Fank-Hurtz Experiment
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Transcript of Fank-Hurtz Experiment
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The Frank-Hertz Experiment
March 25, 2014
Instructor: Prof. Robert Kramer
Dane Mettam
Lab Partners:
1. Abstract:
2. Introduction/Background:
3. Equipment Desc & Procedure:
4. Data:
5. Analysis:
6. Conclusion
Overall Lab Grade:
/ 100
/ 100
Robert Maldonado, Xuan Chen
1
1. Abstract
The Franck-Hertz effect is replicated in order to verify the claim that energy is
transferred in quantized packets. Energy loss of free electrons to inelastic collisions with
mercury is investigated. A discrete quantization interval is investigated by observing the
current as electrons collide with gaseous mercury in a vacuum diode. An accelerating
voltage is applied to a grid and when the electrons collide inelastically with the mercury
atoms, the current is dropped. This is done multiple times to determine the set voltage
required to excite mercury. Mercury was observed to absorb 4.93±0.53eV and produced a
249.6nm wavelength. Current levels dropped each time a mercury atom was excited and
thus produced a dramatic decrease in current at the observed eV intervals. This
experiment proved without a doubt that inelastic collisions absorb the same amount of
energy at every collision, all the time.
2
2. Introduction/Background
It was found that energy levels are emitted and absorbed in discrete packages
called photons. From the Bohr model the equation E=hf (equation 1) was obtained which says
that the energy of any beam of light is dependent upon the frequency of the light. This
was proven by the photoelectric effect. However, these effects still were not observed
with electrons on atoms. In 1914, J. Frank and G. Hertz conducted an experiment to test
the Bohr model and observe excitation of atoms with discrete energy levels and compare
with the excited atoms spectrum.
In the replication of the Franck-
Hertz experiment, electrons are
thermionically emitted in an oven from
a cathode by an acelerating voltage
through a grid to another grid and to an
anode. In between the two grids is
mercury vapor that the electrons collide
with. Two types of collisions occur
between the electron and mercury atom, elastic and inelastic collisions. In the elastic
collisions, the electron bounces off of the atom like a bouncy ball on a hard floor. Some
energy is lost form the moving electron to the stationary atom but not much since the
atom is so much larger. However, if the electrons are provided with enough energy with
the accelerating voltage then it will collide inelastically. An in elastic collision will take
nearly all of the energy from the electron and transfer it to the atom. The atom now in an
excited state will eventually stabalize by emitting the energy it gained in the collision as
light with the same energy. The emission of light returns the atom to its ground state. The
light emitted can hit the cathode to release further electrons as in the photoelectric effect.
The electron after the collision, continues on to the second grid with the loss of energy. A
small retarding voltage of 1.5 Volts on the grid is enough to prevent the electron from
reaching the anode. All of the other electrons that had elastic collisions still have more
than enough energy left over to go through the retarding voltage to the anode where it is
read as a small current. The graph shows the electrons position in a vacuum tube with the
described set up as a function of position.
Graph 1: Set up for an observation of a single excitation
Image 1: Diagram of inside the Franck-Hertz Tube
3
Equation 3
There are two ways to measure the energy
levels absorbed and emitted by the atoms. The first
way is to detect the light it produces and measure its
wavelenth. This meathod is difficult and
impractical. The other meathod of measuring the
quantized energy levels is by measuring the current
with applied voltage. In this meathod, the current
will drop when the electrons collide inelastically. If
the electrons are given enough energy when initially
accelerated, they can have multiple collisions before they no longer have enough to
overcome the retarding voltage. Inelastic collisions will drastically reduce the current
and is seen on graph 2. If energy is indeed quantized, then the mercury atoms will take
the same amount of energy to exite it in every collision. This will be a dip in current at
regular voltage intervals. This regular interval will be the change in voltage (ΔV). The
observed ΔV is the same energy that the mercury atom absorbs. The emission of light
that it produces will be of the same magnitude. This energy should be the same as a line
in its spectrum of light. If ΔV is consistent and it corilates with a specific frequency of
light produced from mercury, then the theory that energy is quantized is validated. Also,
it will verify that atoms emit and absorb only in discrete amounts.
To verify this with the experiment, a larger voltage is applied to the electron so
that it can have multiple collisions. With mercury, ΔV is supposed to be 4.86eV which
corrilates to a wavelength of 253.7nm. To calculate the ΔV into the wavelenth, a simple
calculation is done. The voltage is divided form the constant 1237.8x10−9. 1.2378−6
𝛥𝑉=λ
As the temperature increases of the oven increases, the cathode also increases in
temperture which in turn increases the average energy of conduction electrons within the
cathode. As the electrons gain kinetic energy, they will eventually overcome the work
function of the cathode. So while the heat aids in the emission of electrons and vaporizes
the mercury, it also heats the anode which has its own work function. The work function
difference between the anode and cathode can be calculated with the first dip in current
versus the average. First an average of all of the ΔV is taken. The first ΔV should be
higher than the average and subtracted from each other. This gives the work function (ф).
𝛥𝑉̅̅ ̅̅ − 𝛥𝑉1 = ф
It is imperative that the temperture within the tube remains at a constant
temperature for the success of the experiment. The reason for this is that
mercury’s vapor pressure will vare greatly with temperature. Differences with the
temperature will create differences with the vapor pressure and will affect the overall out
come. If more heat is added then the vapor pressure will be higher. With a higher vapor
pressure, more elections will collide (N)which will inturn create more collisions per
volume (n). Increased collisions create flatter peaks in when analyzing current and
voltage. A lower temperature will allow more electrons to flow in to the anode and could
damage the tube. To calculate the change in pressure, the Clausius-Clapeyron equation is
Graph 2: Electron current as a
function of acceleration voltage
Equation 2
4
used. The equation when graphed gives a linear description of temperature (T) to pressure
(P). There are three constants with in it. ∆𝐻𝑣𝑎𝑝 which is the enthalpy of vaporization, R
which is the universal gas constant, and C which is dependent upon the type of material
used and gives the y-intercept.
𝑙𝑛 (𝑃𝑓
𝑃𝑖) = −
∆𝐻𝑣𝑎𝑝
𝑅(
1
𝑇𝑓+
1
𝑇𝑖) + 𝐶
The electrons, when they collide with the mercury atom doesn’t just keep going
straight, it scatters in different directions. Very little kinetic energy from collisions is lost
from elastic collisions of the electron on the atom. The atom will deflect the electron into
a different direction. The electron will collide multiple times throughout the tube and will
average out a mean free path. Normally the mean free path of a particle is represented
with λ but since that is already being used for the wavelength in this report, the mean free
path will now be represented with ( ). The scattering is affected by the cross section (σ)
of the mercury atom. The number density of mercury is the same number as the number
of collisions per unit volume (n) which can also be refered to as atoms/𝑐𝑚3. The mean
free path can be calculated with equation 5. To determine the probability of whether any
given electron will scatter while moving throught the vapor can be calculated with
equation 6. The cross section can be estimated with the experiment if desired and used to
find the thickness ( )of the vapor or the probability of scattering.
=1
√2𝑛𝜎 𝑃(𝑠𝑐𝑎𝑡𝑡𝑒𝑟) = 𝜎𝑛
Equation 4
Equation 5 Equation 6
5
3. Equipment Description and Procedure
1. Connect everything together and heat
up the mercury to 180±10̊C. Do not
exceed 200̊C. Wait 20 minutes for
mercury to heat up.
2. Set the ammeter or picometer to
measure positive and negative current.
3. With accelerating voltage at 0 volts,
increase the filament current until the
tube has an orange glow that is dim.
4. As filament current is increased; observe the anode current.
5. Ensure that the tube is not glowing blue and or white throughout the experiment.
If it does then lower the accelerating voltage by at least 10 volts.
6. Increase accelerating voltage to about 60 volts. Increase retarding voltage to 1.5
volts.
7. Record the current as a function of accelerating voltages. Repeat this step for
accelerating voltages of 50 volts, 40 volts, and 30 volts.
8. Record and calculate all data.
6
4. Data
The chart below shows all of the data collected from the picometer. Each time the
current dropped down to a point, that point was subtracted from the next lowest point to
create a potential difference. Each difference is roughly the same and represents the
quatization energy of electrons colliding with mercury atoms inelastically. All voltage
changes are summed up then divided by 21 (the number of potential differences) to
obtain the mean value. The value of each difference was then subtracted from the mean
value then squared to get all of the values in the right most column. These values were
then summed together and divided by 20 (number of trials minus one). This gave the
variance. The square root was then taken to give the standard deviation. The reported
value is the mean plus or minus the standard deviation or 4.93±0.53eV.
Mean Quantized Voltage and Standard Deviation
Low-V High-V ΔV mean Σ(ΔV-V)^2
60V
7.09 12.11 5.02 4.929524 0.008185907
12.11 16.88 4.77 4.929524 0.025447907
16.88 21.98 5.10 4.929524 0.029062067
21.98 27.15 5.17 4.929524 0.057828707
27.15 32.00 4.85 4.929524 0.006324067
32.00 36.87 4.87 4.929524 0.003543107
36.87 41.75 4.88 4.929524 0.002452627
41.75 46.55 4.80 4.929524 0.016776467
50V
7.11 10.75 3.64 4.929524 1.662872147
10.72 15.75 5.03 4.929524 0.010095427
15.74 20.41 4.67 4.929524 0.067352707
20.41 25.64 5.23 4.929524 0.090285827
25.64 30.42 4.78 4.929524 0.022357427
30.42 35.19 4.77 4.929524 0.025447907
40V
8.65 13.64 4.99 4.929524 0.003657347
13.64 18.37 4.73 4.929524 0.039809827
18.37 23.54 5.17 4.929524 0.057828707
23.54 28.12 4.58 4.929524 0.122167027
30V
5.02 11.51 6.49 4.929524 2.435085347
11.51 17.20 5.69 4.929524 0.578323747
17.20 21.49 4.29 4.929524 0.408990947
Sum=103.5 Sum=5.673895238
Mean=4.930 Variance=0.283694762
Standard Deviation=0.532630042
Reported Value=4.93±0.53eV
Chart 1: Mean quantized voltage and standard deviation
7
The chart on the previous page
came from graphs such as the one
right. The graphs are the current as
a function of the accelerating voltages.
Two points are chosen as shown and
The difference is automatically
calculated. The error of each
measurement is approximated to how
certain the person moving the cursor
onto the right spot feels that it is
center. Unlike the picture to the right,
the points chosen were actually at the lower points where the current bottoms out. The
difference between each bottom is about the same.
Each bottom signifies that a mercury atom has absorbed that specific amount of
energy. It absorbs the same amount at each bottom and does not change regardless of
accelerating voltage.
The wavelength of the light
produced form the excited mercury is
calculated to be 249.6nm which is consistent
with the spectrum of mercury that has a
significant line at 253.7nm. The actual
energy that mercury needs to create this
wavelength is 4.86eV which is within the
error. The percent error of the energy
needed is 1.44% and the percent error for
the wavelength calculation is 1.62%. In the
image to the right, it is clearly seen that
mercury has a spike of light at around 254nm which is within the error of calculation.
The equation to convert the voltage to wavelength is below.
𝜆 =1237.8𝑥10−9
𝑒𝑉
The anode and cathode each has a different work function as is calculated using
the first ΔV in a set of ΔV for a given accelerating voltage and is subtracted from the
mean value. This gives the potential between the two probes.It only affects the first
calculation. This equation is given on page 3, equation 3. ф=1.56±0.53V.
Graph 3: Current as function of voltage with 60V accelerating voltage
Image 7: Spectrum wavelengths of Hg radiation
Equation 7
8
5. Analysis
The results of the experiment had very consistent results that signify a very low
probability for error. This shows with a percent error of 1.44% in the accelerating
voltage. The 4.93±0.53eV is within the error of 4.86eV. The mercury atom absorbs the
4.93±0.53eV of energy from the collisions and emits it in light quanta of equal value with
a frequency of 1.20x1015Hz and a wavelength of 249.6±54.6nm.
There were a few sources of error. Locating the right spot on each bottomed out
point since it was not perfectly pointed was probably the biggest source of error. Each of
those spots was varied a bit and not exact. Not many points were measured outside the
standard deviation, 80.95% of the ΔV were within 1 sigma of the error and 90.48% were
within 2 sigma. Another source of error was the heat of the oven. It was given in the lab
instructions that the temperature was supposed to be 180̊C but we kept it at 190±1̊C.
There was no adjustment in the calculations or in data collection to compensate for this.
The last source of error was the work function and potential between the anode and
cathode. The only initial voltage drop that makes sense to find the work function off of
was the final set when the accelerating voltage was set at 30 volts. This first value
should be higher than the rest but for whatever reason at 40V, 50V, and 60V; this was not
seen. The work function was calculated using only that number (6.49V) and the mean
voltage (ΔV).
One thing I was never able to figure out was what the constant 1237.8x10−9 was
from in determining the wavelength. This constant was found in Melissinos, Experiments
in Modern Physics but never derived. In short the accuracy of this constant cannot be
determined but it is a correct translation for electron volts to wavelength and provided me
with a very convenient way of determining the emitted spectrum frequency of mercury.
The error of the voltage was calculated by taking the mean of all of the ΔV. 𝛥𝑉̅̅ ̅̅
was then subtracted from each individual ΔV and then squared. The sum of all of these
was taken then divided by the number of trials minus 1 (20). The square root of this was
then taken to be 𝛿±0.53eV. This calculation is show below.
𝛿 = √∑(𝛥𝑉̅̅ ̅̅ −𝛥𝑉𝑖)2
𝑛−1
Equation 8
9
6. Conclusion
This experiment was extremely successful and it showed that energy is absorbed
and emitted in discrete packages. The energy lost form inelastic collisions matched the
energy needed for mercury to emit a 249.6nm photon. Mercury was observed absorb
4.93±0.53eV to produce the 249.6nm wavelength. This emission matches up with what is
seen from the spectrum of mercury on page 7. In this investigation of quantization of
mercury vapor in a vacuum diode, the current levels dropped each time a mercury atom
became excited from the inelastic collisions and this occurred at regular intervals of
4.93±0.53V. This experiment proved without a doubt that inelastic collisions absorb the
same amount of energy at every collision, all the time. It also verified the results first
seen by Franck and Hertz in 1914.
10
7. Assigned Questions
1. The mean free path of electrons propagating in a gas is given by 𝜆−1=σn where σ
is the total cross section summed for all processes, elastic and inelastic, and n is
the number density of the mercury. The number density can be found using the
tables for mercury vapor pressure in the CRC handbook. Assume that the elastic
scattering cross section is the area of a disk with the radius of a mercury atom.
Find the mean free path and 𝑡1/2 for the vapor at 180̊C. Compare this to the size
of the Franck-Hertz tube, and explain what is different in the case of elastic
scattering.
I could not find the vapor pressure of mercury or the size of the exact size of the tube.
Elastic scattering will move the electron in a random direction with almost all of its
momentum intact while inelastic collisions will eliminate most of its momentum and
energy.
2. Why is the retarding voltage needed to observe the Franck-Hertz effect?
The retarding voltage exists to ensure that electrons that scatter inelastically to not reach
the anode. That way, only elastic collisions are detected by the anode so that when a
sharp drop in the current is observed, it is the retarding voltage eliminating the electrons
that excite the mercury atoms. When it excites the atoms it loses most of its energy and
cannot move past it.
3. Should you use the positions of the peaks or of the valleys to determine the
excitation energy? Or both? Explain.
The valley points should be used when determining the excitation energy since it is a bit
sharper than the peaks. This will allow for a more precise measurement.
4. Why are some peaks and valleys smeared out rather than sharp?
The peaks and valleys are not pointed because of the energy dependence of the excitation
cross section and the fact that the thermionically emitted electrons are not distributed
evenly. Basically, the electrons are not evenly emitted from the cathode and the collisions
don’t exactly occur evenly at all point within the vacuum tube.
5. How would increasing the temperature affect your observations? Would there be
a higher or lower background current? Sharper of less sharp peaks? More peaks?
Increasing the temperature would increase the pressure of the mercury within the tube.
Increased pressure is calculated with the Clausius-Clapeyron equation. This would create
more collisions (N) and therefore more collisions per volume (n). Since each collision
11
produces ultraviolet light, the increased collisions would cause significantly more
electrons to be emitted via the photo electric effect. Overall, this will lower the current
that actually gets to the anode and mask continuous discharge. By the time you would
notice it being continuous, it would already be damaged. Additionally, there would be an
increase in inelastic electrons moving back towards the cathode because of the retarding
voltage. The number of peaks would be unaffected but they would be flatter.
6. Look up the spectrum for mercury to see if there is a spectral line (or lines) whose
wavelength (energy) corresponds to the energy differences you measured for
mercury.
There is a very prominent spectral line at 253.7nm that corresponds to the accepted
electron voltage of 4.86eV. A 249.6nm wavelength was calculated from the observed
4.93±0.53eV.
12
8. References Davidson, MW. Fundamentals of Mercury Arc Lamps. N.d. Chart. Zeiss Microscopy and Digital
Imaging, Tallahassee, Florida. Web. 8 Apr 2014. <http://zeiss-
campus.magnet.fsu.edu/articles/lightsources/mercuryarc.html>.
Franck-Hertz experiment with mercury. Diss. Leybold, Germany: Web.
Lab handout: PHYS 34300 Modern Physics; Robert Kramer, spring 2014 34300 lab.
Kramer, R. (2014). Modern physics notes. Informally published manuscript, Department of
Chemistry and Physics, Purdue University Calumet, Hammond, IN, Retrieved from
https://mycourses.purduecal.edu/webapps/portal/frameset.jsp?url=/webapps/blackboard/exec
ute/launcher?type=Course&id=_97498_1
Melissinos, A., & Napolitano, J. (2003). The franck-hertz experiment In J. Hayhurst
(Ed.), Experiments in Modern Physics. San Diego: Academic Press. doi:www.academicpress.com
Mettam, Dane. 2014. Photograph. n.p. Web. 25 Mar 2014.