Phys. Rev. B 76, 115426 (2007) [6 pages]
Ab initio modeling of CaTiO3 (110) polar surfaces
Abstract
References (31)
Citing Articles
Jian-Min Zhang, 1 Jie Cui, 1 Ke-Wei Xu, 2 Vincent Ji, 3 and Zhen-Yong Man41College of Physics and Information Technology, Shaanxi Normal University, Xi'an 710062, Shaanxi, People's Republic of China
2State Key Laboratory for Mechanical Behavior of Materials, Xi'an Jiaotong University, Xi'an 710049, Shaanxi, People's Republic of China
3ICMMO/LEMHE UMR CNRS 8182, Université Paris-Sud 11, 91405 Orsay Cedex, France
4State Key Laboratory of High Performance Ceramics and Superfine Microstructures, Shanghai Institute of Ceramics, Chinese Academy of Sciences, Shanghai 200050, People's Republic of China
Received 15 April 2007; revised 21 June 2007; published 20 September 2007
The TiO, Ca, asymmetric A-type O-terminated and symmetric B-type O-terminated surfaces have been constructed for CaTiO3 (110) surface. The cleavage and surface energies, surface grand potential, surface relaxation, and surface electronic structure have been calculated for these polar terminations by using ab initio plane waves ultrasoft pseudopotential method based on generalized gradient approximation. The results show that the favorable CaTiO3 (110) and (001) surfaces are CaO-terminated (001) surface, A-type O-terminated (110) surface, and TiO2-terminated (001) surface successively, in view of the surface energy minimization. The Ca termination is stable in O- and Ca-rich environments, however, its complementary TiO termination is stable in O- and Ca-poor conditions. The A-type O termination shows a stability domain in moderate O and Ca environments. In the range of accessible values of µO, only Ca and A-type O-terminated surfaces are likely to be observed. Moreover, a large surface rumpling s of 12.10% a is found for the TiO-terminated surface due to inward movement of Ti ion and outward movement of O ion. The surface band gaps for the relaxed TiO and A-type O terminations are larger than the bulk band gap; however, the values for Ca and B-type O terminations are smaller.
©2007 The American Physical Society
REFERENCES (31)
For access to fully linked references, you need to log in.
For access to fully linked references, you need to Log in.
- I. A. Kornev, L. Bellaiche, P. Bouvier, P.-E. Janolin, B. Dkhil, and J. Kreisel, Phys. Rev. Lett. 95, 196804 (2005).
- R. E. Cohen and H. Krakauer, Phys. Rev. B 42, 6416 (1990).
- O. Auciello, J. F. Scott, and R. Ramesh, Phys. Today 51 (7), 22 (1998).
- A. Asthagiri and D. S. Sholl, J. Chem. Phys. 116, 9914 (2002).
- E. Heifets, W. A. Goddard III, E. A. Kotomin, R. I. Eglitis, and G. Borstel, Phys. Rev. B 69, 035408 (2004).
- E. Heifets, R. I. Eglitis, E. A. Kotomin, J. Maier, and G. Borstel, Phys. Rev. B 64, 235417 (2001).
- C. Cheng, K. Kunc, and M. H. Lee, Phys. Rev. B 62, 10409 (2000).
- L. Fu, E. Yaschenko, L. Resca, and R. Resta, Phys. Rev. B 60, 2697 (1999).
- Y. X. Wang, M. Arai, T. Sasaki, and C. L. Wang, Phys. Rev. B 73, 035411 (2006).
- J. P. Perdew, K. Burke, and M. Ernzerhof, Phys. Rev. Lett. 77, 3865 (1996).
- X. G. Wang, A. Chaka, and M. Scheffler, Phys. Rev. Lett. 84, 3650 (2000).
CITING ARTICLES
For access to citing articles, you need to log in.
For access to citing articles, you need to Log in.
|
A new free weekly publication from APS
|