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Spectroscopy of Hydrogenic Atoms Dennis V. Perepelitsa with Brian - PowerPoint PPT Presentation

Spectroscopy of Hydrogenic Atoms Dennis V. Perepelitsa with Brian J. Pepper MIT Department of Physics October 23rd, 2006 Introduction Theory Bohr Equation Balmer Series Rydberg Constant Mass Corrected Bohr Equation Hydrogen Isotope


  1. Spectroscopy of Hydrogenic Atoms Dennis V. Perepelitsa with Brian J. Pepper MIT Department of Physics October 23rd, 2006

  2. Introduction

  3. Theory Bohr Equation – Balmer Series Rydberg Constant Mass Corrected Bohr Equation Hydrogen Isotope Shift

  4. Experimental Setup Equipment Jobin Yvon 1250 M Monochromator Species Mercury (Hg), Sodium (Na), Hydrogen & Deuterium (H) Precision 1800 gvs./mm. - σ (repeatability) = .02A 3600 gvs./mm. - σ (repeatability) = .01A (but 3600 gvs./mm. scans only < 5000 A) Procedure * Wide scans at 1A * Calibration from Mercury using beam splitter * Lines focused and centered on entrance slit * Scans conducted with both gratings (Figure modified from “Optical Spectroscopy of Hydrogenic Atoms” Lab Guide.)

  5. Calibration and Fitting Voigt Profile (http://wikipedia.com.) Mercury Calibration Offset Hg: 3650 A, 4047A, 4358A, 5460A, 5770A

  6. Data (Hydrogen Balmer 4 -> 2 line, 3600 gvs./mm.)

  7. Hydrogen Balmer Series

  8. Calculation of the Rydberg Constant

  9. Hydrogen Isotope Shift

  10. Conclusions (How good are the results?) Hydrogen Balmer Series 1800 gvs./mm. data agrees with accepted values to within the error. 3600 gvs./mm. is less accurate, but more precise. ➔ Balmer series measured to nearest ~.08 A of accepted values. Rydberg Constant vs. (Accepted) ➔ Measured to within .01% of accepted value. ➔ But! - Error bars too small! Too many sig figs! Systematic error? Bad methodology? Imprecise equation? Hydrogen Isotope Shift vs. (Accepted) ➔ Measured to within 1% of accepted value.

  11. Acknowledgments Brian Pepper, an equal partner in collecting and analyzing the experimental data. Professor Isaac Chuang, who answered our questions about the experiment and pointed us in the right direction. Dr. Scott Sewell, and Scott Sanders, who helped us in our research and talked about spectral line width with us.

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