Abstract
The photoelectron spectrum of the (0001) surface of single-crystalline yttrium bulk samples is rich in structure from the surface state near the Fermi energy to a series of spectral features between 2 and binding energies. Many of them appear on other rare-earth surfaces, e.g., Gd, Ho, Pr, and Er, as well. However, it is an unsolved puzzle that none of the observed features, except for the surface state at the Fermi energy, can be found in data from clean rare-earth thin films. While some of the additional features in the results from single-crystal surfaces were already attributed to impurities such as chlorine, oxygen, and hydrogen, the peak at remains a source of speculation for more than now. In this Rapid Communication, we provide a consistent picture of the surface electronic structure of Y(0001), which explains all differences between the data obtained from single-crystal surfaces and thin films. We show that the peak at , which was previously assigned to a well-ordered clean surface, is in fact due to the formation of ordered carbon compounds originating from impurities in the bulk material.
- Received 23 February 2008
DOI:https://doi.org/10.1103/PhysRevB.77.161401
©2008 American Physical Society