Erratum: Relative isomer abundance of fullerenes and carbon nanotubes correlates with kinetic stability (Physical Review Letters (2011) 107 (175506) DOI: 10.1103/PhysRevLett.107.175506)

A. S. Fedorov; D. A. Fedorov; A. A. Kuzubov; P. V. Avramov; Y. Nishimura; S. Irle; Henryk A. Witek

doi:10.1103/PhysRevLett.108.249902

Erratum: Relative isomer abundance of fullerenes and carbon nanotubes correlates with kinetic stability (Physical Review Letters (2011) 107 (175506) DOI: 10.1103/PhysRevLett.107.175506)

A. S. Fedorov, D. A. Fedorov, A. A. Kuzubov, P. V. Avramov, Y. Nishimura, S. Irle, Henryk A. Witek

Waseda Research Institute for Science and Engineering

Research output: Contribution to journal › Comment/debate

1 Citation (Scopus)

Original language	English
Article number	249902
Journal	Physical Review Letters
Volume	108
Issue number	24
DOIs	https://doi.org/10.1103/PhysRevLett.108.249902
Publication status	Published - 2012 Jun 13

ASJC Scopus subject areas

Physics and Astronomy(all)

Cite this

Fedorov, A. S., Fedorov, D. A., Kuzubov, A. A., Avramov, P. V., Nishimura, Y., Irle, S., & Witek, H. A. (2012). Erratum: Relative isomer abundance of fullerenes and carbon nanotubes correlates with kinetic stability (Physical Review Letters (2011) 107 (175506) DOI: 10.1103/PhysRevLett.107.175506). Physical Review Letters, 108(24), [249902]. https://doi.org/10.1103/PhysRevLett.108.249902

Erratum : Relative isomer abundance of fullerenes and carbon nanotubes correlates with kinetic stability (Physical Review Letters (2011) 107 (175506) DOI: 10.1103/PhysRevLett.107.175506). / Fedorov, A. S.; Fedorov, D. A.; Kuzubov, A. A.; Avramov, P. V.; Nishimura, Y.; Irle, S.; Witek, Henryk A.

In: Physical Review Letters, Vol. 108, No. 24, 249902, 13.06.2012.

Research output: Contribution to journal › Comment/debate

Fedorov, AS, Fedorov, DA, Kuzubov, AA, Avramov, PV, Nishimura, Y, Irle, S & Witek, HA 2012, 'Erratum: Relative isomer abundance of fullerenes and carbon nanotubes correlates with kinetic stability (Physical Review Letters (2011) 107 (175506) DOI: 10.1103/PhysRevLett.107.175506)', Physical Review Letters, vol. 108, no. 24, 249902. https://doi.org/10.1103/PhysRevLett.108.249902

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Access to Document

10.1103/PhysRevLett.108.249902