Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-28T08:05:44.958Z Has data issue: false hasContentIssue false

Fabrication, Characterization and Optical Studies of Cu(In1-xGax)3Se5 Bulk Compounds

Published online by Cambridge University Press:  31 January 2011

Dayane Habib
Affiliation:
[email protected], Lebanese University, Physics, Jdeidet, Lebanon
Georges El Hajj Moussa
Affiliation:
[email protected], Lebanese University, Physics, Jdeidet, Lebanon
Roy Al Asmar
Affiliation:
[email protected], Montpellier University 2, Centre Electronique et Micro-optoélectronique de Montpellier, Montpellier, France
Michael Ibrahim
Affiliation:
[email protected], Lebanese University, Physics, Jdeidet, Lebanon
Mario Remond El Tahchi
Affiliation:
[email protected], Lebanese University, Physics, Jdeidet, Lebanon
Claude Llinares
Affiliation:
[email protected], Montpellier University 2, Centre Electronique et Micro-optoélectronique de Montpellier, Montpellier, France
Get access

Abstract

In this paper we present the structural and optical properties of Cu(In1-xGax)3Se5 ternary and quaternary compounds crystals fabricated by horizontal Bridgman technique. The Cu(In1-xGax)3Se5 materials were characterized by Energy Dispersive Spectrometry (EDS), hot point probe method, X-ray diffraction, Photoluminescence (PL), and Optical response (Photoconductivity). The Cu(In1-xGax)3Se5 have an Ordered Vacancy Chalcopyrite-type structure with lattice constants varying as a function of the x composition. A good stœchiometry given by the EDS characterization method is well observed in our samples and its magnitude deviation Δy is slight; so, our samples present a nearly perfect stœchiometry (Δy = 0) [1]. X-Ray diffraction patterns show the presence of many preferential orientations according to the planes (112), (220) and (312) of all the samples [2]. Also, it shows a linear shifting of peaks towards the higher magnitudes of 2θ when the x composition increases. These compounds can be of stanite structure [3] or an Ordered Vacancy Chalcopyrite structure (OVC) [4] or Ordered Defect Chalcopyrite Structure (ODC). We observe a large shift of the main PL and optical response emission peak versus x composition. The band gap energy of Cu(In1-xGax)3Se5 compounds is found to vary from 1.23 eV to 1.85 eV as a function of x. [1] Migual A. Contreras, Holm Wiesner, Rick Mtson, John Tuttle, Kanna Ramanathan, Rommel Noufi, Mat. Res. Soc. Symp. Proc. Vol. 426 (1996) 243-254. [2] Ariswan, G. El Haj Moussa, M. Abdelali, F. Guastavino, C. Llinares, Solid State Communications 124 (2002) 391-396. [3] M. Suzuki, T. Uenoyama, T. Wada, T. Hanada, Y. Nakamura, Jpn. J. Appl. Phys. 36 L1139 (1997). [4] Kristjan Laes, Sergei Bereznev, A. Tverjanovich, E.N. Borisov, Tiit Varema, Olga Volobujeva , Andres Öpik. Thin Solid Films 517 (2009) 2286–2290.

Type
Research Article
Copyright
Copyright © Materials Research Society 2010

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] Laes, Kristjan, Bereznev, Sergei, Tverjanovich, A. Borisov, E.N. Varema, Tiit, Volobujeva, Olga, Öpik, Andres. Thin Solid Films 517, 2286 (2009).10.1016/j.tsf.2008.10.106Google Scholar
[2] Schmid, D. Ruckh, M. Grunwald, F. and Schock, H.W. J. Appl. Phys. 73, 2902 (1993).Google Scholar
[3] Contreras, Migual A. Wiesner, Holm, Mtson, Rick, Tuttle, John, Ramanathan, Kanna, Noufi, Rommel, Mat. Res. Soc. Symp. Proc. 426, 243 (1996).Google Scholar
[4] Marin, G. Tauleigne, S. Wasim, S. M. Guervara, R. Degado, J. M. Rincon, C. Mora, A. E. perez, G. Sanchez, Mat. Res. Bulletin 33, (7), 1057 (1998).Google Scholar
[5] Negami, T. Kohara, N. Nikihiko, M. Wada, T. Jpn. J. Appl. Phys. 33, 1251 (1994).Google Scholar
[6] Suzuki, M. Uenoyama, T. Wada, T. Hanada, T. Nakamura, Y. Jpn. J. Appl. Phys. 36 L1139 (1997).Google Scholar
[7] Marin, G. Tauleigne, S. Guervara, R. Degado, J. M. Wasim, S. M. Bocaranda, P. perez, G. Sanchez, Diaz, J. the 11th Int. Conf. on Ternary and Multinary Compounds, ICTMC-11, Salford, 8-12 Sept 573 (1997).Google Scholar
[8] Negami, T. Kohara, N. Nikihiko, M. Wada, T. Hirao, T. J. Appl. Phys. Lett. 67 (6), 825 (1995).Google Scholar
[9] Malar, P. Kasiviswanathan, S. Solar Energy Materials & Solar Cells 88, 281 (2005).Google Scholar
[10] Zott, S. Leo, K. Ruckh, M. Schock, H. W. J. Appl. Phys. 82, 356, (1997).Google Scholar
[11] Zott, S. Leo, K. Ruckh, M. Schock, H. W. Cryst. Res. Technol. 31, 729 (1996).Google Scholar
[12] Orsal, G. Mailly, F. Romain, N. Artaud, M.C. Rushworth, S. Duchemin, S. Thin Solid Films 361-263, 135 (2000).Google Scholar
[13] , Ariswan, Moussa, G. El Haj, Abdelali, M. Guastavino, F. Llinares, C. Solid State Communications 124, 391 (2002).Google Scholar