Charge-to-Mass Ratio (e/m) of the Electron
In this lab, an electron beam will be accelerated through a known voltage and then ejected into a magnetic field of known strength. Because of the magnetic field, it will then travel in a circle. We will use the radius of this circle to determine the charge-to-mass ratio (\(e/m\)) of the electron.Hoveroverthese!1
- 1 e/m apparatus consisting of:
- 1 set of Helmholtz coils (wires & mount)
- 2 DC power supplies (one for current in coils, one for accelerating voltage)
- 1 vacuum tube (with some low-pressure Helium gas)
- 1 electron gun
- 1 light-blocking hood
- 1 compass rose (w/ marking for magnetic North)
- Record data in this Google Sheets data table
Calculating \(e/m\)
In this lab, we'll be using the Lorentz force law, \(\vec{F}=q\vec{v}\times\vec{B}\), and the centripetal force law from classical mechanics, \(F_c=\frac{mv^2}{r}\).2
Let \(B_\perp\) denote the component of the magnetic field perpendicular to the plane of motion of the electron. Since the component of \(\vec{F}\) in the inwards direction is made by \(B_\perp\) (check this with the right-hand rule!), we can ignore the other components of magnetic field.
Since the inward magnetic force is the centripetal force and \(|q|=e\), we must have:
$$\frac{mv^2}{r}=evB_\perp\label{FEq}$$This would be nice if we knew the velocity. Fortunately, we know the voltage through which the electrons are accelerated. Setting the change in electrical potential energy equal to the final kinetic energy of the electrons, we find:
$$eV=\frac{1}{2}mv^2\label{EnEq}$$From this point, some algebra lets us eliminate the velocity variable entirely, giving us:
$$\frac{e}{m}=\frac{2V}{(B_\perp r)^2}\label{em}$$Helmholtz Coils
We'll be generating our magnetic field using a Helmholtz coil. This coil consists of two circles of wires (each \(N=130\) turns) specially configured to have their radius \(a\) equal to the separation distance between them. This makes the magnetic field in the center of the pair of coils as close to constant as possible.
In general, we know that magnetic field is proportional to the current that generates it:3
$$B=\alpha I\label{Bgen}$$The constant of proportionality \(\alpha\) in general depends on the geometry of the wires making the magnetic field and the point at which you measure. If we measure at the center of a Helmholtz coil of radius \(a\) with \(N\) turns, the constant \(\alpha\) is:
$$\alpha=\frac{8}{5\sqrt{5}}\frac{\mu_0 N}{a}\label{BHH}$$This means that our final formula for \(e/m\) will be:
$$\frac{e}{m}=\frac{2}{\alpha^2}\frac{V}{(Ir)^2}$$Or, rewritten in the form that we will plot:
$$V=\frac{\alpha^2}{2}\left(\frac{e}{m}\right)(Ir)^2$$First, grab a meter stick and measure the diameter, \(2a\), of the Helmholtz coil. Estimate an uncertainty on this value. Calculate the radius and propagate uncertainty.
Next, plug in and turn on your machine. Wait the 30 seconds it takes to boot up. Drape the hood over the top of the machine, if it is not there already.
Turn your voltage and current knobs until you see a green circle of light illustrating the electron beam. (About 200V and 1.5A are a reasonable starting point.) This circle may be dim, so look closely! It is easiest to see where it crosses the measuring rod in the center.1
Now: let's figure out which direction the magnetic field from the Helmholtz coil points. We will deduce this from how the electrons move.
One fact you need to know about the machine's setup to make this deduction: the electrons in the electron beam travel in a clockwise direction, when the machine is viewed from the front (i.e., from the side with the digital displays). [Note: this is talking about the electrons in the illuminated green beam, not the electrons in the loops of wire.]
With this information and your general knowledge of physics (including, but not limited to, the right-hand rule), deduce the direction of the magnetic field made by the Helmholtz coil. (The questions on your data sheet will guide you.)
Now, we want to align the machine so that the magnetic field generated by the machine is perpendicular to the magnetic field made by the Earth. (We want to be able to ignore the magnetic field of the Earth in our experiment, which we can more-or-less do if our magnetic field of interest is perpendicular.)
A few notes on how to do that. The building is more-or-less aligned with the cardinal directions, with one wall marked as true N. You should first align your compass rose so that N on the compass rose points to true north. Then, the compass rose will give you the direction of magnetic North/South, which of course is aligned with the Earth's magnetic field (neglecting vertical components).
That, combined with your deductions above, should give you enough information to align your machine so that its magnetic field is orthogonal to the Earth's. Do so.
Now, it is time to actually take measurements of the electron beam. Choose a value for current, and adjust your voltage until the beam is centered on the smallest marker. The marker tells you the diameter, in cm; record the diameter, the current, and the voltage (with associated uncertainties).
Then, increase the voltage until you hit the next marker, and again record the same quantities. Repeat until you hit the largest marker.
Then, choose another value for current, and repeat the process (again, for a variety of radii). You can stop when you get sufficiently many data points.
First, from coil diameter, calculate coil radius, \(a\). Then, calculate \(\alpha\) and its uncertainty.2
For each data point, calculate \(r\) from beam diameter, then calculate \((Ir)^2\). Propagate uncertainties.
Finally, make a plot of \(V\) vs. \((Ir)^2\). From the slope and your calculation of \(\alpha\), determine a measurement of \(e/m\) and compare to expectations.
Your TA will ask you to discuss some of the following points (they will tell you which ones):
- Derivation of Eq. \eqref{em}:
- Basic physics principles: Justify equations \eqref{FEq} and \eqref{EnEq} in your own words.
- Doing the algebra: From equations \eqref{FEq} and \eqref{EnEq}, show that equation \eqref{em} holds.
- Calculation of \(B\) Field of Helmholtz Coil:
- B field of a ring: Using the Biot-Savart law4, calculate the formula for the magnetic field on the z-axis generated by \(N\) turns of wire forming a ring of radius \(R\) that lies in the xy plane, through which passes a current \(I\).
- B field of two rings: Now consider a general "Helmholtz-like" setup: consider two parallel rings both with \(N\) turns, radius \(R\) and current \(I\). Suppose they lie in the planes \(z=\pm a/2\). Using the formula for the magnetic field of a ring, compute the magnetic field of this configuration on the z-axis. [You can just use your answer to the previous part and the principle of superposition; you don't need to use Biot-Savart again.]
- Why Helmholtz is Special: Compute the second derivative of that formula w.r.t. \(z\) at \(z=0\) (you may use Wolfram|Alpha to do this calculation). For what value of \(R\) does this second derivative vanish? What does that imply about the magnetic field near the center?3 How does this serve to explain why a Helmholtz coil is set up the way that it is?4
- Final Result (deriving eq. \eqref{BHH}): Take the result for the B field of two rings that you derived above and set \(R=a\) and \(z=0\). Show that you get equation \eqref{BHH} (with the definition of \(\alpha\) from \eqref{Bgen}).
- Other Magnetic Fields: First, based on your value for \(\alpha\) and a typical value from your data for \(I\) in this experiment, compute \(B_{HH}\), the magnetic field of your Helmholtz Coil. Then, compare it to...
- Earth's field: The horizontal component of the Earth's magnetic field is about 20μT. We avoided this impacting our experiment by orienting our machine correctly. Based on how this field compares to the field of our Helmholtz coil, is that a necessary course of action, do you think?
- Other coils: The coils don't only have magnetic fields inside; they make magnetic fields at some distance, too. Consider the magnetic field of the people across the table from you, and consider their coil as a magnetic dipole some distance away. First, compute the magnetic moment of it, based on the current, number of turns and (an estimate of) area. Then, using that magnetic moment, an estimate of how far apart your coil was from theirs, and the formula for the magnetic field of a magnetic dipole, get an order-of-magnitude estimate for the magnetic field that their wires caused at the center of your coil (as a "cross-talk" effect). Is this large enough to be concerned over in this experiment?
- Experimental limitations: Why is it far easier to measure \(e/m\) experimentally than either \(e\) or \(m\) individually (not just with this experiment, but with any setup)? Note: "the numbers involved are small" is not a complete answer; while that has elements of the truth, there's a deeper reason that you should get at.
- Using Protons: Suppose we were to attempt to use a similar machine to measure the charge-to-mass ratio of protons, instead. Suppose, for simplicity, that we can get a "source" for a beam of protons as we do here for electrons (with a similar setup). What complications (if any) do you expect?
- Variation in \(B\): At the edges of the coil, the deviations of the magnetic field from the value at the center is approximately 7%. This is an unaccounted-for uncertainty in our experiment. How does this compare to the other uncertainties you have in this lab?
Hovering over these bubbles will make a footnote pop up. Gray footnotes are citations and links to outside references.
Blue footnotes are discussions of general physics material that would break up the flow of explanation to include directly. These can be important subtleties, advanced material, historical asides, hints for questions, etc.
Yellow footnotes are details about experimental procedure or analysis. These can be reminders about how to use equipment, explanations of how to get good results, troubleshooting tips, or clarifications on details of frequent confusion.
The importance of and history of measurement of e/m is discussed many places, including Ginacoli Chapter 27, Section 7.
For a review of magnetic forces on free charges, see Giancoli Chapter 27.4 or Katz Chapter 30.8. For a review of circular motion, see Giancoli Chapter 5 or Katz section 4.3 and Chapter 6.
For a review of magnetic fields made by wires (and the relation to the current in those wires), see Giancoli Chapter 28 or Katz Chapter 30.
For a review of the Law of Biot et Savart see Giancoli Chapter 28.6 or Katz Chapter 30.4
Technically, this equation is not exactly correct: it assumes that the plane of motion of the electron is always perpendicular to \(B_{HH}\). While this is not exactly true, under an assumption that \(B_E\ll B_{HH}\), it is approximately true.
Protip: using relative errors here saves you a fair amount of effort in re-typing the prefactor, if you know how to do it.
We've done the computation w.r.t. \(z\), but for somewhat deeper reasons the assertion is also true in the \(x\) and \(y\) directions, for this specific choice of radius and separation distance.
This is only theoretical optimal if we talk "purely near the origin," and otherwise is only near-optimal. Better configurations exist if one cares about minimizing error over a larger region.
This is really the same measurement we did in part I, except in part I we took \(e/m\) as unknown and \(B_{HH}\) as known. Here, we take \(B_{HH}\) as unknown and \(e/m\) as known, but use the same relationship.
There are multiple ways ot write this relation. One way to do so is particularly nice because it breaks our fit into two "linear" pieces (which is nice to fit; see appendix C.2 of the Error Analysis Guide). We can fit it as \(B_{\perp}=A*f(\theta)+B*g(\theta)\) for some known functions \(f\) and \(g\) and some unknown parameters \(A\) and \(B\). As an extra challenge, try and determine the \(f\) and \(g\) that allow us to fit our data in this way (perhaps in addition to the more "obvious" way). For that \(f\) and \(g\), what is the physical interpretation of the corresponding \(A\) and \(B\)?
Sometimes it can appear more visibly if you look through a smartphone camera.
An alternative strategy: align your beam so that exactly one of the digits on the 10 (or 11) is lit up (say, just the "1" of the "10"). This can potentially avoid some "angle of viewing" problems, but may be difficult to do precisely if your beam is too broad. Do whatever you find easiest.
Excel, Google Sheets, etc. have built-in trigonometric functions, but they all assume that the argument is entered in radians, thus why we need that conversion.