Physics
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007njph....9..391m&link_type=abstract
New Journal of Physics, Volume 9, Issue 10, pp. 391 (2007).
Physics
17
Scientific paper
Due to their extreme surface sensitivity, the Shockley states of (111) noble metal surfaces can be used to study the modifications of atomic and electronic properties of epitaxial ultra thin films and self-organized nanostructures. In metallic interfaces, the different parameters of the Shockley surface state bands (energy, effective mass and eventually spin orbit splitting) have been shown to be strongly thickness dependent. It was also possible by scanning tunneling spectroscopy to evidence a spectroscopic signature of buried interfaces. Moreover, superperiodic surface structures like the reconstruction on Au(111) vicinal surfaces or self-organized nanodots, lead to spectacular spectroscopic effects. In the vicinal Au(23 23 21) surface, the opening of tiny energy gaps associated with the reconstruction potential of such surfaces has been evidenced. Peculiar growth on these Au vicinal surfaces allows us to obtain high quality self-assembled metallic nanostructures which exhibit homogeneous electronic properties on a large spatial scale resulting from a coherent scattering of the Shockley states.
Bendounan Azzedine
Cercellier Hervé
Didiot Clement
Fagot-Revurat Y.
Kierren B.
No associations
LandOfFree
ARPES and STS investigation of Shockley states in thin metallic films and periodic nanostructures does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with ARPES and STS investigation of Shockley states in thin metallic films and periodic nanostructures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ARPES and STS investigation of Shockley states in thin metallic films and periodic nanostructures will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1878030