User:Michael R Phillips/Notebook/Physics 307L/2008/10/29: Difference between revisions
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where s = Standard Deviation | where s = Standard Deviation | ||
and N = Number of Data Points | and N = Number of Data Points | ||
Here is our Excel worksheet for this lab: [[Media:Balmer.xlsx|Balmer.xlsx]] | |||
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Revision as of 14:16, 6 November 2008
 Balmer Series
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Balmer SeriesIntroduction & SafetyIn this lab, we will be using a very old Constant Deviation Spectrometer to measure the Rydberg constant based on the spectra of Hydrogen and Deuterium, and also the difference between the spectral wavelengths for these two, roughly following this lab manual. As for safety, the main thing is don't get electrocuted. This means turning off and unplugging the lamp power before removing or inserting a new bulb. Other important things to note, for equipment safety rather than our own, is that we should never touch the prism because we could easily damage it with fingerprints and that we should be very careful not to break the bulbs. CalibrationBefore we do any real data taking, we need to perform a simple calibration for our instrument. For this, we will use the given values of wavelengths (λ) and colors to match to our corresponding wavelengths and colors. In the end of the experiment, we will use this data to account for a kind of "calibration error" that will appear in every part of our data. Here is the data we took for initial calibration:
Along with the lines with given wavelengths, we found in our spectrum several low intensity lines that the lab manual indicated were from impurities in the sample. We also saw clearly the blue-green line that the manual directs us to skip. After taking all of this calibration data, we can use the average between our two values for each color and compare these to the values that were supplied to us so that we will have a good correction for the Hydrogen and Deuterium spectral data. Note: after taking this data and guessing as to what the method would be for calibration, we discovered that it was completely wrong! The correct way is to fix the prism rotation so that it gives us a perfect value for one of the middle wavelengths (like yellow or green). This will automatically give us good values for the rest of the experiment. This was done properly, calibrating to "yellow1" (579.0nm), before taking our actual data below. On day two, we started from here once more, calibrating our instrument before doing anything else. This time we calibrated to green (546.1nm). DataDay 1: For Hydrogen:
We were not able to conclusively locate the so-called blue line in the hydrogen spectra, and some of the sources on the web indicated that this is not a frequently used wavelength.
We weren't able to get a second wavelength value for Deuterium's "violet2" because we had to allow another group to have the lights on when we arrived at that color. This may throw off our averages slightly, but shouldn't be a big deal. One thing we noticed while getting this data, both for Hydrogen and for Deuterium, is that the intensity of the bands rose very much as a result of us just touching the power source for the tubes. We found this strange and couldn't come up with any explanation, but it seemed to be quite consistent and had nothing to do with any tilting that may occur from us touching it. Also important to note: we measured all of this data for day 1 from the red side of the spectrum. Day 2: For today, we will be doing the same procedure as before but measuring from the violet side of the spectrum. For Hydrogen:
After this obtaining this data, we switched to a different Hydrogen tube and measured some more data, this time starting from the red end of the spectrum. Hydrogen 2:
We could only find one working Deuterium tube, so we took one set of data measured from red and another measuring from violet but from the same tube. For Deuterium:
This data was from red. Deuterium 2:
This data was from violet. AnalysisThe theory that underlies this experiment is straightforward: as an electron from Hydrogen (or Deuterium) gets excited from the electric current passing through the gas in a tube, it rises to a higher energy state (higher than the ground state). After a very brief amount of time, this electron returns to the ground state and emits a photon, or bundle of light energy, which has a corresponding wavelength which we perceive as color. The reason we see many colors through our spectrometer is because the electron gets excited to many different energy states (corresponding to n=3, n=4, etc) then drops to the second energy state (n=2). The reason we say it drops to the second energy state and not to the first or to ground is (1) because it's the definition of a Balmer series and (2) because we wouldn't be able to see light from any larger drops (this light would be infrared or even longer in wavelength).
[math]\displaystyle{ \frac{1}{\lambda}=R(\frac{1}{2^2}-\frac{1}{n^2}), n=3,4,5,... }[/math] which relates our measured wavelengths, λ, to the Rydberg constant, R, with a couple of constants. The only thing we need to figure out from here is which color corresponds to which quantum number, n. The easiest way to handle all of our data is to plot λ vs n and determine a slope, a part of which will be R-dependent. Note: Upon doing this, we decided it was ridiculous to try to do some kind of fit with a quadratic type equation like λ(n) ends up being. Instead, we just used the below relations to calculate a Rydberg constant for both Hydrogen and Deuterium using averages. The function that we will use is: [math]\displaystyle{ \lambda(n)=\frac{4n^2}{R(n^2-4)}, n=3,4,5,... }[/math]
[math]\displaystyle{ n(\lambda)=\sqrt{\frac{4\lambda R}{\lambda R-4}} }[/math] which we use to decide which n corresponds to the red wavelength. From this, we found [math]\displaystyle{ n_{red}=3 }[/math] [math]\displaystyle{ n_{cyan}=4 }[/math] [math]\displaystyle{ n_{violet1}=5 }[/math] [math]\displaystyle{ n_{violet2}=6 }[/math] for Hydrogen. We can also surmise from this that Deuterium is the same way, e.g. the quantum numbers for the same colors are the same.
[math]\displaystyle{ \frac{1}{\lambda}=R(\frac{1}{m^2}-\frac{1}{n^2}), m=1,2,3,... , n=2,3,4,... , n\gt m }[/math] that is said to be more accurate (the first equation was discovered empirically while this one was a modified version to account for all wavelengths and is reinforced by Bohr's work). However, for our purposes, assuming m=2 and n=3,4,5,... is perfectly okay.
We will then compare our values of R to the actual value: [math]\displaystyle{ R_{accepted}=1.0967758\times10^7m^{-1} }[/math] using a percent error formula [math]\displaystyle{ %Error=\frac{|Accepted-Measured|}{Accepted}\times100 }[/math] We will also use Standard Deviation (using Excel) and the standard error of the mean, which is just [math]\displaystyle{ SEM=\frac{s}{\sqrt{N}} }[/math] where s = Standard Deviation and N = Number of Data Points
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