Characterization of Residual Strain in Si Ingots Grown by the Seed-Cast Method

Article Preview

Abstract:

The residual strain distribution in cast-grown mono-like Si ingots is analyzed. The effect of the crucible during solidification and the influence of different cooling rates is described. To clarify in which process steps residual strain accumulates, several Si ingots were grown in a laboratory scale furnace (100mm) using different cooling conditions after completion of the solidification. For the cooling, two different cooling rates were distinguished: fast cooling (12deg/min) and slow cooling (5deg/min). It was found that changes in cooling gradients greatly influence the amount of residual strain. The results show that slow cooling in any temperature range leads to strain reduction. The greatest reduction could be found when the temperature gradient was changed to slow cooling in the high temperature region.

You might also be interested in these eBooks

Info:

Periodical:

Solid State Phenomena (Volumes 205-206)

Pages:

94-99

Citation:

Online since:

October 2013

Export:

Price:

Permissions CCC:

Permissions PLS:

Сopyright:

© 2014 Trans Tech Publications Ltd. All Rights Reserved

Share:

Citation:

[1] A. Müller, M. Ghosh, R. Sonnenschein and P. Woditsch: Materials Science and Engineering B 134 (2006), p.257.

Google Scholar

[2] L. Arnberg, M. Di Sabatino and E. J. Øvrelid: Journal of Crystal Growth 360 (2012), p.56.

Google Scholar

[3] N. Stoddard, B. Wu, I. Witting, M.C. Wagener, Y. Park, G.A. Rozgonyi and R. Clark: Solid State Phenomena Vol. 131-133 (2008), p.1.

Google Scholar

[4] X. Chen, S. Nakano and K. Kakimoto: Journal of Crystal Growth 312 (2010), p.3261.

Google Scholar

[5] B. Gao, S. Nakano, H. Harada, Y. Miyamura, T. Sekiguchi and K. Kakimoto: Journal of Crystal Growth 352 (2012), p.47.

Google Scholar

[6] V. A. Popovich, A. Yunus, M. Janssen, I. M. Richardson and I. J. Bennett: Solar Energy Materials and Solar Cells 95 (2011), p.97.

DOI: 10.1016/j.solmat.2010.04.038

Google Scholar

[7] X. F. Brun and S. N. Melkote: Solar Energy Materials and Solar Cells 93 (2009), p.1238.

Google Scholar

[8] K. Arafune, E. Ohishi, H. Sai, Y. Ohshita and M. Yamaguchi: Journal of Crystal Growth 308 (2007), p.5.

Google Scholar

[9] M. Yamada: Review of Scientific Instruments 64 (1993), p.1815.

Google Scholar

[10] M. Fukuzawa, M. Yamada, M. Rafiqul Islam, J. Chen and T. Sekiguchi: Journal of Electronic Materials 39 (2010), p.700.

Google Scholar

[11] K. Jiptner, M. Fukuzawa, Y. Miyamura, H. Harada and T. Sekiguchi: Japanese Journal of Applied Physics 52 (2013), p.065501.

DOI: 10.7567/jjap.52.065501

Google Scholar

[12] H. J. Möller, T. Kaden, S. Scholz and S. Würzner: Applied Physics A 96 (2009), p.207.

Google Scholar

[13] H. Alexander and P. Haasen: Solid State Physics 22 (1968), p.27.

Google Scholar

[14] K. Jiptner, H. Harada, Y. Miyamura, M. Fukuzawa and T. Sekiguchi: Materials Science Forum 725 (2012), p.247.

Google Scholar