Effect of in-situ SiNx grown with different carrier gas on structural and electrical properties of GaN-based MISHEMTs

Author:

Zhang Haochen12ORCID,Chen Yao2,Sun Yue1ORCID,Yang Lei1ORCID,Hu Kunpeng1ORCID,Huang Zhe1ORCID,Liang Kun1,Xing Zhanyong1ORCID,Wang Hu1ORCID,Zhang Mingshuo1ORCID,Guo Shiping2ORCID,Sun Haiding1ORCID

Affiliation:

1. School of Microelectronics, University of Science and Technology of China 1 , Hefei, Anhui 230026, People's Republic of China

2. Advanced Micro-Fabrication Equipment Inc. 2 , 188 Taihua Road, Shanghai 201201, People's Republic of China

Abstract

In this work, the effect of in situ SiNx grown with different carrier gas on the structural and electrical properties of the SiNx/AlGaN/GaN MIS-HEMTs is studied. It was found that the growth rate of SiNx grown with N2 as carrier gas (N2-SiNx) is more sensitive to different growth conditions, while the growth rate of SiNx grown with H2 as carrier gas (H2-SiNx) is very stable due to the inhibiting effects of H2 carrier gas on the SiH4–NH3 forward reactions. More importantly, a continuous and smooth SiNx growth at the initial stage can be realized with H2 carrier gas due to its faster surface migration, leading to a decent surface morphology and sharp interface of H2-SiNx. As a result, the SiNx passivated device with H2 as carrier gas shows improved performance compared to that with N2 as carrier gas, featuring ultra-low interface-state density of 2.8 × 1010 cm−2 eV−1, improved on- and off-state current, reduced threshold voltage shift, and mitigated current collapse, especially after long-term electrical stress. These results not only elaborate on the growth mechanisms of in situ SiNx with different carrier gases but also highlight the advances of H2 as carrier gas for in situ SiNx growth, providing an effective strategy to tailor the passivation schemes for GaN-based devices.

Funder

National Natural Science Foundation of China

Students' Innovation and Entrepreneurship Foundation of USTC

Publisher

AIP Publishing

Subject

Physics and Astronomy (miscellaneous)

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