In situ insight into temperature-dependent microstructure evolution of carbon doped phase change materials

Author:

Qi Ruijuan123ORCID,Zhang Jinzhong2ORCID,Sui Fengrui2ORCID,Song Sannian1,Li Xi1,Song Zhitang1

Affiliation:

1. National Key Laboratory of Materials for Integrated Circuits, Shanghai Institute of Microsystem and Information Technology, Chinese Academy of Sciences 1 , Shanghai 200050, China

2. Key Laboratory of Polar Materials and Devices (MOE) and Department of Electronics Sciences, School of Physics and Electronic Science, East China Normal University 2 , Shanghai 200062, China

3. Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences 3 , Beijing 100049, China

Abstract

Carbon-doped Ge2Sb2Te5 (CGST) is a potential candidate in phase change random access memory (PCRAM) with superb thermal stability and ultrahigh cycle endurance. Direct observation of the microstructure evolution of CGST is desirable to uncover the phase transformation mechanism on the relationship of nucleation/crystalline behaviors of the crystalline phase at elevated temperatures and the pristine amorphous phase at room temperature. Here, we investigate the structural evolution of CGST using combined in situ techniques. Our in situ x-ray diffraction and ellipsometry results demonstrate that CGST exhibits a much higher phase transition temperature than undoped one. Temperature-dependent in situ transmission electron microscopy observations further reveal that carbon doping plays a critical role in tailoring the properties of GST by tuning the stochasticity of nucleation/crystallization, stabilizing amorphous and crystalline GST via isolating and refining the grain size at room temperature and elevated temperature. Our work provides detailed information for understanding the microscopic origin of crystallization kinetics of carbon-doped phase change materials toward high-performance PCRAM.

Funder

National Natural Science Foundation of China

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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