Hostname: page-component-7479d7b7d-m9pkr Total loading time: 0 Render date: 2024-07-12T05:34:02.028Z Has data issue: false hasContentIssue false

The Nature of Native and Light Induced Defect States in i-layers of High Quality a-Si:H Solar Cells Derived from Dark Forward-Bias Current-Voltage Characteristics

Published online by Cambridge University Press:  01 February 2011

J. Deng
Affiliation:
Center for Thin Film Devices, Pennsylvania State University, University Park, PA 16802
M. L. Albert
Affiliation:
Center for Thin Film Devices, Pennsylvania State University, University Park, PA 16802
J. M. Pearce
Affiliation:
Physics Department, Clarion University of Pennsylvania, Clarion, PA 16214
R. W. Collins
Affiliation:
Department of Physics and Astronomy, University of Toledo, Toledo, OH 43606
C. R. Wronski
Affiliation:
Center for Thin Film Devices, Pennsylvania State University, University Park, PA 16802
Get access

Abstract

Results are presented on the defect state distributions in intrinsic a-Si:H layers with and without hydrogen dilution in p-i-n solar cells obtained directly from the analysis of dark forwardbias current-voltage (JD-V) characteristics. It is shown that there are distinct differences in the distributions of both native and light induced defect states between the two types of i-layers. Computer simulations using these distributions are presented which show excellent agreement with the experimental results not only for the JD-V but more importantly for the bias dependent differential diode quality factor n(V) characteristics. Results are also presented on the nature of the gap states and their evolution with light induced degradation as well as their effects on the performance and stability of high quality a-Si:H solar cells.

Type
Research Article
Copyright
Copyright © Materials Research Society 2005

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

[1] Fritzsche, H., Annu. Rev. Mater. Res. 31, 47 (2001)10.1146/annurev.matsci.31.1.47Google Scholar
[2] Wronski, C. R., Pearce, J. M., Koval, R. J., Niu, X., Ferlauto, A. S., Koh, J., and Collins, R.W., Mater. Res. Soc. Proc. 715, 459 (2002)10.1557/PROC-715-A13.4Google Scholar
[3] Deng, J., Pearce, J. M., Koval, R. J., Vlahos, V., Collins, R.W., and Wronski, C. R., Appl. Phys. Lett. 82, 3023 (2003)10.1063/1.1571985Google Scholar
[4] Deng, J., Pearce, J. M., Vlahos, V., Collins, R. W., and Wronski, C. R., Mater. Res. Soc. Proc. 808, A8.8 (2004)10.1557/PROC-808-A8.8Google Scholar
[5] Berkel, C. van, Powell, M. J., Franklin, A. R., and French, I. D., J. Appl. Phys. 73, 5264 (1993).10.1063/1.353755Google Scholar
[6] Niu, X., private communications.Google Scholar
[7] Koval, R. J., Koh, J., Lu, Z., Jiao, L., Collins, R. W., and Wronski, C. R., Appl. Phys. Lett. 75, 1553 (1999)10.1063/1.124752Google Scholar
[8] F. A, Rubinelli, Hou, J. Y., Fonash, S., Wronski, C. R., Bennet, M., and Wiedeman, S., Conf. Record of the 22nd IEEE Photovoltaic Specialists Conference, vol. 2, 1992, p.1405.Google Scholar