Chirality Dependence of the Absorption Cross Section of Carbon Nanotubes

Fabien Vialla, Cyrielle Roquelet, Benjamin Langlois, Géraud Delport, Silvia Morim Santos, Emmanuelle Deleporte, Philippe Roussignol, Claude Delalande, Christophe Voisin, and Jean-Sébastien Lauret
Phys. Rev. Lett. 111, 137402 – Published 26 September 2013
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Abstract

The variation of the optical absorption of carbon nanotubes with their geometry has been a long-standing question at the heart of both metrological and applicative issues, in particular because optical spectroscopy is one of the primary tools for the assessment of the chiral species abundance of samples. Here, we tackle the chirality dependence of the optical absorption with an original method involving ultraefficient energy transfer in porphyrin-nanotube compounds that allows uniform photoexcitation of all chiral species. We measure the absolute absorption cross section of a wide range of semiconducting nanotubes at their S22 transition and show that it varies by up to a factor of 2.2 with the chiral angle, with type I nanotubes showing a larger absorption. In contrast, the luminescence quantum yield remains almost constant.

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  • Received 27 April 2013

DOI:https://doi.org/10.1103/PhysRevLett.111.137402

© 2013 American Physical Society

Authors & Affiliations

Fabien Vialla1, Cyrielle Roquelet2,*, Benjamin Langlois1, Géraud Delport2, Silvia Morim Santos2, Emmanuelle Deleporte2, Philippe Roussignol1, Claude Delalande1, Christophe Voisin1,†, and Jean-Sébastien Lauret2

  • 1Laboratoire Pierre Aigrain, École Normale Supérieure, UPMC, Université Paris Diderot, CNRS, 75005 Paris, France
  • 2Laboratoire Aimé Cotton, École Normale Supérieure de Cachan, Université Paris Sud, CNRS, 91405 Orsay, France

  • *Present address: Columbia University, New York, New York, USA.
  • christophe.voisin@lpa.ens.fr

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Issue

Vol. 111, Iss. 13 — 27 September 2013

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