Ultraviolet photoelectron spectroscopy
Ultraviolet photoelectron spectroscopy (UPS) refers to the measurement of kinetic energy spectra of photoelectrons emitted by molecules which have absorbed ultraviolet photons, in order to determine molecular orbital energies in the valence region.
Basic theory
If Albert Einstein's photoelectric law is applied to a free molecule, the kinetic energy () of an emitted photoelectron is given by
- ,
where h is
History
Before 1960, virtually all measurements of photoelectron kinetic energies were for electrons emitted from metals and other solid surfaces. In about 1956, Kai Siegbahn developed X-ray photoelectron spectroscopy (XPS) for surface chemical analysis. This method uses x-ray sources to study energy levels of atomic core electrons, and at the time had an energy resolution of about 1 eV (electronvolt).[1]
![UPS gas, JM Sotiropoulos, IPREM, PAU, CNRS](http://upload.wikimedia.org/wikipedia/commons/thumb/f/fa/Image_UPS_gas.jpg/220px-Image_UPS_gas.jpg)
The ultraviolet photoelectron spectroscopy (UPS) was pioneered by Feodor I. Vilesov, a physicist at St. Petersburg (Leningrad) State University in Russia (USSR) in 1961 to study the photoelectron spectra of free molecules in the gas phase.[2][3] The early experiments used monochromatized radiation from a hydrogen discharge and a retarding potential analyzer to measure the photoelectron energies. The PES was further developed by
Application
The UPS measures experimental
The method was later extended to the study of solid surfaces where it is usually described as photoemission spectroscopy (PES). It is particularly sensitive to the surface region (to 10 nm depth), due to the short range of the emitted photoelectrons (compared to X-rays). It is therefore used to study adsorbed species and their binding to the surface, as well as their orientation on the surface.[8]
A useful result from characterization of solids by UPS is the determination of the work function of the material. An example of this determination is given by Park et al.[9] Briefly, the full width of the photoelectron spectrum (from the highest kinetic energy/lowest binding energy point to the low kinetic energy cutoff) is measured and subtracted from the photon energy of the exciting radiation, and the difference is the work function. Often, the sample is electrically biased negative to separate the low energy cutoff from the spectrometer response.
Gas discharge lines
Gas | Emission line | Energy (eV) | Wavelength (nm) | Relative Intensity (%) |
---|---|---|---|---|
H | Lyman α | 10.20 | 121.57 | 100 |
Lyman β | 12.09 | 102.57 | 10 | |
He | 1 α | 21.22 | 58.43 | 100 |
1 β | 23.09 | 53.70 | approx 1.5 | |
1 γ | 23.74 | 52.22 | 0.5 | |
2 α | 40.81 | 30.38 | 100 | |
2 β | 48.37 | 25.63 | <10 | |
2 γ | 51.02 | 24.30 | negligible | |
Ne | 1 α | 16.67 | 74.37 | 15 |
1 α | 16.85 | 73.62 | 100 | |
1 β | 19.69 | 62.97 | < 1 | |
1 β | 19.78 | 62.68 | < 1 | |
2 α | 26.81 | 46.24 | 100 | |
2 α | 26.91 | 46.07 | 100 | |
2 β | 27.69 | 44.79 | 20 | |
2 β | 27.76 | 44.66 | 20 | |
2 β | 27.78 | 44.63 | 20 | |
2 β | 27.86 | 44.51 | 20 | |
2 γ | 30.45 | 40.71 | 20 | |
2 γ | 30.55 | 40.58 | 20 | |
Ar | 1 | 11.62 | 106.70 | 100 |
1 | 11.83 | 104.80 | 50 | |
2 | 13.30 | 93.22 | 30 | |
2 | 13.48 | 91.84 | 15 |
Outlook
UPS has seen a considerable revival with the increasing availability of synchrotron light sources which provide a wide range of monochromatic photon energies.
See also
- Angle resolved photoemission spectroscopy(ARPES)
- Photoelectron photoion coincidence spectroscopy (PEPICO)
- Time-resolved two-photon photoelectron spectroscopy
References
- ISBN 0-306-33901-3
- Bibcode:1961SPhD....6..490V.
- ISBN 9780120038107.
- ISBN 0-471-70285-4
- OCLC 108745.
- OCLC 539873.
- ^ mdomingo#utilisateurs (2020-09-10). "Jean-Marc Sotiropoulos". iprem.univ-pau.fr (in French). Retrieved 2021-05-17.
- ISBN 0-7167-3539-3
- ISSN 0003-6951.