Observations Interferometer is extremely difficult to align and keep aligned, slightest bump throws the whole thing off, had to re-align using laser When rotating micrometer to increase mirror separation, spring pulling mirror back did not always do so smoothly or had to be manually pushed back Fringes became narrower as mirror separation decreased, made it very hard to see if there was coincidence or not Results ended up being very accurate despite problems, because once it was aligned and your eyes were used to seeing the fringes, they were extremely clear and could easily be read
36 Sources of Error Eyestrain Too much staring at fringes in one day and they start to be harder to focus on Random Measurement limitations Micrometer precision was limited Random Minor misalignment Mirrors might not have been perfectly parallel, could throw readings off slightly Random Resolution of device Though we used the range of positions where we could separate the e two closely spaced lines as our coincidence range, we could not resolve the fringes enough to be able to identify the exact position of maximum coincidence Narrow fringes at smaller mirror separation made position of coincidence even harder to see Systematic device limitations Random human vision limitations
37 References Advanced Optics Laboratory manual Lecture notes astr.gsu.edu/hbase/quantum/sodzee.html Beiser,, Arthur. Concepts of Modern Physics, 6 th ed. rference/multiplebeaminterferencenotes.html %3Bjsessionid5FA663719B44787A BE6CE
THE ZEEMAN EFFECT PHYSICS 359E
THE ZEEMAN EFFECT PHYSICS 359E INTRODUCTION The Zeeman effect is a demonstration of spatial quantization of angular momentum in atomic physics. Since an electron circling a nucleus is analogous to a current
More informationZeeman Effect. Rabia Aslam Chaudary Roll no: LUMS School of Science and Engineering. Friday May 20, 2011
Zeeman Effect Rabia Aslam Chaudary Roll no: 2012-10-0011 LUMS School of Science and Engineering Friday May 20, 2011 1 Abstract In this experiment, we will observe the Zeeman effect which is defined as
More informationThe Zeeman Effect. Oisin De Conduin /2/2011
The Zeeman Effect Oisin De Conduin 07379510 2/2/2011 Abstract The purpose of this experiment was to study the splitting of a spectral line due to a magnetic field, known as the Zeeman effect. Specifically
More informationDepartment of Physics, Colorado State University PH 425 Advanced Physics Laboratory The Zeeman Effect. 1 Introduction. 2 Origin of the Zeeman Effect
Department of Physics, Colorado State University PH 425 Advanced Physics Laboratory The Zeeman Effect (a) CAUTION: Do not look directly at the mercury light source. It is contained in a quartz tube. The
More informationZeeman Effect. Alex Povilus Physics 441- Fall 2003 December 20, 2003
Zeeman Effect Alex Povilus Physics 441- Fall 2003 December 20, 2003 Abstract The Zeeman Effect is observed by application of a strong magnetic field to a mercury vapor cell and exciting transitions by
More informationExperiment O-2. The Michelson Interferometer
Experiment O-2 The Michelson Interferometer The Michelson interferometer is one of the best known and historically important interferometers. It is a very accurate length-measuring device and has been
More informationThe Zeeman Effect in Mercury Vapor and the Determination e/m by Fabry-Perot Interferometry
The Zeeman Effect in Mercury Vapor and the Determination e/m by Fabry-Perot Interferometry Edwin Ng MIT Department of Physics (Dated: March 17, 2012) We analyze the Zeeman fine structure of mercury vapor
More informationMichelson Interferometry and Measurement of the Sodium Doublet Splitting
Michelson Interferometry and Measurement of the Sodium Doublet Splitting PHYS 3330: Experiments in Optics Department of Physics and Astronomy, University of Georgia, Athens, Georgia 30602 (Dated: Revised
More informationINTERFEROMETERS. There are 4 principal types of measurements that can be made with this type of interferometer.
INTERFEROMETERS NOTE: Most mirrors in the apparatus are front surface aluminized. Do not touch the surfaces nor wipe them. they can be easily permanently damaged. Introduction This experiment provides
More informationAtomic Spectra HISTORY AND THEORY
Atomic Spectra HISTORY AND THEORY When atoms of a gas are excited (by high voltage, for instance) they will give off light. Each element (in fact, each isotope) gives off a characteristic atomic spectrum,
More informationThe Zeeman Effect refers to the splitting of spectral
Calculation of the Bohr Magneton Using the Zeeman Effect Robert Welch Abstract The Zeeman Effect was predicted by Hendrik Lorentz and first observed by Pieter Zeeman in 1896. It refers to the splitting
More informationTHE ZEEMAN EFFECT v3 R. A. Schumacher, May 2017 B. B. Luokkala, January 2001
THE ZEEMAN EFFECT v3 R. A. Schumacher, May 2017 B. B. Luokkala, January 2001 I. INTRODUCTION The goal of this experiment is to measure the Bohr magneton using the normal Zeeman effect of the 643.8 nm (red)
More informationInterferometers. PART 1: Michelson Interferometer The Michelson interferometer is one of the most useful of all optical instru
Interferometers EP421 Lab Interferometers Introduction: Interferometers are the key to accurate distance measurement using optics. Historically, when mechanical measurements dominated, interferometers
More informationMichelson Interferometer
Michelson Interferometer Objective Determination of the wave length of the light of the helium-neon laser by means of Michelson interferometer subsectionprinciple and Task Light is made to produce interference
More informationAtomic and nuclear physics
Atomic and nuclear physics Atomic shell Normal Zeeman effect LEYBOLD Physics Leaflets Observing the normal Zeeman effect in transverse and longitudinal configuration Spectroscopy with a Fabry-Perot etalon
More informationChapter 1. Optical Interferometry. Introduction
Chapter 1 Optical Interferometry Experiment objectives: Assemble and align Michelson and Fabry-Perot interferometers, calibrate them using a laser of known wavelength, and then use them characterize the
More informationZeeman Effect - Lab exercises 24
Zeeman Effect - Lab exercises 24 Pieter Zeeman Franziska Beyer August 2010 1 Overview and Introduction The Zeeman effect consists of the splitting of energy levels of atoms if they are situated in a magnetic
More informationZeeman effect - Wikipedia, the free encyclopedia
Zeeman effect From Wikipedia, the free encyclopedia The Zeeman effect (IPA: [ˈzeːmɑn], in English sometimes pronounced /ˈzeɪmən/) is the splitting of a spectral line into several components in the presence
More informationExperiment 10. Zeeman Effect. Introduction. Zeeman Effect Physics 244
Experiment 10 Zeeman Effect Introduction You are familiar with Atomic Spectra, especially the H-atom energy spectrum. Atoms emit or absorb energies in packets, or quanta which are photons. The orbital
More informationExperiment 6: Interferometers
Experiment 6: Interferometers Nate Saffold nas2173@columbia.edu Office Hour: Mondays, 5:30PM-6:30PM @ Pupin 1216 INTRO TO EXPERIMENTAL PHYS-LAB 1493/1494/2699 NOTE: No labs and no lecture next week! Outline
More informationIntroduction. Procedure. In this experiment, you'll use the interferometer to EQUIPMENT NEEDED: Lens 18mm FL. Component holder.
12-7137A Precision Interferometer Experiment 1: Introduction to Interferometry EQUIPMENT NEEDED: Basic Interferometer (OS-9255A) Laser (OS-9171) Laser Alignment Bench (OS-9172) Interferometer Accessories
More informationExperiment 8 Michelson Interferometer
Experiment 8 Michelson Interferometer Introduction This week s experiment utilizes the Michelson interferometer. You are to measure the wavelength of the green mercury light, the wavelength of the sodium
More informationDiffraction Gratings, Atomic Spectra. Prof. Shawhan (substituting for Prof. Hall) November 14, 2016
Diffraction Gratings, Atomic Spectra Prof. Shawhan (substituting for Prof. Hall) November 14, 2016 1 Increase number of slits: 2 Visual Comparisons 3 4 8 2 Diffraction Grating Note: despite the name, this
More informationThe Michelson Interferometer
Experiment #33 The Michelson Interferometer References 1. Your first year physics textbook. 2. Hecht, Optics, Addison Wesley - Chapter 9 in the 4th Ed. (2001). 3. Jenkins and White, Fundamentals of Optics
More informationRevisiting Fizeau s Observations: Spectral study of Na source using Newton s rings. Abstract
Revisiting Fizeau s Observations: Spectral study of Na source using Newton s rings K S Umesh #, Denny Melkay, J Adithya, Sai Prem Shaji, N Ganesh, R Dharmaraj, Rajkumar Jain, S Nanjundan # Author for correspondence:
More informationZeeman Effect Physics 481
Zeeman Effect Introduction You are familiar with Atomic Spectra, especially the H- atom energy spectrum. Atoms emit or absorb energies in packets, or quanta which are photons. The orbital motion of electrons
More informationAtomic emission spectra experiment
Atomic emission spectra experiment Contents 1 Overview 1 2 Equipment 1 3 Measuring the grating spacing using the sodium D-lines 4 4 Measurement of hydrogen lines and the Rydberg Constant 5 5 Measurement
More informationMeasurments with Michelson interferometers
Please do not remove this manual from from the lab. It is available at www.cm.ph.bham.ac.uk/y2lab Optics Measurments with Michelson interferometers Objectives In this experiment you will: Understand the
More informationMichelson Interferometer. crucial role in Einstein s development of the Special Theory of Relativity.
Michelson Interferometer The interferometer Michelson experiment Interferometer of Michelson and Morley played 0 a crucial role in Einstein s development of the Special Theory of Relativity. Michelson
More information2. OPERATIONAL CONDITIONS
1. INTRODUCTION This device was designed for modern physics labs of colleges and graduate schools. It demonstrates the influence of a magnetic field on light, known as Zeeman Effect, and reveals the behavior
More informationExperiment 3 1. The Michelson Interferometer and the He- Ne Laser Physics 2150 Experiment No. 3 University of Colorado
Experiment 3 1 Introduction The Michelson Interferometer and the He- Ne Laser Physics 2150 Experiment No. 3 University of Colorado The Michelson interferometer is one example of an optical interferometer.
More informationLABORATORY WRITE-UP MICHELSON INTERFEROMETER LAB AUTHOR S NAME GOES HERE STUDENT NUMBER:
LABORATORY WRITE-UP MICHELSON INTERFEROMETER LAB AUTHOR S NAME GOES HERE STUDENT NUMBER: 111-22-3333 MICHELSON INTERFEROMETER 1. PURPOSE The purpose of this experiment is to give some practice in using
More informationLecture 11: Polarized Light. Fundamentals of Polarized Light. Descriptions of Polarized Light. Scattering Polarization. Zeeman Effect.
Lecture 11: Polarized Light Outline 1 Fundamentals of Polarized Light 2 Descriptions of Polarized Light 3 Scattering Polarization 4 Zeeman Effect 5 Hanle Effect Fundamentals of Polarized Light Electromagnetic
More informationNORTHERN ILLINOIS UNIVERSITY PHYSICS DEPARTMENT. Physics 211 E&M and Quantum Physics Spring Lab #9: Diffraction Spectroscopy
NORTHERN ILLINOIS UNIVERSITY PHYSICS DEPARTMENT Physics 211 E&M and Quantum Physics Spring 2018 Lab #9: Diffraction Spectroscopy Lab Writeup Due: Mon/Wed/Thu/Fri, April 30/ May 2/3/4, 2018 Background All
More informationAtomic and nuclear physics
Atomic and nuclear physics Atomic shell Normal Zeeman effect LEYBOLD Physics Leaflets Observing the normal Zeeman effect in transverse and longitudinal Objects of the experiment Observing the line triplet
More informationExam 4. P202 Spring 2004 Instructor: Prof. Sinova
Exam 4 P202 Spring 2004 Instructor: Prof. Sinova Name: Date: 4/22/04 Section: All work must be shown to get credit for the answer marked. You must show or state your reasoning. If the answer marked does
More informationAny first year text, sections on atomic structure, spectral lines and spectrometers
Physics 33 Experiment 5 Atomic Spectra References Any first year text, sections on atomic structure, spectral lines and spectrometers Any modern physics text, eg F.K. Richtmeyer, E.H. Kennard and J.N.
More informationLecture 4: Polarimetry 2. Scattering Polarization. Zeeman Effect. Hanle Effect. Outline
Lecture 4: Polarimetry 2 Outline 1 Scattering Polarization 2 Zeeman Effect 3 Hanle Effect Scattering Polarization Single Particle Scattering light is absorbed and re-emitted if light has low enough energy,
More informationDiffraction I. Physics 2415 Lecture 37. Michael Fowler, UVa
Diffraction I Physics 2415 Lecture 37 Michael Fowler, UVa Today s Topics Michelson s interferometer The Michelson Morley experiment Single-slit diffraction Eye of a fly Angular resolution Michelson Interferometer
More informationUNITED SCIENTIFIC SUPPLIES, INC. OPERATION AND EXPERIMENT GUIDE
UNITED SCIENTIFIC SUPPLIES, INC. OPERATION AND EXPERIMENT GUIDE ZEEMAN EFFECT APPARATUS 1. Introduction This apparatus was designed for modern physics labs at universities and colleges. It demonstrates
More informationInterference- Michelson Interferometer. Interference lecture by Dr. T.Vishwam
Interference- Michelson Interferometer Interference lecture by Dr. T.Vishwam * Measurement of the coherence length of a spectral line * Measurement of thickness of thin transparent flakes * Measurement
More informationThe Grating Spectrometer and Atomic Spectra
PHY 192 Grating Spectrometer Spring 2012 1 The Grating Spectrometer and Atomic Spectra Introduction In the previous experiment diffraction and interference were discussed and at the end a diffraction grating
More informationPHYS 229: Experiment 1 Expansion Coefficients of Copper and Invar Bars Through Laser Interferometry
PHYS 229: Experiment 1 Expansion Coefficients of Copper and Invar Bars Through Laser Interferometry Jack Hong 30935134 Partner: Omar Mrani Zentar January 15, 2015 1 Introduction: When objects are heated,
More informationF 44 Normal Zeeman Effect
F 44 Normal Zeeman Effect Christina Schwarz Martin-I. Trappe (Dated: February 28, 2006) Abstract We first invesigate the normal Zeeman Effect of the red Cd line emerging from a gas discharge lamp in the
More informationLecture 4: Polarimetry 2. Polarizers and Retarders. Polarimeters. Scattering Polarization. Zeeman Effect. Outline
Lecture 4: Polarimetry 2 Outline 1 Polarizers and Retarders 2 Polarimeters 3 Scattering Polarization 4 Zeeman Effect Christoph U. Keller, Utrecht University, C.U.Keller@uu.nl Observational Astrophysics
More information(b) The wavelength of the radiation that corresponds to this energy is 6
Chapter 7 Problem Solutions 1. A beam of electrons enters a uniform 1.0-T magnetic field. (a) Find the energy difference between electrons whose spins are parallel and antiparallel to the field. (b) Find
More informationComplete all the identification fields below or 10% of the lab value will be deduced from your final mark for this lab.
Physical optics Identification page Instructions: Print this page and the following ones before your lab session to prepare your lab report. Staple them together with your graphs at the end. If you forgot
More informationSome Topics in Optics
Some Topics in Optics The HeNe LASER The index of refraction and dispersion Interference The Michelson Interferometer Diffraction Wavemeter Fabry-Pérot Etalon and Interferometer The Helium Neon LASER A
More informationPhysics 24, Spring 2007 Lab 2 - Complex Spectra
Physics 24, Spring 2007 Lab 2 - Complex Spectra Theory The optical spectra of isolated atoms consist of discrete, unequally spaced lines. This fact could not be understood on the basis of classical atomic
More informationExperimental Determination of the Mass of a Neutron
Experimental Determination of the Mass of a Neutron A. Andonian Department of Physics & Astronomy, Bates College, Lewiston, ME 04240, USA (Dated: April 13, 2016) The neutron is fundamental to our understanding
More informationThe Michelson Interferometer and the He-Ne Laser Physics 2150 Experiment No. 3 University of Colorado
Experiment 3 1 Introduction The Michelson Interferometer and the He-Ne Laser Physics 2150 Experiment No. 3 University of Colorado In the experiment, two different types of measurements will be made with
More informationCompendium of concepts you should know to understand the Optical Pumping experiment. \ CFP Feb. 11, 2009, rev. Ap. 5, 2012, Jan. 1, 2013, Dec.28,2013.
Compendium of concepts you should know to understand the Optical Pumping experiment. \ CFP Feb. 11, 2009, rev. Ap. 5, 2012, Jan. 1, 2013, Dec.28,2013. What follows is specialized to the alkali atoms, of
More informationLecture 09: Interferometers
1/31/16 PHYS 45 Fall semester 16 Lecture 9: Interferometers Ron Reifenberger Birck Nanotechnology Center Purue University Lecture 9 1 Two Types of Interference Division of Wavefront primary wavefront emits
More informationTHE MICHELSON INTERFEROMETER Intermediate ( first part) to Advanced (latter parts)
THE MICHELSON INTERFEROMETER Intermediate ( first part) to Advanced (latter parts) Goal: There is a progression of goals for this experiment but you do not have to do the last goal. The first goal is to
More informationOptical Pumping in 85 Rb and 87 Rb
Optical Pumping in 85 Rb and 87 Rb John Prior III*, Quinn Pratt, Brennan Campbell, Kjell Hiniker University of San Diego, Department of Physics (Dated: December 14, 2015) Our experiment aimed to determine
More informationThe Zeeman Effect in Atomic Mercury (Taryl Kirk )
The Zeeman Effect in Atomic Mercury (Taryl Kirk - 2001) Introduction A state with a well defined quantum number breaks up into several sub-states when the atom is in a magnetic field. The final energies
More informationChapter Electron Spin. * Fine structure:many spectral lines consist of two separate. lines that are very close to each other.
Chapter 7 7. Electron Spin * Fine structure:many spectral lines consist of two separate lines that are very close to each other. ex. H atom, first line of Balmer series n = 3 n = => 656.3nm in reality,
More informationInterference. Part-2. Gambar: Museum Victoria Australia
Interference Part-2 Gambar: Museum Victoria Australia Amplitude Splitting Interferometer S 2. Michelson Interferometer The principle: amplitude splitting d HM D F B M1 Detector C M1 E Interference at F
More informationThe Diffraction Grating
The Diffraction Grating If one extends the double slit to large number of slits very closely spaced, one gets what is called a diffraction grating. d sin θ. Maxima are still at d sin θ m = mλ, m = 0, 1,
More informationOptical Pumping of Rb 85 & Rb 87
Optical Pumping of Rb 85 & Rb 87 Fleet Admiral Tim Welsh PhD. M.D. J.D. (Dated: February 28, 2013) In this experiment we penetrate the mystery surrounding the hyperfine structure of Rb 85 and Rb 87. We
More informationTHE DIFFRACTION GRATING SPECTROMETER
Purpose Theory THE DIFFRACTION GRATING SPECTROMETER a. To study diffraction of light using a diffraction grating spectrometer b. To measure the wavelengths of certain lines in the spectrum of the mercury
More informationMIDSUMMER EXAMINATIONS 2001 PHYSICS, PHYSICS WITH ASTROPHYSICS PHYSICS WITH SPACE SCIENCE & TECHNOLOGY PHYSICS WITH MEDICAL PHYSICS
No. of Pages: 6 No. of Questions: 10 MIDSUMMER EXAMINATIONS 2001 Subject PHYSICS, PHYSICS WITH ASTROPHYSICS PHYSICS WITH SPACE SCIENCE & TECHNOLOGY PHYSICS WITH MEDICAL PHYSICS Title of Paper MODULE PA266
More informationMIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova
MIDTERM 3 REVIEW SESSION Dr. Flera Rizatdinova Summary of Chapter 23 Index of refraction: Angle of reflection equals angle of incidence Plane mirror: image is virtual, upright, and the same size as the
More informationLecture 11: Doppler wind lidar
Lecture 11: Doppler wind lidar Why do we study winds? v Winds are the most important variable studying dynamics and transport in the atmosphere. v Wind measurements are critical to improvement of numerical
More informationATOMIC SPECTRA. To identify elements through their emission spectra. Apparatus: spectrometer, spectral tubes, power supply, incandescent lamp.
ATOMIC SPECTRA Objective: To measure the wavelengths of visible light emitted by atomic hydrogen and verify the measured wavelengths against those predicted by quantum theory. To identify elements through
More informationFabry-Perot Interferometer for atmospheric monitoring useful for EAS detection E.Fokitis 1, K. Patrinos 1, Z. Nikitaki 1
Fabry-Perot Interferometer for atmospheric monitoring useful for EAS detection E.Fokitis 1, K. Patrinos 1, Z. Nikitaki 1 ABSTRACT A piezotunable Fabry-Perot interferometer is studied as a candidate Doppler
More informationNote to 8.13 students:
Note to 8.13 students: Feel free to look at this paper for some suggestions about the lab, but please reference/acknowledge me as if you had read my report or spoken to me in person. Also note that this
More informationPhysical Structure of Matter /07 Zeeman effect/ normal and anomalous version. Physics of the Electron. What you need:
Physical tructure of Matter Physics of the Electron /07 Zeeman effect/ normal and anomalous version What you can learn about Bohr s atom ic model Quan tisa tion of ener gy lev els Elec tron spin Bohr s
More informationMIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova
MIDTERM 3 REVIEW SESSION Dr. Flera Rizatdinova Summary of Chapter 23 Index of refraction: Angle of reflection equals angle of incidence Plane mirror: image is virtual, upright, and the same size as the
More informationAtomic Structure Ch , 9.6, 9.7
Ch. 9.2-4, 9.6, 9.7 Magnetic moment of an orbiting electron: An electron orbiting a nucleus creates a current loop. A current loop behaves like a magnet with a magnetic moment µ:! µ =! µ B " L Bohr magneton:
More informationThe Grating Spectrometer and Atomic Spectra
PHY 192 Grating Spectrometer 1 The Grating Spectrometer and Atomic Spectra Introduction In the previous experiment diffraction and interference were discussed and at the end a diffraction grating was introduced.
More informationPhysics 476LW Advanced Physics Laboratory Atomic Spectroscopy
Physics 476LW Atomic Spectroscopy 1 Introduction The description of atomic spectra and the Rutherford-Geiger-Marsden experiment were the most significant precursors of the so-called Bohr planetary model
More informationSpeed of Light in Air
Speed of Light in Air Electromagnetic waves represent energy in the form of oscillating electric and magnetic fields which propagate through vacuum with a speed c = 2.9979246x10 8 m/s. Electromagnetic
More informationEdward S. Rogers Sr. Department of Electrical and Computer Engineering. ECE426F Optical Engineering. Final Exam. Dec. 17, 2003.
Edward S. Rogers Sr. Department of Electrical and Computer Engineering ECE426F Optical Engineering Final Exam Dec. 17, 2003 Exam Type: D (Close-book + one 2-sided aid sheet + a non-programmable calculator)
More informationMASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Electrical Engineering and Computer Science
Student Name Date MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Electrical Engineering and Computer Science 6.161 Modern Optics Project Laboratory Laboratory Exercise No. 3 Coherence and Interferometry
More informationWhere are the Fringes? (in a real system) Div. of Amplitude - Wedged Plates. Fringe Localisation Double Slit. Fringe Localisation Grating
Where are the Fringes? (in a real system) Fringe Localisation Double Slit spatial modulation transverse fringes? everywhere or well localised? affected by source properties: coherence, extension Plane
More informationImproving and Characterizing a High Resolution Spectrograph For Use in Measuring the Zeeman Effect in Mercury Gas Emission Lines
Improving and Characterizing a High Resolution Spectrograph For Use in Measuring the Zeeman Effect in Mercury Gas Emission Lines Caitlin M. Pennington Department of Physics and Astronomy, Carthage College,
More informationMossbauer Spectroscopy
Mossbauer Spectroscopy Emily P. Wang MIT Department of Physics The ultra-high resolution ( E = E 10 12 ) method of Mossbauer spectroscopy was used to probe various nuclear effects. The Zeeman splittings
More informationInterference. Reminder: Exam 2 and Review quiz, more details on the course website
Chapter 9 Interference Phys 322 Lecture 25 Reminder: Exam 2 and Review quiz, more details on the course website Interferometers Wavefront-splitting interferometers Amplitude-splitting interferometers ed
More informationAtomic Spectra. d sin θ = mλ (1)
Atomic Spectra Objectives: To measure the wavelengths of visible light emitted by atomic hydrogen and verify that the measured wavelengths obey the empirical Rydberg formula. To observe emission spectra
More informationA beam of coherent monochromatic light from a distant galaxy is used in an optics experiment on Earth.
Waves_P2 [152 marks] A beam of coherent monochromatic light from a distant galaxy is used in an optics experiment on Earth. The beam is incident normally on a double slit. The distance between the slits
More informationHigher -o-o-o- Past Paper questions o-o-o- 3.4 Spectra
Higher -o-o-o- Past Paper questions 1991-2010 -o-o-o- 3.4 Spectra 1992 Q37 The diagram below shows the energy levels for the hydrogen atom. (a) Between which two energy levels would an electron transition
More informationLecture 6: Polarimetry 2. Polarizers and Retarders. Polarimeters. Scattering Polarization. Zeeman Effect. Hanle Effect. Outline
Lecture 6: Polarimetry 2 Outline 1 Polarizers and Retarders 2 Polarimeters 3 Scattering Polarization 4 Zeeman Effect 5 Hanle Effect Christoph U. Keller, Utrecht University, C.U.Keller@uu.nl Solar Physics,
More informationExperimental Physics I & II "Junior Lab" Fall Spring 2008
MIT OpenCourseWare http://ocw.mit.edu 8.13-14 Experimental Physics I & II "Junior Lab" Fall 2007 - Spring 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms.
More informationLecture 8: Polarimetry 2. Polarizers and Retarders. Polarimeters. Scattering Polarization. Zeeman Effect. Outline
Lecture 8: Polarimetry 2 Outline 1 Polarizers and Retarders 2 Polarimeters 3 Scattering Polarization 4 Zeeman Effect Christoph U. Keller, Utrecht University, C.U.Keller@uu.nl Observational Astrophysics
More informationFabry-Perot Interferometers
Fabry-Perot Interferometers Astronomy 6525 Literature: C.R. Kitchin, Astrophysical Techniques Born & Wolf, Principles of Optics Theory: 1 Fabry-Perots are best thought of as resonant cavities formed between
More informationThe Michelson Interferometer as a Device for Measuring the Wavelength of a Helium-Neon Laser
Journal of Advanced Undergraduate Physics Laboratory Investigation Volume 3 2017-2018 Article 2 2018 The Michelson Interferometer as a Device for Measuring the Wavelength of a Helium-Neon Laser Carly E.
More informationOPTICAL SPECTROSCOPY AND THE ZEEMAN EFFECT Beyond the First Year workshop Philadelphia, July Greg Elliott, University of Puget Sound
OPTICAL SPECTROSCOPY AND THE ZEEMAN EFFECT Beyond the First Year workshop Philadelphia, July 5-7 Greg Elliott, University of Puget Sound The Zeeman effect offers a striking visual demonstration of a quantum
More informationBrillouin-Light-Scattering Spectroscopy
Brillouin-Light-Scattering Spectroscopy 20th 21th of July 2010 Content Spin waves Brillouin Light Scattering (BLS) Quantum mechanical picture Conventional experimental setup Applications Time-resolved
More informationUNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics
UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics Physics 117.3 Physics for the Life Sciences FINAL EXAMINATION April 12, 2016 Time: 3 hours NAME: STUDENT NO.: (Last) Please Print
More informationChapter 8 Optical Interferometry
Chapter 8 Optical Interferometry Lecture Notes for Modern Optics based on Pedrotti & Pedrotti & Pedrotti Instructor: Nayer Eradat Spring 009 4/0/009 Optical Interferometry 1 Optical interferometry Interferometer
More informationPHYSICAL SCIENCES PART A
PHYSICAL SCIENCES PART A 1. The calculation of the probability of excitation of an atom originally in the ground state to an excited state, involves the contour integral iωt τ e dt ( t τ ) + Evaluate the
More informationPh 3455/MSE 3255 Experiment 2: Atomic Spectra
Ph 3455/MSE 3255 Experiment 2: Atomic Spectra Background Reading: Tipler, Llewellyn pp. 163-165 Apparatus: Spectrometer, sodium lamp, hydrogen lamp, mercury lamp, diffraction grating, watchmaker eyeglass,
More informationPHYSICS 359E: EXPERIMENT 2.2 THE MOSSBAUER EFFECT: RESONANT ABSORPTION OF (-RAYS
PHYSICS 359E: EXPERIMENT 2.2 THE MOSSBAUER EFFECT: RESONANT ABSORPTION OF (-RAYS INTRODUCTION: In classical physics resonant phenomena are expected whenever a system can undergo free oscillations. These
More informationEdward S. Rogers Sr. Department of Electrical and Computer Engineering. ECE318S Fundamentals of Optics. Final Exam. April 16, 2007.
Edward S. Rogers Sr. Department of Electrical and Computer Engineering ECE318S Fundamentals of Optics Final Exam April 16, 2007 Exam Type: D (Close-book + two double-sided aid sheets + a non-programmable
More informationLab 10: Spectroscopy & the Hydrogen Atom Phy208 Fall 2008
Lab 10: Spectroscopy & the Hydrogen Atom Phy208 Fall 2008 Name Section This sheet is the lab document your TA will use to score your lab. It is to be turned in at the end of lab. To receive full credit
More informationNormal and anomalous Zeeman effect
Normal and anomalous Zeeman effect LEP Related topics Quantization of energy levels, Bohr s atomic model, vector model of atomic states, orbital angular moment, electron spin, Bohr s magneton, interference
More information(M.I. - F.P.) Michelson and Fabry Perot Interferometers and Study of Channeled Spectra
Michelson and Fabry Perot Interferometers and Channeled Spectra (M.I. - F.P.) Michelson and Fabry Perot Interferometers and Study of Channeled Spectra References. ** Jenkins and White. Fundamentals of
More informationOptics Optical Testing and Testing Instrumentation Lab
Optics 513 - Optical Testing and Testing Instrumentation Lab Lab #6 - Interference Microscopes The purpose of this lab is to observe the samples provided using two different interference microscopes --
More informationSeat Number. Print and sign your name, and write your Student ID Number and seat number legibly in the spaces above.
Physics 123A Final Spring 2001 Wednesday, June 6 Name last first initial Seat Number Signature Student Number Print and sign your name, and write your Student ID Number and seat number legibly in the spaces
More information