CONDENSED MATTER: ELECTRONIC STRUCTURE, ELECTRICAL, MAGNETIC, AND OPTICAL PROPERTIES |
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Anomalous Pressure Behavior of N-Cluster Emissions in GaAs0.973Sb0.022N0.005 |
WANG Wen-Jie1, DENG Jia-Jun1, FU Xing-Qiu2, HU Bing1, DING Kun1 |
1Mathematics and Physics Department, North China Electric Power University, Beijing 1022062State Key Laboratory for Superlattices and Microstructures,Institute of Semiconductor, Chinese Academy of Sciences, Beijing 100083 |
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Cite this article: |
WANG Wen-Jie, DENG Jia-Jun, FU Xing-Qiu et al 2009 Chin. Phys. Lett. 26 127101 |
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Abstract Photoluminescence of GaAs0.973Sb0.022N0.005 is investigated at different temperatures and pressures. Both the alloy band edge and the N-related emissions, which show different temperature and pressure dependences, are observed. The pressure coefficients obtained in the pressure range 0-1.4GPa for the band edge and N-related emissions are 67 and 45meV/GPa, respectively. The N-related emissions shift to a higher energy in the lower pressure range and then begin to redshift at about 8.5GPa. This redshift is possibly caused by the increase of the X-valley component in the N-related states with increasing pressure.
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Keywords:
71.55.Eq
78.55.Cr
78.20.Bh
61.43.-j
68.37.Uv
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Received: 03 July 2009
Published: 27 November 2009
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PACS: |
71.55.Eq
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(III-V semiconductors)
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78.55.Cr
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(III-V semiconductors)
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78.20.Bh
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(Theory, models, and numerical simulation)
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61.43.-j
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(Disordered solids)
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68.37.Uv
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(Near-field scanning microscopy and spectroscopy)
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[1] Weyers M, Sato M and Ando H 1992 Jpn. J. Appl. Phys.I$\!$I 31 L853 [2]Wei S H and Zunger A 1996 Phys. Rev. Lett. 76664 [3]Perkins J D, Mascarenhas A, Zhang Y, Geisz J F, Friedman DJ, Olson J M and Kurtz S R 1999 Phys. Rev. Lett. 82 3312 [4]Zhang Y, Mascarenhas A, Xin H P and Tu C W 2000 Phys.Rev. B 61 7479 [5] Ma B S, Su F H, Ding K, Li G H, Zhang Y, Mascarenhas A,Xin H P and Tu C W 2005 Phys. Rev. B 71 045213 [6]Berti M, Bisognin G, Salvador D D, Napolitani E andVangelista S 2007 Phys. Rev. B 76 205323 [7] Bosa I, McPeake D and Fahy S 2008 Phys. Rev. B 78 245206 [8]Jin Z, Su Y B, Cheng W, Liu X Y, Xu A H and Qi M 2008 Chin. Phys. Lett. 25 3075 [9]Shan W, Walukiewicz W, Ager J W, Haller E E, Geisz J F,Friedman D J, Olson J M and Kurtz S R 1999 Phys. Rev. Lett. 82 1221 [10] Kent P R C and Zunger A 2001 Phys. Rev. B 64115208 [11] Varshni Y P 1967 Physica 34 149 [12] Liang X G, Jiang D S, Bian L F, Zhong P, Li L H and Wu RH 2002 Chin. Phys. Lett. 19 1203 [13] Bian L F, Jiang D S, Liang X G and Lu S L 2004 Chin.Phys. Lett. 21 548 [14] Kudrawiec R, Sek G, Misiewicz J, Li L H and Harmand J C2004 Eur. Phys. J. Appl. Phys. 27 313 [15] Kudrawiec R, Motyka M, Misiewicz J, Yuen H B, Bank S R,Wistey M A, Bae H P and Harris J S 2005 J. Appl. Phys. 98 063527 [16] Tsang M S, Wang J N, Ge W K, Li G H, Fang Z L, Chen Y,Han H X, Li L H and Pan Z 2001 Appl. Phys. Lett. 78 3595 [17] Li G H, Goni A R, Abraham C, Syassen K, Santos P V,Cantarero A, Brabdt O and Ploog K 1994 Phys. Rev. B 501575 [18] Weinstein B A, Stambach S R, Ritter T M, Maclean J O andWallis D J 2003 Phys. Rev. B 68 035336 [19] Eremets M I, Krasnovskij O A, Struzhkin V V and ShirokovA M 1989 Semicond. Sci. Technol. 4 267 [20] Mattila T, Wei S H and Zunger A 1999 Phys. Rev. B 60 R11245 |
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