Denser than diamond: Ab initio search for superdense carbon allotropes

Qiang Zhu, Artem R. Oganov, Miguel A. Salvadó, Pilar Pertierra, and Andriy O. Lyakhov
Phys. Rev. B 83, 193410 – Published 26 May 2011; Erratum Phys. Rev. B 83, 239902 (2011)
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Abstract

Diamond has the highest number density (i.e., the number of atoms per unit volume) of all known substances and a remarkably high valence electron density (rws = 0.697 Å). Searching for possible superdense carbon allotropes, we have found three structures (hP3, tI12, and tP12) that have significantly greater density. The hP3 and tP12 phases have strong analogy with two polymorphs of silica (β-quartz and keatite), while the tI12 phase is related to the high-pressure SiS2 polymorph. Furthermore, we found a collection of other superdense structures based on the motifs of the aforementioned structures, but with different ways of packing carbon tetrahedra, and among these the hP3 and tI12 structures are the densest. At ambient conditions, the hP3 phase is a semiconductor with the GW band gap of 3.0 eV, tI12 is an insulator with the band gap of 5.5 eV, while tP12 is an insulator, the band gap of which is remarkably high (7.3 eV), making it the widest-gap carbon allotrope. These allotropes are metastable and have comparable to diamond or slightly higher bulk moduli; their Vickers hardnesses are calculated to be 87.6 GPa for hP3, 87.2 GPa for tI12, and 88.3 GPa for tP12, respectively, thus making these allotropes nearly as hard as diamond (for which the same model gives the hardness of 94.3 GPa). Superdense carbon allotropes are predicted to have remarkably high refractive indices and strong dispersion of light.

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  • Received 12 April 2011
  • Corrected 7 June 2011

DOI:https://doi.org/10.1103/PhysRevB.83.193410

©2011 American Physical Society

Corrections

7 June 2011

Erratum

Publisher’s Note: Denser than diamond: Ab initio search for superdense carbon allotropes [Phys. Rev. B 83, 193410 (2011)]

Qiang Zhu, Artem R. Oganov, Miguel A. Salvado, Pilar Pertierra, and Andriy O. Lyakhov
Phys. Rev. B 83, 239902 (2011)

Authors & Affiliations

Qiang Zhu1,*, Artem R. Oganov1,2, Miguel A. Salvadó3, Pilar Pertierra3, and Andriy O. Lyakhov1

  • 1Department of Geosciences, Department of Physics and Astronomy, and New York Center for Computational Sciences, Stony Brook University, Stony Brook, New York 11794, USA
  • 2Geology Department, Moscow State University, 119992, Moscow, Russia
  • 3MALTA Consolider Team, Departamento de Química Física y Analítica, Universidad de Oviedo, ES-33006, Oviedo, Spain

  • *qiang.zhu@stonybrook.edu

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Issue

Vol. 83, Iss. 19 — 15 May 2011

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