Rydberg Constant from Balmer Series Jordan Brown 4/20/11

Rydberg Constant from Balmer Series Jordan Brown 4/20/11

Rydberg Constant from Balmer Series Jordan Brown 4/20/11 “The most accurately measured fundamental physical constant.” [2] Background ● 1885: Johann Balmer experimentally determined 4 spectral lines of hydrogen in the visible spectrum. ● 1888: Johannes Rydberg determined a formula to predict the position of spectral lines in hydrogen-like atoms. ● Rydberg's formula is a modification of the Balmer formula with a constant Rm. ● 1913: Niels Bohr went on to present an updated model of the atom. He also empirically determined Rm from more fundamental constants. [1] Method ● Calibrate the apparatus ● Went on to measure alpha, beta, and gamma spectral ● Use Hg to determine lines. diffraction width. ● Determined Rm from these spectral lines. Apparatus Calibration ● We observed spectral lines of Hg to determine diffraction width with known wavelength of 546.074 nm. ● Determined diffraction slit width d of 3.276 +/- .005 um ● This value of slit width was determined from the diffracted angle theta which could only be determined within about 5 arc-minutes. ● Width d was determined from the slope of the next graph which has the relation d=(1/a) in this case, a is m_2=.00030416 => d=3276 nm. Hg Calibration Results ● We determined diffraction grating width d=3276 nm. ● For each data set, the value of the angles between the +/- n-values differed at most by about 0.4° but usually around 0.1° ● With d, we calculated wavelength of the alpha line to be 654.0 +/- 0.8 nm where the accepted value is 656.3 nm. Chi2- 18.4, Chi2/dof- 3.07, p-value of .006 ● Determined wavelength of Beta line to be 484.4+/- 0.8 nm. Accepted value is 486.1 nm Chi2- 4.04, Chi2/dof- .673, p-value of .67 ● Determined wavelength of Gamma line to be 433.4+/- 0.9 nm. Accepted value is 434.1 nm Chi2- 5.68, Chi2/dof- .947, p-value of .43 ● From these values of wavelengths, we plotted and found the value of Rm to be (1.097+/- 0.003) *10^7 (1/m). Accepted value: 1.0967* 10^7 (1/m). Chi2-1.60, Chi2/dof- 0.80. for 2 dof, p-value was .45 [3] Alpha Beta Gamma Rm Discussion ● We determined a good value for Rm that was only 0.02% off, achieving the 0.05% goal. ● Took a look at the values for the wavelengths for alpha, beta, and gamma and noticed a trend that they were all lower than the accepted value by about 2nm ● We suspected some sort of systematic error for this discrepancy; most likely to be the original calibration with Hg. ● To investigate the discrepancy, we considered altering the number of n-values to include in the fit for Hg. Unfortunately, this brought Rm down further. Conclusion ● We may have had a bit of error in original calibration of Hg. ● Given percent probability of 45 for Rm, it's a good model and the data supports the linear fit ● We calculated Rm of 1.097+/-0.003*10^7 (1/m). which is close to the accepted value of 1.0967*10^7 (1/m). References [1] Bohr, N. (1985). “Rydberg’s discovery of the spectral laws”. In Kalckar, J.. Collected works. 10. Amsterdam: North-Holland Publ. Cy.. pp.373/200/223379. [2] Mohr, P. J.; taylor, B. N.; Newell, D. B. (2008). “CODATA recommended values of the fundamental physical constants: 2006”. Reviews of Modern Physics 80: 633/200/223730. doi:10.1103/RevModPhys.80.633. [3] J.R. Taylor, An Introduction to Error Analysis, 2nd Ed. University Science Books, Suasalito CA (1997). .

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    14 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us