2008Acta Physica SinicaOpen access

Influence of defects on the melting and premelting of carbon nanotubes

Kaiwang Zhang, Zhong Jian-Xin, 湘潭大学材料与光电物理学院,湘潭 411105

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Abstract

We report results of molecular dynamics simulations of melting and premelting of single-walled carbon nanotubes (SWNTs) with different types of point defects, namely, the Stone-Wales defect, vacancy defect, and impurity defect. Using the Lindemann parameter, we found that the melting temperature of perfect SWNTs is around 4800K. We further show that premelting occurs in the regions close to the defects with premelting temperatures of 2600K for the Stone-Wales defect and3200K for the cavity defect. The SWNTs with Si impurity defects are thermally stable up to 3800K.

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What this paper is about

We report results of molecular dynamics simulations of melting and premelting of single-walled carbon nanotubes (SWNTs) with different types of point defects, namely, the Stone-Wales defect, vacancy defect, and impurity defect. Using the Lindemann parameter, we found that the melting temperature of perfect SWNTs is around 4800K. We further show that premelting occurs in the regions close to the defects with premelting temperatures of 2600K for the Stone-Wales defect and3200K for the cavity defect. The SWNTs with Si impurity defects are thermally stable up to 3800K.

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Available abstract

We report results of molecular dynamics simulations of melting and premelting of single-walled carbon nanotubes (SWNTs) with different types of point defects, namely, the Stone-Wales defect, vacancy defect, and impurity defect. Using the Lindemann parameter, we found that the melting temperature of perfect SWNTs is around 4800K. We further show that premelting occurs in the regions close to the defects with premelting temperatures of 2600K for the Stone-Wales defect and3200K for the cavity defect. The SWNTs with Si impurity defects are thermally stable up to 3800K.

Key concepts: Premelting, Carbon nanotube, Materials science, Melting point, Impurity, Vacancy defect, Melting temperature, Molecular dynamics

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