Table of Contents

Hyperfine Spectroscopy of Rubidium - Winter 2022

In this experiment you will use a narrow bandwidth, tunable diode laser to probe the hyperfine structure of natural Rubidium (Rb). The technique of Doppler-free saturated absorption spectroscopy will be used to resolve the hyperfine structure which is otherwise masked by the effect of Thermal Doppler broadening of the spectral lines.

Introduction


Research


Before your first meeting with your TA, your group should do some background research.  You want to go into your first group meeting with the TA having some idea of:

What are you measuring?

  • What is the hyperfine effect?
  • What is the predicted magnitude of the hyperfine splitting for the first excited state of atomic Rb-87?

What is the experimental technique that you will use?

  • What is absorption spectroscopy?

What makes this measurement challenging and how is this challenge dealt with?

  • What is thermal doppler broadening and why does it prevent direct observation of the hyperfine splitting in Rb?
  • What is Doppler-free saturated spectroscopy?

Some other useful concepts.

  • What does bandwidth mean when used to describe a laser beam?
  • What is a natural linewidth when used to describe an atomic transition and how is it calculated?

This literature search should be done in the first few days of the lab. Break the subjects up among the group, and then get together to discuss what you have learned. In your first meeting with your TA, your goal is to make sure that you have a basic understanding of what it is that you are trying to measure and how you might go about making the measurement with the apparatus at your disposal. We will not tell you what to do and how to do it; we expect you to figure this out. What we will do is provide guidance and advice to make sure that your efforts are productive and to keep you moving on the right track.

Day 1 and Day 2 questions


Complete this question before coming to lab on Day 1.Late work will not be accepted.

DAY 1 QUESTION: An important concept in this experiment is the resolvability of spectral lines based on their spacing and width. This exercise is intended to illustrate why the experimental technique we employ is necessary. As is the convention in atomic physics, we will characterize photon energy differences in frequency (with units of MHz).

Consider the following two cases:

Case 1

First consider the case of an atom with two allowed transitions between different excited states to the ground states, where the energy difference between the two transitions is 3000 MHz. Although you may be used to thinking of atomic transitions as having very specific energies, they are not delta functions. An ensemble of atoms all emitting light from the the same transition will produce a range of photon energies about an average value. The spread of photon energies emitted by the ensemble can be characterized by the linewidth which is defined as the full width half maximum (FWHM) of the distribution of energies. The linewidth of the light detected in an experiment is determined by multiple factors including the uncertainty principle $\Delta E \Delta T \geq \hbar/2$ ), thermal doppler broadening, and the response characteristics of the detector. Suppose that as a result of these line-broadening effects the FWHM of each of our atomic transitions is 500 MHz.
Assume our detector measures the intensity of light emitted by a large ensemble of atoms emitting light from these two transitions. In your lab notebook, sketch (by hand) what you would expect a plot of light intensity versus frequency would look like.

Case 2

Now consider an atom with three transitions to the ground state where the energy difference between transitions 1 and 2 is 150 MHz and the difference between 2 and 3 is 300 MHz. Assume the FWHM of each transition is 500 MHZ (the same as in Case 1).

Now draw in your lab notebook what the light intensity versus frequency would look like.

If the goal of your experiment is to measure the transition energies, what impact does the linewidth have on these two cases?

Complete this question before coming to lab on Day 2.Late work will not be accepted.

DAY 2 QUESTION: Answer the following questions. (You may work on them in lab if you make enough progress on the experiment, but don't work on them at the expense of getting your optics aligned.)

(a) Use the quantum mechanical selection rules to determine the allowed hyperfine transitions for 87Rb(F = 2).

(b) For Rb atoms at room temperature, T = 300 K, calculate the line width due to Doppler-broadening in units of frequency. 

(c) Compare this linewidth to the frequency separations for appropriate the hyperfine transitions from Fig. 1. Do you expect to be able to resolve these hyperfine features based on the results of this comparison?
  1. The same technique is used to measure hyperfine splitting in positronium, which may help resolve discrepancies between measurements and Quantum Electrodynamic(QED) calculations.
    1. Follow-up precision measurements seem to indicate that there may be agreement with theory after all

Research


Before your preparation meeting with your TA, your and your lab partner(s) need to do some background research.  The purpose of this is so that you can go into your first meeting with the TA with a picture of what you need to measure, how those measurements will be made, what complications you are likely to encounter, and how you might deal with them. Then, at your first meeting you can focus on the details of what you need to do to start getting data to work with. Remember that you are expected to come to this meeting prepared to participate and demonstrate your understanding of these concepts.

Questions that your group should be prepared to answer are the following:

What are you measuring?

What is the experimental technique that you will use?

Some other useful concepts.

Theory and Apparatus


The following are links to our wiki pages discussing some of the concepts that you need to be familiar with. Outside of these links Google and Wikipedia are good sources of information if you come across concepts or terms you are not familiar with.

A description of the Hyperfine interaction as it applies to atomic Rb. Rb Hyperfine

A description of thermal doppler broadening of atomic emission/absorption lines for atoms in a gas. Thermal Doppler Broadening

A description of the technique of Doppler Free Saturated Absorption Spectroscopy. Doppler Free Saturated Absorption Spectroscopy

A description of using a Michelson Interferometer to calibrate the frequency sweep of a laser. Calibrating Frequency Sweep of Laser

A description of the optical components available for your use in the lab. Description of Optical Components

Notes on Experimental Procedure


LASER SAFETY

Details about how to safely operate the laser will be given in the lab by the instructor.

  • Always wear the protective laser goggles provided when the laser is on.
  • Note that the beam from the laser will cause permanent damage if it strikes your eye. If the laser is on and you are in the room you must wear the protective goggles provided. Additionally, anyone entering the room while the laser is on must be wearing goggles as well.
  • The laser beam is not harmful to the skin, so it is safe to operate with your hands in the beam. However, you should remove any reflective objects – such as watches and rings – from your hands and wrists before working on the optics table to prevent accidental deflection of the beam out of the plane of the table. 

Overview

By the time you get to the lab you should understand what it is that you will be measuring and have a plan for how you are going to do the experiment.

In the lab we provide you with everything you need to do the experiment. You have to select the optical components available, arrange them on the table to create the beam geometries that you need and align the beams so that they all go precisely where they need to go.

The heart of the experiment is a Toptica DL100 laser which produces a very narrow bandwidth beam which can be tuned over an appropriate frequency range for the measurement you need to make. The laser operates at wavelengths near 780nm. The power output can be as high as 120mW which makes it a class IIIB laser which can cause permanent damage to the eye. The process of placing and aligning optical components is when you are most likely to struck in the eye by a stray beam. In addition to the safety measures already discussed, you will do build and align your optics using a separate low power alignment light laser which is equivalent to a laser pointer used in presentations. Nevertheless you should still practice proper laser safety, even while working with the lower power alignment laser. You will also be sharing the laser and photo detectors other groups which will be working on their own version of the experiment on days when you are not in lab. To accommodate this you will arrange your optical components on a small 300mm x 600mm optical bread board which can be attached to the main optical table while you are working on it, and then removed and stored at the end of the lab period. When you return to the lab you simply reattach your optical setup to the main table and continue your work. The other groups sharing the laser will be doing the same.

If you think you need something which is not provided, ask the lab staff.

Main Optical Table

The above photo shows the main optical table on which you will be working, it is shared by all groups working on the experiment.

Mounted on this table are the main 780nm laser which will be used to perform the spectroscopy experiment. Two mirrors are used to direct the beam from this laser through a pair of irises. Your groups smaller optical table will bolt to the main optical table in the location shown, and then you can place and align all of your components on your table which can then be removed from the main table and stored in between lab sessions. The two optical tables are made with sufficient precision that you can easily return your table to the main table and all of your previous optical alignment will still be intact. The two irises are there to ensure that the laser beam always passes over the same path across the main table.

There is also a low power HeNe laser which will you can use to align your optics. You do not want to build your optical setup using the main laser for two reasons.

  1. The beam from the main laser is hazardous and can cause serious eye injury. Most accidents with laser beams occur during alignment work when you are moving optical around on the table.
  2. The beam from the main laser is almost invisible to the human eye and is difficult to see without the aid of beam cards and CCD cameras which are sensitive in the near infra red part of the spectrum.

The beam from the alignment laser is also directed through the same two irises that the main beam passes through. This is accomplished by using a flip mirror which can be flipped in and out of the beam path without changing its alignment. Using the flip mirror you can determine whether the main laser beam or the alignment beam is going through the irises.

Only one of the two lasers should ever be on at any given time. Either the main laser or the alignment laser. The main laser should only be turned on after you have completely aligned the optics using the alignment laser and you are ready to take data.

There are three photo diodes on in moveable mounts which can be positioned to detect the beams.

There is an inexpensive CCD camera which can be used to view the beam from the main laser.

There will also be a set of bolts and an allen wrench for attaching your optical table to the main table. Other apparatus shown in the photo but now actually on the optical table include:

The basic procedure can be summarized as follows:

This is likely to be an iterative process. You may have to go through the entire procedure outlined above more than once before you obtain acceptable results. This can be frustrating at times, but it is a part of lab work.

Individual Group Components

The photo below shows four smaller optical tables, each with a complete set of optics. Each lab group will use one of these tables and optics sets. Each group has an identical set of optical components which are more than sufficient to do the experiment.

Use only your optics, do not borrow or use components from any other groups set. Even if they are not using them. If you think you need additional components, or if one of yours is damaged talk to a member of the lab staff about obtaining what you need.

Under no circumstances should you disturb any of the other optical setups with belong to other groups. Be careful when retrieving and returning your table to the storage area so as not to bump someone else's setup.

Do not work on your table in the setup area. Take your table to the main optical table or to the free standing table at the far wall to work on it.

Each group has the following optical components to work with in designing and building your experiment.

Component Qty
Silver Mirror 5
50/50 Cube Beam Splitter 2
Linear Polarizer 2
780nm Half-Waveplate 1
Iris 2

Symbols

When drawing your optical layout you can use the following symbols to represent the different components on the table.

Mirror 50/50 Beam Splitter Linear Polarizer Photo Detector Rb Vapor Cell

Tips

Aligning optics is a skill which requires practice to get good at. If this is your first time working with laser optics you may find it a frustrating experience at times. Here are some tips to keep in mind while you work:

Video on Aligning Optics.

Once you have your optical paths setup and aligned, it is time to turn on the Toptica laser and use the flip mirror as shown in the video to switch from the guide laser to the main beam. Remember everyone in the room must be wearing goggles appropriate for the 120mW 180nm laser before the beam is turned on. The door should be closed and anyone entering the room will need to put on goggles before entering or the beam should be shutoff. You should also have all of the detectors on and connected to the scope and the scope should be on and triggering on the sync pulse from the Toptica laser before turning its beam on.

Use the IR card to follow the Topica beam and make sure that it is aligned the same as your guide beam was. At this point you should not have to do more than minor tweaking to the Toptica beam in order to have its alignment in good order.

Now you should find the signals from the photo-detectors on the scope and tune the laser onto resonance with the Rb Hyperfine transitions as shown in the video. Don't spend more than 20 minutes trying to tune the laser onto resonance. If you cannot get it to the point where you see at least three of the four doppler broadened peaks you should find the TA or one of the lab staff. Sometimes the laser itself needs a slight adjustment which is not something you can do yourself.

Video on tuning the laser onto resonance.

Once you have the Toptica laser sweeping over the Hyperfine transitions you can begin the process of optimizing the signal and and recording spectra. Part of the optimization process involves maximizing the overlap of the probe and pump beams. Another significant part of the process involves setting the power in the probe and pump beams. Finding the correct beam powers is accomplished through the process of trial and error. To help you in this process we provide a power meter with which you can measure the approximate power in the laser beam at any point on the table. In order to control how much of the laser power passes through the first iris on the main table we have placed a combination of a 1/2 waveplate and a polarizing beam splitter (pbs) in the main laser beam as shown in the following image. The pbs has been aligned to pass horizontally polarized light and reflect vertically polarized light. The 1/2 waveplate in front of the pbs allows you to rotate the plane of polarization of the light incident on the pbs, thus you can control how much of the laser light is horizontally polarized so that it passes through the pbs.

To get the beam powers in the correct range use the 1/2 waveplate and the power meter to set the power of the pump beam to be somewhere between 1mW and 1.5mW. The intensity of the probe beam should be about a factor of 5 or 6 less than the pump beam.

When You Leave The Lab

Since there will be other groups working on the apparatus it is your responsibility to ensure that everything in the lab is in order with the next group arrives. The room should be tidy and everything should be either put away or reset to it's default. If the lab room was in disarray when you arrived you are still responsible for leaving it in the appropriate state for the next group.. Here are some general tips on things to check before you leave.

Analysis and Final Report


Your analysis is due 4 days after your second day in lab. The analysis is not a lab report, rather it is all of the data reduction, number crunching, calculations, curve fitting, error propagation etc. which is necessary for you to establish your final conclusions. Think of it as being more like an extended homework set where you have to show how you got your final results.

Three days after your analysis submission your group will have a meeting with the TA to go over your analysis and make sure you are prepared to write your final report.

The final report is due three days after the analysis meeting.

Your graded analysis will be returned along with your graded final report.

Analysis

Three days after your analysis is due your group will meet with the TA to discuss the overall analysis and make clear what needs to go into your final report. Note that this meeting is not for the purpose of discussing your grade on the analysis, you will receive the grade on the analysis along with the graded final report. Instead this is an opportunity for the TA to have reviewed your analysis to identify where you may have short comings or misconceptions in your understanding of the experiment with the goal of improving what goes into your final report. It is also an opportunity for you to make sure that you understand what your TA is looking for in your report.

You are expected to bring a detailed outline for your final report to this meeting. The outline should consist of section and sub-section headings which make clear what information you will put into the report as well as the order in which that information will appear. This should literally be a single page document. Having a meaningfully thought out outline will count towards your participation grade for the meeting.

The expectation is that between feedback on your analysis and your outline you should leave this meeting with a clear idea of how you will write up your final report.

Analysis Rubric

Your analysis, like your reports, should be submitted as a single PDF. It is not expected that you will write narrative descriptions as you will in your final report. For the analysis it is acceptable to organize it into sections with one or two brief sentences of description. Things should be put in a sensible order so that the TA can follow what you are doing. For example plots, fits and calculations related to your energy calibration should be grouped together into a section, and that section should be placed before you apply the calibration to your data. For cases such as fitting and extracting peak locations for all of your scattering data it is sufficient to show one representative plot of a fit to the data along with a table containing all of the values. Scans or photographs of calculations done on paper or in your lab notebook are acceptable but absolutely MUST be clear and readable.

Each item below is graded on a 0-4 point scale:

All rubric items carry the same weight. The final grade for the analysis will be assigned based on the average (on a 4.0 scale) over all rubric items.

Item Good (4)
Data Reduction All relevant quantities with uncertainties have been extracted from the raw data. It is clear how the raw data was processed. When multiple data sets are processed in the same manner is it acceptable to show the process in detail for one data set and then tabulate the results for the remaining data.
Calibration All necessary instrumental calibration is done. Calculations are shown, uncertainties in measured quantities are included, final calibration relationship is provided.
Error Propagation Uncertainties are propagated properly and it is clear how this was done. In cases where the same propagation procedure is used for multiple data sets it is sufficient to show the details for one set and then tabulate the rest.
Measured values for hyperfine splitting Features in spectrum are properly identified, peak locations are extracted and their associated energy differences are calculated with uncertainties.
Comparison of measured energy splitting with literature values Measured energies are compared with uncertainties to the predicted values.
Other specific items which may have been discussed with your TA Anything else which your TA has made clear they expect to see in your analysis. Items in this category need to be discussed between the TA and Students before the end of their last day in lab and need to have been approved by the course instructor or a member of the lab staff.

Final Report


The final report is due three days after your scheduled analysis meeting with the TA.

Your final report will be evaluated based on the following rubric. The rubric is not a format for your analysis, you are not expected to have a specific section on Data Handling or Presentation of Data. Elements of the different rubric categories will appear at different points through out your analysis writeup. For example you will be presenting data in your discussion of the calibration, your discussion of determining peak locations, and likely in your final results. Your writeup of your analysis should be structured in a way that is clear and readable, there should be a logic to the flow of it.

Each item below is graded on a 0-4 point scale:

All rubric items carry the same weight. The final grade for the analysis will be assigned based on the average (on a 4.0 scale) over all rubric items.

Final Report Rubric

Section Good (4)
Optical Setup The optical setups used are clearly and completely described.
Flow The report is well organized and clearly written. The logical flow of how information is presented makes it easy for the reader to understand what is being communicated. Extraneous information unrelated to the conclusions is minimized.
Presentation of Data Presents plots of data as needed and uses them to support the narrative of the report. Properly labels plots, and makes presentation clean and clear. Uses error bars where appropriate. Includes captions that provide appropriate context. Presents all numerical values with appropriate units and significant figures. Clearly formats numbers, equations, tables, etc.
Data Handling Describes how the raw data was processed including with uncertainties. Details fit functions and provides sample fits (if appropriate). Details other calculations/considerations and provides sample calculations or reasoning (if appropriate).
Discussion of Uncertainties Identifies relevant sources of uncertainty in measured quantities, and quantifies values when possible. Describes how uncertainties were assessed and incorporated into the analysis. Identifies potential sources of systematic bias and describes how they are accounted for in the analysis or eliminated.
Presentation of Results Final results are presented clearly. Data tables and plots are used where appropriate and are properly labeled and annotated. Measured and calculated quantities include units and uncertainties where appropriate.
Conclusions Makes clear final conclusions that are fully supported by the experimental results and discusses the overall take-aways of the experiment appropriately. Properly accounts for or contextualizes measurement uncertainties and potential sources of systematic bias.