Abstract

We investigated the electronic and structural properties of the infinite linear carbon chain (carbyne) using density functional theory (DFT) and the random phase approximation (RPA) to the correlation energy. The studies are performed in vacuo and for carbyne inside a carbon nano tube (CNT). In the vacuum, semi-local DFT and RPA predict bond length alternations of about 0.04 Å and 0.13 Å, respectively. The frequency of the highest optical mode at the Γ point is 1219 cm-1 and about 2000 cm-1 for DFT and the RPA. Agreement of the RPA to previous high level quantum chemistry and diffusion Monte-Carlo results is excellent. For the RPA we calculate the phonon-dispersion in the full Brillouine zone and find marked quantitative differences to DFT calculations not only at the Γ point but also throughout the entire Brillouine zone. To model carbyne inside a carbon nanotube, we considered a (10,0) CNT. Here the DFT calculations are even qualitatively sensitive to the k-points sampling. At the limes of a very dense k-points sampling, semi-local DFT predicts no bond length alternation (BLA), whereas in the RPA a sizeable BLA of 0.09 Å prevails. The reduced BLA leads to a significant red shift of the vibrational frequencies of about 350 cm-1, so that they are in good agreement with experimental estimates. Overall, the good agreement between the RPA and previously reported results from correlated wavefunction methods and experimental Raman data suggests that the RPA provides reliable results at moderate computational costs. It hence presents a useful addition to the repertoire of correlated wavefunction methods and its accuracy clearly prevails for low dimensional systems, where semi-local density functionals struggle to yield even qualitatively correct results.

Highlights

  • Carbyne – the infinite sp[1] hybridized carbon chain – is a model 1D material with fascinating properties that point to promising applications

  • Since we considered the geometry of the tube to be fixed in its equilibrium state, the chain’s bond length alternation (BLA) is the only structure parameter left that significantly affects the energy of the system

  • The tube induced redshift of the carbyne’s longitudinal optical (LO) G frequency is 346 cmÀ1 at 40 kpc. This value is quite close to the 290 cmÀ1 reported by Wanko et al.,[7] which was obtained by calculating the difference between the theoretical carbyne in vacuo frequency from extrapolated CCSD(T) and the experimentally observed frequencies of long linear carbon chains inside double-wall carbon nano tube (CNT) (DWCNTs)

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Summary

Introduction

Carbyne – the infinite sp[1] hybridized carbon chain – is a model 1D material with fascinating properties that point to promising applications. The very recent introduction of a finite-temperature generalization of the low-scaling RPA algorithms[16] provides an elegant way to treat the partial occupancies that occur due to the charge transfer from the tube to the chain. These prospects lead us to believe that investigating the performance of the RPA for the carbyne–CNT system will yield a valuable contribution to further our knowledge on this intriguing material

Geometries and k-points
Computational details
Phonon frequencies
Preliminary tests
BLA and phonons in vacuo
Method
Conclusion
Full Text
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