Hydrostatic Pressure Effects on the Structural and Electronic Properties of Carbon Nanotubes
Rodrigo B. Capaz, Catalin D. Spataru, Paul Tangney, Marvin L. Cohen, and Steven G. Louie

TL;DR
This paper investigates how hydrostatic pressure affects the structure and electronic properties of single-wall carbon nanotubes using various theoretical methods, revealing a pressure-induced collapse transition and family-dependent electronic behavior.
Contribution
It combines multiple theoretical techniques to analyze pressure effects on SWNTs, providing a unified understanding of structural transitions and electronic property changes under pressure.
Findings
SWNTs remain cylindrical below a critical pressure P_c
Electronic energy gaps show family-dependent pressure coefficients
SWNTs undergo a symmetry-breaking collapse at P_c
Abstract
We study the structural and electronic properties of isolated single-wall carbon nanotubes (SWNTs) under hydrostatic pressure using a combination of theoretical techniques: Continuum elasticity models, classical molecular dynamics simulations, tight-binding electronic structure methods, and first-principles total energy calculations within the density-functional and pseudopotential frameworks. For pressures below a certain critical pressure , the SWNTs' structure remains cylindrical and the Kohn-Sham energy gaps of semiconducting SWNTs have either positive or negative pressure coefficients depending on the value of , with a distinct "family" (of the same ) behavior. The diameter and chirality dependence of the pressure coefficients can be described by a simple analytical expression. At , molecular-dynamics simulations predict that isolated SWNTs undergo a…
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