Surface band bending at n-type and p-type InN by Auger Electron Spectroscopy
|Volker Cimalla 2, Merten Niebelschütz 2, Gernot Ecke 2, Oliver Ambacher , Ruediger Goldhahn 3, Hai Lu 1, William J. Schaff 1|
1. Cornell University, 425 Philips Hall, Ithaca, NY 14853, United States
Thin films of InN show high n-type conductivity, for which the origin is not completely identified up to date. InN layers with carrier concentrations down to 1017 cm-3 have been prepared, however, no p-type InN could be demonstrated. Electron accumulation at the surface was verified on air , and on clean InN surfaces in ultrahigh vacuum . It was explained as an intrinsic property of InN layers ascribed to its band structure . In a previous work  we showed by Auger electron spectroscopy (AES) depth profiling and simultaneous conductivity measurements the correlation between the oxygen content and the electron accumulation. In this work we extend this study by analyzing the peak energy shift in AES on both undoped and Mg-doped InN. The position of the Auger peaks is sensitive to the position of the Fermi level . This capability was used to obtain information about the type of conductivity and the band bending. On all InN surfaces a strong increase of the resistivity within the first 5 nm confirms the existence of a highly conductive n-type surface layer. A strong Auger peak shift of about 2 eV was observed due to the formation of a wide band gap In2O3. After reaching equilibrium of the peak shift after the removal of about 50 nm a difference of 0.3 eV was observed between undoped and Mg-doped InN. Consequently, Mg-doped InN layers have indeed p-type conduction; however, the high n-type surface conductivity is overlaying it and the InN layer appears to be n-type.
 H. Lu, W.J. Schaff, et al, Appl. Phys. Lett. 82, 1736 (2003)
 I. Mahboob, T.D. Veal, et al, Phys. Rev. B 69, 201307 (R) (2004).
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 R. Kosiba, Thesis, Technical University Ilmenau, 2004
Presentation: oral at E-MRS Fall Meeting 2005, Symposium A, by Volker Cimalla
See On-line Journal of E-MRS Fall Meeting 2005
Submitted: 2005-05-20 13:06 Revised: 2009-06-07 00:44
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