Formation of CN, C3N, and C5N Molecules by Radiative Electron Attachment and their Destruction by Photodetachment

Marjan Khamesian, Nicolas Douguet, Samantha Fonseca dos Santos, Olivier Dulieu, Maurice Raoult, Will J. Brigg, and Viatcheslav Kokoouline
Phys. Rev. Lett. 117, 123001 – Published 13 September 2016

Abstract

The existence of negative ions in interstellar clouds has been associated for several decades with the process of radiative electron attachment. In this Letter, we report compelling evidence supporting the fact that the radiative attachment of a low-energy electron is inefficient to form the carbon chain anions CN, C3N, and C5N detected in interstellar clouds. The validity of the approach is confirmed by good agreement with experimental data obtained for the inverse photodetachment process, which represents the major cause of anion destruction in interstellar space. As a consequence, we suggest alternative models that could explain the formation of anions.

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  • Received 13 April 2016

DOI:https://doi.org/10.1103/PhysRevLett.117.123001

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Atomic, Molecular & OpticalGravitation, Cosmology & Astrophysics

Authors & Affiliations

Marjan Khamesian1, Nicolas Douguet2, Samantha Fonseca dos Santos2, Olivier Dulieu3, Maurice Raoult3, Will J. Brigg4, and Viatcheslav Kokoouline1

  • 1Department of Physics, University of Central Florida, Orlando, Florida 32816, USA
  • 2Department of Physics and Astronomy, Drake University, Des Moines, Iowa 50311, USA
  • 3Laboratoire Aimé Cotton, CNRS, Université Paris-Sud, ENS Cachan, Université Paris-Saclay, bâtiment 505, Campus d’Orsay, 91405 Orsay cedex, France
  • 4Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom

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Issue

Vol. 117, Iss. 12 — 16 September 2016

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