structural phase transition on Si(111)-Ã3xÃ3-Ag surface studied by x-ray diffraction

 

T. Takahashi,a H. Tajiri,a K. Sumitani,a S. Nakatani,a A. Nojima,a

K. Akimoto,b H. Sugiyama,c X. Zhang,a and H. Kawata c

 

aInstitute for Solid State Physics, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa-shi, Chiba 277-8581, Japan; bDepartment of Quantum Engineering, Nagoya University, Furo-cho, Chikusa, Nagoya 464-8603, Japan; cPhoton Factory, High Energy Accelerator Research Organization, Tsukuba 305-0801, Japan (ttaka@issp.u-tokyo.ac.jp).

 

 

A Si(111)-Ã3xÃ3-Ag (for short Ã3-Ag) surface structure at room temperature is generally accepted as a honeycomb chained triangle (HCT) structure with a number of experimental and theoretical results[1]. However, recently, Aizawa et al.[2] reported that the most stable structure of the surface is not the HCT structure but an in-equivalent triangle (IET) structure by means of first principles calculations and scanning tunneling microscopy at low temperatures. Structural reinvestigations on the Ã3-Ag surface by x-ray diffraction have revealed that the Ã3-Ag surface transforms from the HCT structure of high temperature phase into the IET structure of low temperature one at 150K[3]. In addition, an abrupt change in x-ray scattering intensities in the vicinity of the transition temperature has implied the displacive phase transition[3]. However, properties of the phase transition on the surface are still unclear in detail.

In this work, we further studied the Ã3-Ag surface structure, especially around the transition temperature of 150K by x-ray diffraction. We discuss critical exponents and an order parameter in this system based on anharmonic thermal vibration analyses.

 

References

1           Takahashi, T., Nakatani, S. (1993) Surf. Sci. 282, 17, and references there in.

2           Aizawa, H., Tsukada, M., Sato, N., Hasegawa, S. (1999) Surf. Sci. Lett. 429, L509.

3           Tajiri, H., Sumitani, K., Nakatani, S., Nojima, A., Takahashi, T., Akimoto, K., Sugiyama, H., Zhang, X., Kawata, H. (2002) submitted to Phys. Rev. B.