First Principles Calculations of Advanced Nitrides, Oxides and Alloys

Article Preview

Abstract:

The phase stability of silicon nitride is examined using a series of first principles phonon calculations. -phase shows slightly higher free energy than  in the temperature range from 0 to 2000K. The difference between  and is only 0.02 eV/Si3N4 or 2 kJ/mol at 300 K. The result is consistent with the experimental report by high-temperature oxide-melt-drop solution-calorimetry. Similar calculations are made for ZrO2, Ga2O3, BN and some perovskites. Using cluster expansion technique combined with a large set of first principles calculations, the cation disordering of II-III spinel oxides and the phase diagram of diamond vs. c-BN are theoretically investigated. Theoretical results on the atomic structures of  and  sialons are also shown.

You might also be interested in these eBooks

Info:

Periodical:

Pages:

73-76

Citation:

Online since:

December 2008

Export:

Price:

Permissions CCC:

Permissions PLS:

Сopyright:

© 2009 Trans Tech Publications Ltd. All Rights Reserved

Share:

Citation:

[1] A. Kuwabara and I. Tanaka: submitted to Phys. Rev. B (2008).

Google Scholar

[2] A. Zerr, R. Riedel, T. Sekine, J. E. Lowther, W. Y. Ching, and I. Tanaka, Adv. Mater. 18, (2006) 2933.

DOI: 10.1002/adma.200501872

Google Scholar

[3] J-J. Liang, L. Topor, A. Navrotsky, and M. Mitomo, J. Mater. Res., 14, (1999) (1960).

Google Scholar

[4] Y. Zhang, A. Navrotsky and T. Sekine, J. Mater. Res., 21 (2006) 41.

Google Scholar

[5] A. Kuwabara, T. Tohei, T. Yamamoto, and I. Tanaka, Phys. Rev. B 71, (2005) 064301.

Google Scholar

[6] S. Yoshioka, H. Hayashi, A. Kuwabara, F. Oba, K. Matsunaga, and I. Tanaka, J. Phys: Condens. Matter 19, (2007) 346211.

DOI: 10.1088/0953-8984/19/34/346211

Google Scholar

[7] T. Tohei, A. Kuwabara, F. Oba, and I. Tanaka, Phys. Rev. B 73, (2006) 064304.

Google Scholar

[8] T. Tohei, A. Kuwabara, T. Yamamoto, F. Oba, and I. Tanaka, Phys. Rev. Lett. 94, (2005) 035502.

Google Scholar

[9] A. Seko, F. Oba, A. Kuwabara, and I. Tanaka, Phys. Rev. B 72, (2005) 024107.

Google Scholar

[10] A. Seko, K. Yuge, F. Oba, A. Kuwabara, and I. Tanaka, Phys. Rev. B 73, (2006) 184117.

Google Scholar

[11] A. Seko, K. Yuge, F. Oba, A. Kuwabara, I. Tanaka, and T. Yamamoto, Phys. Rev. B 73, (2006) 094116.

Google Scholar

[12] A. Seko, A. Togo, F. Oba and I. Tanaka. Phys. Rev. Lett. in press (2008).

Google Scholar

[13] K. Yuge, A. Seko, Y. Koyama, F. Oba, and I. Tanaka, submitted to Phys. Rev. B (2008).

Google Scholar

[14] K. Tatsumi, I. Tanaka, H. Adachi, and M. Yoshiya, Phys. Rev. B 66, (2002) 165210.

Google Scholar

[15] K. Tatsumi, T. Mizoguchi, S. Yoshioka, T. Yamamoto, T. Suga, T. Sekine, and I. Tanaka, Phys. Rev. B 71, (2005) 033202.

Google Scholar